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Turbine Fuel Pump Extreme Teardown

Turbine Fuel Pump
Turbine Fuel Pump

Here’s a destructive teardown of an automotive in-tank turbine fuel pump, used on modern Petrol cars. These units sit in the tank fully immersed in the fuel, which also circulates through the motor inside for cooling. These pumps aren’t serviceable – they’re crimped shut on both ends. Luckily the steel shell is thin, so attacking the crimp joint with a pair of mole grips & a screwdriver allowed me inside.

End Bell
End Bell

The input endbell of the pump has the fuel inlet ports, the channels are visible machined into the casting. There’s a pair of channels for two pump outputs – the main fuel rail to the engine, and an auxiliary fuel output to power a venturi pump. The fuel pump unit sits inside a swirl pot, which holds about a pint of fuel. These are used to ensure the pump doesn’t run dry & starve the engine when the tank level is low & the car is being driven hard. The venturi pump draws fuel from the main tank into the swirl pot. A steel ball is pressed in to the end bell to provide a thrust bearing for the motor armature.

Turbine Impeller
Turbine Impeller

The core of the pump is this impeller, which is similar to a side-channel blower. From what I’ve been able to find these units supply pressures up to about 70PSI for the injector rail. The outside ring is the main fuel pump, while the smaller inner one provides the pressure to run the venturi pump.

Pump Housing
Pump Housing

The other side of the machined pump housing has the main output channel, with the fuel outlet port at the bottom. The motor shaft is supported in what looks like a carbon bearing.

Midsection
Midsection

Removing the pump intermediate section with the bearing reveals quite a bit of fungus – it’s probably been happy sat in here digesting what remains of the fuel.

Armature Exposed
Armature Exposed

Some peeling with mole grips allows the motor to come apart entirely. The drive end of the armature is visible here.

Motor Can
Motor Can

The outer shell of the motor holds yet more fungus, along with some rust & the pair of ceramic permanent magnets.

Brushes
Brushes

The other end of the pump has the brush assembly, and the fuel outlet check valve to the right. The bearing at this end is just the plastic end cap, since there are much lower forces at this end of the motor. The fuel itself provides the lubrication required.

Potted Armature
Potted Armature

With the armature pulled out of the housing, it’s clear that there’s been quite a bit of water in here as well, with the laminations rusting away. This armature is fully potted in plastic, with none of the copper windings visible.

Carbon Commutator
Carbon Commutator

The commutator in these motors is definitely a strange one – it’s axial rather than radial in construction, and the segments are made of carbon like the brushes. No doubt this is to stop the sparking that usually occurs with brushed motors – preventing ignition of fuel vapour in the pump when air manages to get in as well, such as in an empty tank.

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Chinese “1200W” DC-DC Boost Converter DOA Fix

1200W DC-DC Converter
1200W DC-DC Converter

Ah the curse of the Chinese Electronics strikes again. These large DC-DC boost converters have become very common on the likes of AliExpress & eBay, and this time my order has arrived DOA… On applying power, the output LED lights up dimly, and no matter how I twiddle the adjustment pots, the output never rises above the input voltage.

Boost Converter Topology
Boost Converter Topology

From the usual topology above, we can assume that the switching converter isn’t working, so the input voltage is just being directly fed through to the output. The switching IC on these converters is a TL494,

Control Circuitry
Control Circuitry

The switching IC on these converters is a TL494,with it’s surrounding support components, including a LM358 dual Op-Amp. Power for this lot is supplied from the input via a small DC-DC converter controlled by an XL Semi XL7001 Buck Converter IC. Some testing revealed that power was getting to the XL7001, but the output to the switching controller was at zero volts.

Inductor
Inductor

The 100µH inductor for this buck converter is hidden behind the output electrolytic, and a quick prod with a multimeter revealed this inductor to be open circuit. That would certainly explain the no-output situation. Luckily I had an old converter that was burned out. (Don’t try to pull anything near their manufacturer “rating” from these units – it’s utter lies, more about this below).

Donor Converter
Donor Converter

The good inductor from this donor unit has been desoldered here, it’s supposed to be L2. This one had a heatsink siliconed to the top of the TL494 PWM IC, presumably for cooling, so this was peeled off to give some access.
After this inductor was grafted into place on the dead converter, everything sprang to life as normal. I fail to see how this issue wouldn’t have been caught during manufacture, but they’re probably not even testing them before shipping to the distributor.
The sensational ratings are also utter crap – they quote 1.2kW max power, which at 12v input would be 100A. Their max input rating is given as 20A, so 240W max input power. Pulling this level of power from such a cheaply designed converter isn’t going to be reliably possible, the input terminals aren’t even rated to anywhere near 20A, so these would be the first to melt, swiftly followed by everything else. Some of these units come with a fan fitted from the factory, but these are as cheaply made as possible, with bearings made of cheese. As a result they seize solid within a couple of days of use.
Proper converters from companies like TDK-Lambda or muRata rated for these power levels are huge, with BOLTS for terminals, but they’re considerably more expensive. These Chinese units are handy though, as long as they are run at a power level that’s realistic.

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Maplin A24GU Wireless Audio Module Teardown

Transmitter
Transmitter

This is a pair of modules that Maplin was selling some time back, to send stereo audio over a 2.4GHz radio link. The transmitter identifies as a USB sound card, I’ve personally used these units to transmit audio about 60ft. The transmitter, above, has a single button for pairing with the receiver below.

Receiver
Receiver

The receiver unit has a large external antenna, a link status LED & volume buttons, these directly control the volume level on the host PC via the sound card drivers.

Receiver PCB Top
Receiver PCB Top

Popping the case open on the receiver reveals a large PCB, holding the chipset, along with the audio output jacks & Mini-USB power input. The antenna Coax is soldered to the PCB.

Receiver PCB Bottom
Receiver PCB Bottom

The top of the board has the control buttons, and the status LED.

Receiver Chipset
Receiver Chipset

The chipset used here is a Nordic Semiconductor nRF20Z01 2.4GHz Stereo Audio Streamer, there’s a small microcontroller which does all the register magic on the RF transceiver. The RF chain is at the top of the photo, audio outputs on the top left, and the micro USB power input & voltage regulators at bottom left.

Transmitter PCB Top
Transmitter PCB Top

The transmitter PCB has a Sonix USB Audio Codec, to interface with the host PC. This is then fed into another Nordic Semi part on the opposite side of the board:

Transmitter PCB Bottom
Transmitter PCB Bottom

The bottom of the transmitter has the RF section, and another small control microcontroller.

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Blog Housekeeping & More Of The Same

Since I’ve been working on the backend servers a lot over the past few days, I’ve decided it was time to get some broken things on the blog fixed.

Firstly, the radiation monitor graphs. Originally I was using a Raspberry Pi to grab the data from the local monitor, and that was connecting via FTP to the server over in the datacentre to push it’s graph images. Since the server is now on the same local network as the monitor, there’s no need to faff about with FTP servers, so I’ve rejigged things with some perl scripts from cristianst85 over on GitHub, running on the web server itself.
I deviated from the suggested place to put the scripts on the server & opted to store everything within the Experimental Engineering hosting space, so it gets backed up at the same time as everything else on a nightly basis.

This is also accessible from the menu at top left, the script pulls data from the monitor & updates the images every 60 seconds via a cron job.

I’ve removed a couple of dead pages from the blog system, along with some backend tidying of the filesystem. Over the years things have gotten quite messy behind the scenes. This blog is actually getting quite large on disk, I’ve hit the 15GB mark, not including the database!

Caching is enabled for all posts on the blog now, this should help speed things up for repeat visitors, but as most of my content is (large) image based, this might be of limited help. I’m currently tuning the MySQL server for the load conditions, but this takes time, as every time I change some configuration settings I have to watch how things go for a few days, before tweaking some more.

Server Control Panels – More Of The Same

Sorry Sentora. I tried, and failed to convert over to using it as my new server control panel. Unfortunately it just doesn’t give me the same level of control over my systems, so I’ll be sticking with Virtualmin for the foreseeable future. Sentora stores everything in, (to me at least), very odd places under /var/ and gave me some odd results with “www.” versions of websites – some www. hosts would work fine, others wouldn’t at all & just redirect to the Sentora login interface instead. This wasn’t consistient between hosting accounts either, and since I didn’t have much time to get the migration underway, this problem was the main nail in the coffin.

Just storing everything under the sun in /var/ makes life a bit more awkward with the base CentOS install, as it allocates very little space to / by default, (no separate /var partition in default CentOS), giving most of the disk space to /home. Virtualmin on the other hand, stores website public files & Maildirs under /home, saving /var for MySQL databases & misc stuff.

The backup system provided is also utterly useless, there’s no restore function at all, and just piles everything in the account into a single archive. By comparison, Virtualmin has a very comprehensive backup system built in, that supports total automation of the process, along with full automatic restore functionality for when it’s needed.

Sentora did have some good points though:
It handled E-Mail logins & mail filters much more gracefully than Virtualmin does, and comes with Roundcube already built into the interface ready to use. With Virtualmin the options are to use the Usermin side of the system for E-Mail, which I find utterly awful to use, or install a webmail client under one of the hosted domains (my personal choice).
Mail filtering is taken care of with Sieve under Sentora, while Procmail does the job under Virtualmin.

Sentora does have a nicer, simpler, more friendly interface, but it hides most of the low-level system stuff away, while under Virtualmin *everything* on the system is accessible, and it provides control interfaces for all the common server daemons.

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Securing The New Server & Security In General

This was originally going to be part of another post, but it ended up getting more complex than I originally intended so it’s been given it’s own. I go into into many of my personal security practices, on both my public facing servers & personal machines. Since the intertubes are so central to life these days, good security is a must, especially since most people use the ‘net to do very sensitive operations, such as banking, it’s becoming even more essential to have strong security.

Since bringing the new server online & exposing it to the world, it’s been discovered in record time by the scum of the internet, SSH was under constant attack within 24 hours, and within that time there were over 20,000 failed login attempts in the logs.
This isn’t much of an issue, as I’ve got a strong Fail2Ban configuration running which at the moment is keeping track of some 30 IP addresses that are constantly trying to hammer their way in. No doubt these will be replaced with another string of attacks once they realise that those IPs are being dropped. I also prevent SSH login with passwords – RSA keys only here.
MySQL is the other main target to be concerned about – this is taken care of by disabling root login remotely, and dropping all MySQL traffic at the firewall that hasn’t come from 127.0.0.1.

Keeping the SSH keys on an external device & still keeping things simple just requires some tweaking to the .bashrc file in Linux:

This little snippet makes the ssh client look somewhere else for the keys themselves, while keeping typing to a minimum in the Terminal. This assumes the external storage with the keys always mounts to the same location.

Everything else that can’t be totally blocked from outside access (IMAP, SMTP, FTP, etc), along with Fail2Ban protection, gets very strong passwords, unique to each account, (password reuse in any situation is a big no-no) and where possible TOTP-based two factor authentication is used for front end stuff, all the SSH keys, master passwords & backup codes are themselves kept offline, on encrypted storage, except for when they’re needed. General password management is taken care of by LastPass, and while they’ve been subject to a couple of rather serious vulnerabilities recently, these have been patched & it’s still probably one of the best options out there for a password vault.
There’s more information about those vulnerabilities on the LastPass blog here & here.


This level of security paranoia ensures that unauthorized access is made extremely difficult – an attacker would have to gain physical access to one of my mobile devices with the TOTP application, and have physical access to the storage where all the master keys are kept (along with it’s encryption key, which is safely stored in Meatware), to gain access to anything.
No security can ever be 100% perfect, there’s always going to be an attack surface somewhere, but I’ll certainly go as far as is reasonable, while not making my access a total pain, to keep that attack surface as small as possible,and therefore keeping the internet scum out of my systems.
The last layer of security is a personal VPN server, which keeps all traffic totally encrypted while it’s in transit across my ISP’s network, until it hits the end point server somewhere else in the world. Again, this isn’t perfect, as the data has to be decrypted *somewhere* along the chain.

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Philips LED PAR38 Lamp Teardown

Philips PAR38
Philips PAR38

These large LED Philips PAR38 lamps were recently on clearance sale in my local T.N. Robinsons electrical contractors for about £3, so I decided to grab one in the hopes I might be able to hack it into a low-voltage LED lamp. These are full-size PAR38 format, with most of the bulk being the large aluminium heatsink on the front. The back section with the power supply module is secured with silicone, so some unreasonable force was required to liberate the two pieces.

Specification
Specification

These lamps are rated at 18W in operation, and are surprisingly bright for this power level.

Lens
Lens

The front has the moulded multi-lens over the LEDs, to spread the light a bit further than the bare dies.

LED Array
LED Array

The LED array is two series strings of 4 LEDs, for ~24v forward voltage. Unusual for a high power LED array, this PCB isn’t aluminium cored, but 0.8mm FR4. Heat is transferred to the copper plane on the backside by the dozens of vias around the Luxeon Rebel LEDs. There is a thermal pad under the PCB for improved heat transfer to the machined surface of the heatsink.

Control PCB Top
Control PCB Top

The power supply & control PCB is pretty well made, it’s an isolated converter, so no nasty mains on the LED connections.

Control PCB Bottom
Control PCB Bottom
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IC Decap – TDA3606 Multi Regulator With Battery Sense

This is a chip aimed at the automotive market – this is a low power voltage regulator for supplying power to microcontrollers, for instance in a CD player.

TDA3606 Die
TDA3606 Die

The TDA3606 is a voltage regulator intended to supply a microprocessor (e.g. in car radio applications). Because of low voltage operation of the application, a low-voltage drop regulator is used in the TDA3606. This regulator will switch on when the supply voltage exceeds 7.5 V for the first time and will switch off again when the output voltage of the regulator drops below 2.4 V. When the regulator is switched on, the RES1  and RES2 outputs (RES2 can only be HIGH when RES1 is HIGH) will go HIGH after a fixed delay time (fixed by an external delay capacitor) to generate a reset to the microprocessor. RES1 will go HIGH by an internal pull-up resistor of 4.7 kΩ, and is used to initialize the microprocessor. RES2 is used to indicate that the regulator output voltage is within its voltage range. This start-up feature is built-in to secure a smooth start-up of the microprocessor at first connection, without uncontrolled switching of the regulator during the start-up sequence. All output pins are fully protected. The regulator is protected against load dump and short-circuit (foldback
current protection). Interfacing with the microprocessor can be accomplished by means of a battery Schmitt-trigger and output buffer (simple full/semi on/off logic applications). The battery output will go HIGH when the battery input voltage exceeds the HIGH threshold level.

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nb Tanya Louise Heating System – Oxide Sludge

I wrote a few weeks ago about replacing the hot water circulating pump on the boat with a new one, and mentioned that we’d been through several pumps over the years. After every replacement, autopsy of the pump has revealed the failure mode: the first pump failed due to old age & limited life of carbon brushes. The second failed due to thermal shock from an airlock in the system causing the boiler to go a bit nuts through lack of water flow. The ceramic rotor in this one just cracked.
The last pump though, was mechanically worn, the pump bearings nicely polished down just enough to cause the rotor to stick. This is caused by sediment in the system, which comes from corrosion in the various components of the system. Radiators & skin tanks are steel, engine block cast iron, back boiler stainless steel, Webasto heat exchanger aluminium, along with various bits of copper pipe & hose tying the system together.
The use of dissimilar metals in a system is not particularly advisable, but in the case of the boat, it’s unavoidable. The antifreeze in the water does have anti-corrosive additives, but we were still left with the problem of all the various oxides of iron floating around the system acting like an abrasive. To solve this problem without having to go to the trouble of doing a full system flush, we fitted a magnetic filter:

Mag Filter
Mag Filter

This is just an empty container, with a powerful NdFeB magnet inserted into the centre. As the water flows in a spiral around the magnetic core, aided by the offset pipe connections, the magnet pulls all the magnetic oxides out of the water. it’s fitted into the circuit at the last radiator, where it’s accessible for the mandatory maintenance.

Sludge
Sludge

Now the filter has been in about a month, I decided it would be a good time to see how much muck had been pulled out of the circuit. I was rather surprised to see a 1/2″ thick layer of sludge coating the magnetic core! The disgusting water in the bowl below was what drained out of the filter before the top was pulled. (The general colour of the water in the circuit isn’t this colour, I knocked some loose from the core of the filter while isolating it).

If all goes well, the level of sludge in the system will over time be reduced to a very low level, with the corrosion inhibitor helping things along. This should result in much fewer expensive pump replacements!

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eBay Flyback High Voltage PSU

Flyback PSU
Flyback PSU

I have found myself needing some more in the way of High Voltage supplies of late, with the acquisition of the new He-Ne laser tubes, so I went trawling eBay for something that would be suitable to run these tubes. (I currently only have a single He-Ne laser PSU brick, and they’re notoriously hard to find & rather expensive).
This supply is rated at 1kV-10kV output, at 35W power level. Unfortunately this supply isn’t capable of sustaining the discharge in a large He-Ne tube, the impedance of the supply is far too high. Still, it’s useful for other experiments.
The flyback-type transformer clearly isn’t a surplus device from CRT manufacture, as there are very few pins on the bottom, and none of them connect to the primary side. The primary is separately wound on the open leg of the ferrite core.

Drive Electronics
Drive Electronics

The drive electronics are pretty simple, there’s a controller IC (with the number scrubbed off – guessing it’s either a 556 dual timer or a SMPS controller), a pair of FDP8N50NZ MOSFETs driving the centre-tapped primary winding.
The drive MOSFETs aren’t anything special in this case: they’re rated at 500v 8A, 850mΩ on resistance. This high resistance does make them get rather hot even with no load on the output, so for high power use forced-air cooling from a fan would definitely be required.

Test Setup
Test Setup

Here’s the supply on test, I’ve got the scope probes connected to the gate resistors of the drive MOSFETs.

Waveforms
Waveforms

On the scope the primary switching waveforms can be seen. The FETs operate in push-pull mode, there’s a bit of a ring on the waveform, but they’re pretty nice square waves otherwise.

Arc
Arc

At maximum power on 12v input, about 25mm of gap is possible with an arc.

Viewing Spectral Lines in Discharge, Other Colours in Output

For accurate measurements, you’ll need an optical instrument such as a monochromator or spectrophotometer or optical spectrum analyzer. But to simply see the complexity of the discharge spectrum inside the bore of a He-Ne laser tube, it’s much easier and cheaper.

(Spectra for various elements and compounds can be easily found by searching the Web. The NIST Atomic Spectra Database has an applet which will generate a table or plot of more spectral lines than you could ever want.)

Instant Spectroscope for Viewing Lines in He-Ne Discharge

It is easy to look at the major visible lines. All it takes is a diffraction grating or prism. I made my instant spectroscope from the diffraction grating out of some sort of special effects glasses – found in a box of cereal, no less! – and a monocular (actually 1/2 of a pair of binoculars).

  • If you missed the Kellogg’s option, diffraction gratings can be purchased from places like Edmund Scientific. You don’t need anything fancy – any of the inexpensive ‘transmission replica gratings’ on a flat rigid substrate or mounted between a pair of plane glass plates will be fine. In a pinch, a CD disc or other optical media will work but only as a reflection grating so mounting may be a problem. A spectroscope can also be made with a prism of course but a diffraction grating is likely to be less expensive and better for this application since it is much lighter and easier to mount.
  • The plasma tube of a bare He-Ne laser is an ideal light source since it provides its own slit as the glow discharge is confined to the long narrow capillary bore. However, this approach can also be used with other lasers as long as the beam can be focused to a spot on a wall or screen. This will produce a ‘bright spot spectra’ instead of politically correct lines but you can’t have everything. 🙂
  • The diffraction grating can be used by itself but the additional optics will provide magnification and other benefits for people with less than perfect eyeballs.
  • Glue the diffraction grating to a cardboard sleeve that can be slipped over the (or one) objective of a monocular, binocular, or small telescope – or the telephoto lens of your camera. Orient it so that the dispersion will be vertical (since your slit will be horizontal).
  • Operate the HeNe tube on a piece of black velvet or paper. This will result in optimum contrast. This is best done in a darkened room where the only source of light is the laser tube itself. Just don’t trip and zap yourself on the high voltage!
  • A diffraction grating produces several images. The zero’th order will be the original image seen straight ahead. The important ones are the first order spectra. Tip the instrument up or down to see these. The dispersion direction – order of the colours – will depend on which way it is tipped.
  • Any distance beyond the closest focus of your instrument will work but being further away will reduce the effective width of the ‘slit’ resulting in the ability to distinguish more closely spaced lines.

The shear number of individual spectral lines present in the discharge is quite amazing. You will see the major red, orange, yellow, and green lines as well as some far into the blue and violet portions of the spectrum and toward the IR as well.

Bright Line Spectra of Helium and Neon
Bright Line Spectra of Helium and Neon

All of those shown will be present as well as many others not produced by the individual gas discharges. There are numerous IR lines as well but, of course, these will not be visible.

Place a white card in the exit beam and note where the single red output line of the He-Ne tube falls relative to the position and intensity of the numerous red lines present in the gas discharge.

As an aside, you may also note a weak blue/green haze surrounding the intense main red beam (not even with the spectroscope). This is due to the blue/green (incoherent) spectral lines in the discharge being able to pass through the output mirror which has been optimized to reflect well (>99 percent) at 632.8 nm and is relatively transparent at wavelengths some distance away from these (shorter and longer but you would need an IR sensor to see the longer ones). Since it is not part of the lasing process, this light diverges rapidly and is therefore only visible close to the tube’s output mirror.

Dynamic Measurement of Discharge Spectra

The following is trivial to do if you have a recording spectrometer and external mirror He-Ne laser. For an internal mirror He-Ne laser tube, it should be possible to rock one of the mirrors far enough to kill lasing without permanently changing alignment. If you don’t have proper measuring instruments, don’t worry, this is probably in the “Gee wiz, that’s neat but of marginal practical use” department. 🙂

(From: George Werner (glwerner@sprynet.com).)

Here is an effect I found many years ago and I don’t know if anyone has pursued it further.

We had a recording spectrometer in our lab which we used to examine the incoherent light coming from the laser discharge. This spectrum when lasing was slightly different from the spectrum when not lasing, which one can expect since energy levels are redistributed. As with most detectors, ours used a chopper in the spectrometer light beam and a lock-in amplifier.

Instead of putting the chopper in the path of light going to the spectrometer, I put it in the path of the internal laser beam, so that instead of an open/closed signal going to the amplifier it was a lasing/not-lasing signal. What was recorded then was three kinds of spectrum lines: some deflected positive in the normal way, others deflected negative, and the third group were those that were unaffected by chopping, in which case when we passed over the line we only saw an increase in the noise level. Setting up such a test is easy. The hard part is interpreting the data in a meaningful way.

Other Colour Lines in Red He-Ne Laser Output

When viewing spectral lines in the actual beam of a red He-Ne laser, you may notice some very faint ones far removed from the dominant 632.8 nm line we all know and love. (This, of course, also applies to other colour He-Ne lasers.)

For He-Ne lasers, the primary line (usually 632.8 nm) is extremely narrow and effectively a singularity given any instrumentation you are likely to have at your disposal. Any other lines you detect in the output are almost certainly from two possible sources but neither is actual laser emission:

  • Plasma discharge – there are many strong emission lines in the actual discharge – and none of them are actually at the 632.8nm lasing wavelength! These extend from the mid-IR through the violet.Close to the output mirror, you may see some of this light seeping through especially at wavelengths in the green, blue, and violet, for which the dielectric mirrors are nearly perfectly transparent. However, such light will be quite divergent and diffuse and won’t be visible at all more than a couple of inches from the mirror.
  • Superradiance – As we know, He-Ne lasers can be made to operate at a variety of wavelengths other than the common 632.8nm red. The physics for these is still applicable in a red He-Ne tube but the mirrors do not have the needed reflectivity at these other wavelengths and therefore the resonator gain is too low to support true laser action. However, stimulated emission can still take place in superradiance mode – one pass down the tube and out, exiting easily for the green wavelength in particular since the dielectric mirrors are quite transparent in that region of the spectrum.The result will be a weak green beam that can sometimes be observed with a spectroscope in a very dark room room. It isn’t really quite as coherent or monochromatic as the beam from a true green He-Ne laser and probably has much wider divergence but nonetheless may be present. It may be easier to see this by using your spectroscope to view the bright spot from the laser on a white card rather than by deflecting the beam and trying to locate the green dot off to one side.Note: I have not been able to detect this effect on the short He-Ne tubes I have checked.

Since the brightness of the discharge and superradiance output should be about the same from either mirror, using the non-output end (high reflector) should prove easier (assuming it isn’t painted over or otherwise covered) since the red beam exiting from this mirror will be much less intense and won’t obscure the weak green beam.

Note that argon and krypton ion lasers are often designed for multiline output where all colours are coherent and within an order of magnitude of being equal to each other in intensity or with a knob to select an individual wavelength. Anything like this is only rarely done with He-Ne lasers because it is very difficult (and expensive) due to the low gain of the non-red lines.

Internal Mirror He-Ne Tubes up to 35 mW – Red and Other Colours

Typical He-Ne Tube Specifications

Prior to the introduction of the CD player, the red He-Ne laser was by far the most common source of inexpensive coherent light on the planet. The following are some typical physical specifications for a variety of red (632.8 nm) He-Ne tubes (all are single transverse mode – TEM00):

Where:

  • Power Output is the minimum beam power after a specified warm up period over the spec’d life of the tube.
  • Tube Operating Voltage is the voltage across the bare tube at the nominal operating current.
  • Tube Start Voltage is the minimum voltage across the bare tube required to guarantee starting.
  • Tube Size is generally the maximum diameter of the tube envelope and the total length from the outer surfaces of the mirrors.

Tubes like this are generally available in both random and linearly polarized versions which are otherwise similar with respect to the above characteristics (for red tubes at least, more below).

At least one other basic specification may be critical to your application: Which end of the tube the beam exits! There is no real preference from a manufacturing point of view for red He-Ne lasers. (For low gain “other-colour” He-Ne laser tubes, it turns out that anode output results is slightly higher gain and thus slightly higher output for the typical hemispherical cavity because it better utilizes the mode volume.) However, this little detail may matter a great deal if you are attempting to retrofit an existing barcode scanner or other piece of equipment where the tube clips into a holder or where wiring is short, tight, or must be in a fixed location. For example, virtually all cylindrical laser heads require that the beam exits from the cathode-end of the tube. It is possible that you will be able to find two versions of many models of He-Ne tubes if you go directly to the manufacturer and dig deep enough. However, this sort of information may not be stated where you are buying surplus or from a private individual, so you may need to ask.

The examples above (as well as all of the other specifications in this and the following sections) are catalog ratings, NOT what might appear on the CDRH safety sticker (which is typically much higher). See the section: About Laser Power Ratings for info on listed, measured, and CDRH power ratings.

Note how some of the power levels vary widely with respect to tube dimensions, voltage, and current. Generally, higher power implies a longer tube, higher operating/start voltages, and higher operating current – but there are some exceptions. In addition, you will find that physically similar tubes may actually have quite varied power output. This is particularly evident in the manufacturers’ listings. (See the chapter: A HREF=”laserhcl.htm#hcltoc”>Commercial Unstabilized HeNe Lasers.)

These specifications are generally for minimum power over the guaranteed life of the tube. New tubes and individual sample tubes after thousands of hours may be much higher – 1.5X is common and a “hot” sample may hit 2X or more. My guess is that for tubes with identical specifications in terms of physical size, voltage, and current, the differences in power output are due to sample-to-sample variations. Thus, like computer chips, they are selected after manufacture based on actual performance and the higher power tubes are priced accordingly! This isn’t surprising when considering the low efficiency at which these operate – extremely slight variations in mirror reflectivity and trace contaminants in the gas fill can have a dramatic impact on power output.

I have a batch of apparently identical 2 mW Aerotech tubes that vary in power output by a factor of over 1.5 to 1 (2.6 to 1.7 mW printed by hand on the tubes indicating measured power levels at the time of manufacture).

And, power output also changes with use (and mostly in the days of soft-sealed tubes, just with age sitting on the shelf):

(From: Steve Roberts.)

“I have a neat curve from an old Aerotech catalogue of He-Ne laser power versus life. The tubes are overfilled at first, so power is low. They then peak at a power much higher than rated power, followed by a long period of constant power, and then they SLOWLY die. It’s not uncommon for a new He-Ne tube to be in excess of 15% greater than rated power.”

And the answer to your burning question is: No, you cannot get a 3 mW tube to output 30 mW – even instantaneously – by driving it 10 times as hard!

I have measured the operating voltage and determined the optimum current (by maximizing beam intensity) for the following specific samples – all red (632.8 nm) tubes from various manufacturers. (The starting voltages were estimated.):

Melles Griot, Uniphase, Siemens, PMS, Aerotech, and other HeNe tubes all show similar values.

The wide variation in physical dimensions also means that when looking at descriptions of He-Ne lasers from surplus outfits or the like, the dimensions can only be used to determine an upper (and possibly lower) bound for the possible output power but not to determine the exact output power (even assuming the tube is in like-new condition). Advertisements often include the rating on the CDRH safety sticker (or say ‘max’ in fine print). This is an upper bound for the laser class (e.g., Class IIIa), not what the particular laser produces or is even capable of producing. It may be much lower. For example, that Class IIIa laser showing 5 mW on the sticker, may actually only be good for 1 mW under any conditions! The power output of a He-Ne laser tube is essentially constant and cannot be changed significantly by using a different power supply or by any other means. See the section: Buyer Beware for Laser Purchases.

Also see the section: Locating Laser Specifications.

In addition to power output, power requirements, and physical dimensions, key performance specifications for He-Ne lasers also include:

  • Beam Diameter at the laser’s output aperture and beam profile (Gaussian TEM00 for most small He-Ne laser tubes).
  • Beam Divergence (probably far field ignoring beam waist). Note that this may not always be the same as the expected value from the diffraction limit based on beam/bore diameter as it also depends on the combination of the HR and OC mirror (inside) curvature and the shape of the exterior surface of the OC.
  • Mode Spacing (frequency) between the multiple longitudinal modes that are active simultaneously in all but single mode frequency stabilized lasers.

With manufacturers like Aerotech, Melles Griot, and Siemens, a certain amount of information can be determined from the model number. For example, here is how to decipher most of those from Melles Griot (e.g., 05-LHP-121-278):

  • All Melles Griot He-Ne laser tubes and power supplies start with 05. Matched systems may start with 25 (e.g., laser head and lab-style power supply).
  • The first letter will be an L for all He-Ne laser tubes and heads except for perpendicular window terminated tubes (in which case it will be W – this is inconsistent with the rest of their numbering but who am I to complain!), and some of their self contained lasers where it will be S.
  • The second letter will be one of: H = red (632.8 nm), G = green (543.5 nm), Y = yellow (594.1 nm), O = orange (611.9 nm), or I = infra-red (1,523 or 3,391 nm). A couple of self contained red lasers use R for red but for most, I guess they got stuck using H (presumably denoting He-Ne) before ‘other colour’ He-Ne lasers were part of their product line. And, their stabilized He-Ne lasers use a T here. Confused yet? 🙂
  • The third letter will be one of: R = Randomly polarized, L = linearly polarized, or B = Brewster window at one or both ends.
  • The following three digit number determines the physical characteristics of the laser tube to some extent. Unfortunately, there may be no direct mathematical relationship of this number to anything useful. As will be seen below, for some models, it (or some of its digits) sort of correlates with output power or length but for others, they might as well be totally random! However, it does appear as though an identical set of numbers among different colour tubes (see below) will denote similar physical size tubes at least.
  • If there are additional numbers, they relate to a special variation on the basic design done for a particular customer. For example, this might be a different curvature on the outer surface of the output mirror to provide a non-standard divergence to eliminate the need for an additional lens in a barcode scanner. Or, an external window for protection from the elements or to deliberately reduce output power. Go figure. 🙂 It may also just denote a specific configuration like -249 (meaning 115 VAC operation, kind of arbitrary, huh?) or -55 (meaning 5.5 mA). In these cases, the user may be able to modify the settings (flip a switch or twiddle a pot) but the warranty may then be void.

The vast majority of Melles Griot lasers you are likely to come across will follow this numbering scheme though there are some exceptions, especially for custom assemblies. (Some surplus places drop the leading ’05-‘ when reselling Melles Griot laser tubes or heads so an 05-LHP-120 would become simply an LHP-120.)

For other manufacturers like Spectra-Physics, the model numbers are totally arbitrary!

He-Ne Tubes of a Different Colour

Although a red beam is what everyone thinks of when a He-Ne laser is discussed, He-Ne tubes producing green, yellow, and orange beams, as well as several infra-red (IR) wavelengths, are also manufactured. However, they are not found as often on the surplus market because they are not nearly as common as the red variety. In terms of the number of He-Ne lasers manufactured, red is far and away the most popular, with all the others combined accounting for only 1 to 2 percent of the total production. In order of decreasing popularity, it’s probably: red, green, yellow, infra-red (all IR wavelengths), orange. Non-red tubes are also more expensive when new since for a given power level, they must be larger (and thus have higher voltage and current ratings) due to their lower efficiency (the spectral lines being amplified are much weaker than the one at 632.8 nm). Operating current for non-red He-Ne tubes is also more critical than for the common red variety so setting these up with an adjustable power supply or adjusting the ballast resistance for maximum output is recommended.

Maximum available power output is also lower – rarely over 2 mW (and even those tubes are quite large (see the tables below). However, since the eye is more sensitive to the green wavelength (543.5 nm) compared to the red (632.8 nm) by more than a factor of 4, a lower power tube may be more than adequate for many applications. Yellow (594.1 nm) and orange (611.9 nm) He-Ne lasers appear more visible by factors of about 3 and 2 respectively compared to red beams of similar power.

Infrared-emitting He-Ne lasers exist as well. In addition to scientific uses, these were used for testing in the Telecom industry before sufficiently high quality diode lasers became available.Yes, you can have a He-Ne tube and it will light up inside (typical neon glow), but if there is no output beam (at least you cannot see one), you could have been sold an infrared He-Ne tube. However, by far the most likely explanation for no visible output beam is that the mirrors are misaligned or the tube is defective in some other way. Unfortunately, silicon photodiodes or the silicon sensors in CCD or CMOS cameras do not respond to any of the He-Ne IR wavelengths, so the only means of determining if there is an IR beam are to use a GaAs photodiode, IR detector card, or thermal laser power meter. IR He-Ne tubes are unusual enough that it is very unlikely you will ever run into one. However, they may turn up on the surplus market especially if the seller doesn’t test the tubes and thus realize that these behave differently – they are physically similar to red (or other colour) He-Ne tubes except for the reflectivity of the mirrors as a function of wavelength. (There may be some other differences needed to optimize each color like the He:Ne ratio, isotope purity, and gas fill pressure, but the design of the mirrors will be the most significant factor and the one that will be most obvious with a bare eyeball, though the color of the discharge may be more pink for green He-Ne tubes and more orange and brighter for IR He-Ne tubes compared to red ones, more below.) Even if the model number does not identify the tube as green, yellow, orange, red, or infra-red, this difference should be detectable by comparing the appearance of its mirrors (when viewed down the bore of an UNPOWERED tube) with those of a normal (known to be red) He-Ne tube. (Of course, your tube could also fail to lase due to misaligned or damaged mirrors or some other reason.

As noted above, the desired wavelength is selected and the unwanted wavelengths are suppressed mostly by controlling the reflectivity functions of the mirrors. For example, the gains of the green and yellow lines (yellow may be stronger) are both much much lower than red and separated from each other by about 50 nm (543.5 nm versus 594.1 nm). To kill the yellow line in a green laser, the mirrors are designed to reflect green but pass yellow. I have tested the mirrors salvaged from a Melles Griot 05-LGP-170 green He-Ne tube (not mine, from “Dr. Destroyer of Lasers”). The HR (High Reflector) mirror has very nearly 100% reflectivity for green but less than 25% for yellow. The OC (Output Coupler) also has a low enough reflectivity for yellow (about 98%) such that it alone would prevent yellow from lasing. The reflectivities for orange, red, and IR, are even lower so they are also suppressed despite their much higher gain, especially for the normal red (632.8 nm) and even stronger mid-IR (3,391 nm) line.

However, to manufacture a tube with optimum and stable output power, it isn’t sufficient to just kill lasing for unwanted lines. The resonator must be designed to minimize their contribution to stimulated emission – thus the very low reflectivity of the HR for anything but the desired green wavelength. Otherwise, even though sustained oscillation wouldn’t be possible, unwanted colour photons would still be bouncing back and forth multiple times stealing power from the desired colour. The output would also be erratic as the length of the tube changed during warm up (due to thermal expansion) and this affected the longitudinal mode structure of the competing lines relative to each other. Some larger He-Ne lasers have magnets along the length of the tube to further suppress (mostly) the particularly strong mid-IR line at 3,391 nm. (See the section: Magnets in High Power or Precision HeNe Laser Heads.)

In addition, you can’t just take a tube designed for a red laser, replace the mirrors, and expect to get something that will work well – if at all – for other wavelengths. For one thing, the bore size and mirror curvature for maximum power while maintaining TEM00 operation are affected by wavelength.

Furthermore, for these other colour He-Ne lasers which depend on energy level transitions which have much lower gain than red – especially the yellow and green ones – the gas fill pressure, He:Ne ratio, and isotopic composition and purity of the helium and neon, will be carefully optimized and will be different than for normal red tubes.

Needless to say, the recipes for each type and size laser will be closely guarded trade secrets and only a very few companies have mastered the art of other colour He-Ne lasers, especially for high power (in a relative sort of way) in yellow and green. I am only aware of four companies that currently manufacture their own tubes: Melles Griot, Research Electro-Optics, Uniphase, and LASOS, with the last two having very few models to choose from. Others (like Coherent) simply resell lasers under their own name.

And, the answer to that other burning question should now be obvious: No, you can’t convert an ordinary red internal mirror He-Ne tube to generate some other colour light as it’s (almost) all done with mirrors and they are an integral part of the tube. 🙂 Therefore, your options are severely limited. As in: There are none. (However, going the other way, at least as a fun experiment, may be possible. For a laser with external mirrors, a mirror swap may be possible (though the cavity length may be insufficient to resonate with the reduced gain of other-colour spectral lines once all loses taken into consideration). But realistically, this option doesn’t even exist where the mirrors are sealed into the tube.

There are also a few He-Ne lasers that can output more than one of the possible colors simultaneously (e.g., red+orange, orange+yellow) or selectively by turning knob (which adjusts the angle of a Littrow or other similar dispersion prism) inside the laser cavity using a Brewster window He-Ne tube). But such lasers are not common and are definitely very expensive. So, you won’t likely see one for sale at your local hamfest – if ever! One manufacturer of such lasers is Research Electro-Optics (REO). See the section: Research Electro-Optics’s Tunable HeNe Lasers.

However, occasionally a He-Ne tube turns up that is ‘defective’ due to incorrect mirror reflectivities or excessive gain or magic 🙂 and actually outputs an adjacent colour in addition to what it was designed to produce. I have such a tube that generates about 3 mW of yellow (594.1 nm) and a fraction of a mW of orange (611.9 nm) but isn’t very stable – power fluctuates greatly as it warms up. Another one even produces the other orange line at 611.9 nm, and it’s fairly stable. But, finding magic ‘defective’ tubes such as these by accident is extremely unlikely though I’ve heard of the 640.1 nm (deep red) line showing up on some supposedly good normal red (632.8 nm) He-Ne tubes.

As a side note: It is strange to see the more or less normal red-orange glow in a green He-Ne laser tube but have a green beam emerging. A diffraction grating or prism really shows all the lines that are in the glow discharge. Red through orange, yellow and green, even several blue lines (though they are from the helium and can’t lase under any circumstances)!! The IR lines are present as well – you just cannot see them.

Actually, the colour of the discharge may be subtly different for non-red He-Ne tubes due to modified gas fill and pressure. For example, the discharge of green He-Ne tubes may appear more pink compared to red tubes) which are more orange), mostly due to lower fill pressure. The fill mix and pressure on green He-Ne tubes is a tricky compromise among several objectives that conflict to some extent including lifetime, stability (3.39µm competition), and optical noise. This balancing act and the lower fill pressure are why green He-Ne tubes don’t last as long as reds. Have I totally confused you, colour-wise? 🙂

The expected life of ‘other colour’ He-Ne tubes is generally much shorter than for normal red tubes. This is something that isn’t widely advertised for obvious reasons. Whereas red He-Ne tubes are overfilled initially (which reduces power output) and they actually improve with use to some extent as gas pressure goes down, this luxury isn’t available with the low gain wavelengths – especially green – everything needs to be optimal for decent performance.

The discharge in IR He-Ne tubes may be more orange and brighter due to a higher fill pressure. Again, this is due to the need to optimize parameters for the specific wavelength.

Determining He-Ne Laser Colour from the Appearance of the Mirrors

Although most He-Ne lasers are the common red (632.8 nm) variety (whose beam actually appears orange-red), you may come across unmarked He-Ne tubes and just have to know what colour output the produce without being near a He-Ne laser power supply.

Since the mirrors used in all He-Ne lasers are dielectric – functioning as a result of interference – they have high reflectivity only around the laser wavelength and actually transmit light quite well as the wavelength moves away from this peak. By transmitted light, the appearance will tend to be a colour which is the complement of the laser’s output – e.g., cyan or blue-green for a red tube, pink or magenta for a green tube, blue or violet for a yellow tube. Of course, except for the IR variety, if the tube is functional, the difference will be immediately visible when it is powered up!

The actual appearance may also depend on the particular manufacturer and model as well as the length/power output of the laser (which affects the required reflectivity of the OC), as well as the revision number of your eyeballs. 🙂 So, there could be considerable variation in actual perceived colour. Except for the blue-green/magenta combination which pretty much guarantees a green output He-Ne tube, more subtle differences in colour may not indicate anything beyond manufacturing tolerances.

Appearance of He-Ne Laser Mirrors
Appearance of He-Ne Laser Mirrors

The chart above in conjunction with will help to identify your unmarked He-Ne tube. (For accurate rendition of the graphic, your display should be set up for 24 bit colour and your monitor should be adjusted for proper colour balance.)

The entry labelled ‘Broadband’ relates to the HR mirror in some unusual multiple colour (combinations of red and/or orange and/or yellow) internal mirror tubes as well as those with an internal HR and Brewster window for external OC optics. And, the yellow and orange tubes may actually use broad band HRs. The OCs would then be selected for the desired wavelength(s) and may also have a broad band coating.

For low gain tubes, they play games with the coatings. I guess it isn’t possible to just make a highly selective coating for one wavelength that’s narrow enough to have low reflectivity at the nearby lines so they won’t lase. So, one mirror will be designed to fall off rapidly on one side of the design wavelength, the other mirror on the other side. That’s one reason front and back mirrors on yellow and green tubes in particular have very different appearances.

As noted, depending on laser tube length/output power, manufacturer, and model, the appearance of the mirrors can actually vary quite a bit but this should be a starting point at least. For example, I have a Melles Griot 05-LHR-170 He-Ne laser tube that should be 594.1 nm (yellow) but actually outputs some 604.6 nm (orange) as well. It’s mirror colours for the HR and OC are almost exactly opposite of those I have shown for the yellow and orange tubes! I don’t know whether this was intentional or part of the problem And, while from this limited sample, it looks like the OCs for orange, yellow, and green He-Ne lasers appear similar, I doubt that they really are in the area that counts – reflectivity/transmission at the relevant wavelengths.

More on Other Colour He-Ne Lasers

Here are some comments on the difficulty of obtaining useful visible output from He-Ne lasers at wavelengths other than our friendly red (632.8 nm):

(From: Steve Roberts.)

You do need a isotope change in the gases for green, and a He:Ne ratio change for the other orange and yellow lines. In addition, the mirrors to go to another line will have a much lower output transmission. The only possible lines you’ll get on a large frame He-Ne laser will be the 611.9 nm orange and 594.1 nm yellow. The green requires external mirror tubes in excess of a meter and a half long and a Littrow prism to overcome the Brewster losses and suppress the IR.

The original work on green was done by Rigden and Wright. The short tubes have lower losses because they have no Brewsters and thus can concentrate on tuning the coatings to 99.9999% reflectivity and maximum IR transmission. There is one tunable low power unit on the market that does 6 lines or so, but only 1 line at a time, and the $6,000 cost is kind of prohibitive for a few milliwatts of red and fractional milliwatt powers on the other lines. But, it will do green and has the coatings on the back side of the prism to kill the losses.

Also look for papers by Erkins and Lee. They are the fellows who did the green and yellow for Melles Griot and they published one with the energy states as part of a poster session at some conference. Melles Griot used to hand it out, that’s how I had a copy, recently thrown away.

Even large He-Ne lasers such as the SP-125 (rated at 50mW of red) will only do about 20mW of yellow, with a 35mW SP-127 you’re probably only looking at 3 to 5mW of yellow. And, for much less then the cost of the custom optics to do a conversion, you can get two or three 4 to 5 mW yellow heads from Melles Griot. I know for a fact that a SP-127 only does about 3mW of 611.9 with a external prism and a remote cavity mirror, when it does 32mW of 632.8nm.

So in the end, unless you have a research use for a special line, it’s cheaper to dig up a head already made for the line you seek, unless you have your own optics coating lab that can fabricate state-of-the-art mirrors.

I have some experience in this, as I spent months looking for a source of the optics below $3,000.

(From: Sam.)

I do have a short (265 mm) one-Brewster He-Ne tube (Melles Griot 05-LGB-580) with its internal HR optimized for green that operates happily with a matching external green HR mirror (resulting in a nice amount of circulating power) but probably not with anything having much lower reflectivity to get a useful output beam. In fact, I could not get reliable operation even with the HR from a dead green He-Ne laser tube as the Brewster window would not remain clean enough for the time required to align the mirror.

I would expect an SP-127 to do more than 3 to 5 mW of yellow, my guess would be 10 to 15 mW with optimized mirrors but no tuning prism. If I can dig up appropriate mirrors, I intend to try modifying an SP-127 to make it tunable and/or do yellow or green. 🙂

(From: Lynn Strickland (stricks760@earthlink.net).)

You can find 640.1 nm in a lot of red He-Ne lasers. I have a paper on it somewhere, and cavity design can influence it to a large extent. If you have a decent quality grating, it’s pretty easy to pick up. 629 nm is the one you don’t see too much.

I’m no physicist, but the lower gain lines can lase simultaneously with the higher gain lines, no problem, as long as there is sufficient gain available in the plasma. It’s really pretty easy to get a He-Ne laser to output on all lines at the same time (if you have the right mirrors). The trick is optimizing the bore-to-mode ratio, gas pressure, and isotope mixture to get good TEM00 power. Usually the all-lines He-Ne lasers are multi (transverse) mode. I don’t know of anyone who makes them commercially though – at least not intentionally.

Steve’s Comments on Superradiance and the 3.39µm He-Ne Laser

Generally, when a gas laser is superradiant, there is a limit to its maximum power output (with exceptions for nitrogen and copper vapour laser, although nitrogen’s upper limit is defined by the maximum cavity length into which you can generate a 300ns or less excitation pulse.

The 3.39µm He-Ne laser’s gain is still, like all other He-Ne lines limited by a wall collision to return the excited atoms to the ground state. 3.39 µm He-Ne lasers have larger bores then normal He-Ne lasers, and the bores are acid etched to fog them and create more surface area, but still the most power I’ve ever seen published was 40 mW – nothing to write home about. The massive SP-125, the largest commercial He-Ne laser, could be ordered with a special tube and special optics for 3.39µm, and it still only did about 1/3rd the visible power. Superradiance and ultimate power are not tied together.

The reason 3.39µm got all the writeups it did was that it started on the same upper state as all the other He-Ne lines, was easily noticed when it sapped power from the visible line, and was, at the time, a exotic wavelength for which there were few other sources.

Theory of Operation, Modes, Coherence Length

Instant He-Ne Laser Theory

The term laser stands for “Light Amplification by Stimulated Emission of Radiation”. However, lasers as most of us know them, are actually sources of light – oscillators rather than amplifiers. (Although laser amplifiers do exist in applications as diverse as fibre optic communications repeaters and multi-gigawatt laser arrays for inertial fusion research.) Of course, all oscillators – electronic, mechanical, or optical – are constructed by adding the proper kind of positive feedback to an amplifier.

All materials exhibit what is known as a bright line spectra when excited in some way. In the case of gases, this can be an electric current or (RF) radio frequency field. In the case of solids like ruby, a bright pulse of light from a xenon flash lamp can be used. The spectral lines are the result of spontaneous transitions of electrons in the material’s atoms from higher to lower energy levels. A similar set of dark lines result in broad band light that is passed through the material due to the absorption of energy at specific wavelengths. Only a discrete set of energy levels and thus a discrete set of transitions are permitted based on quantum mechanical principles (well beyond the scope of this document, thankfully!). The entire science of spectroscopy is based on fact that every material has a unique spectral signature.

The HeNe laser depends on energy level transitions in the neon gas. In the case of neon, there are dozens if not hundreds of possible wavelength lines of light in this spectrum. Some of the stronger ones are near the 632.8 nm line of the common red HeNe laser – but this is not the strongest:

The strongest red line is 640.2 nm. There is one almost as strong at 633.4 nm. That’s right, 633.4 nm and not 632.8 nm. The 632.8 nm one is quite weak in an ordinary neon spectrum, due to the high energy levels in the neon atom used to produce this line.

 Bright Line Spectra of Helium and Neon
Bright Line Spectra of Helium and Neon

(The relative brightnesses of these don’t appear to be accurate though at present.) More detailed spectra can be found at the: Laser Stars – Spectra of Gas Discharges Page. And there is a photo of an actual HeNe laser discharge spectra with very detailed annotation of most of the visible lines in: Skywise’s Lasers and Optics Reference Section. The comment about the output wavelength not being one of the stronger lines is valid for most lasers as if it were, that energy level would be depleted by spontaneous emission, which isn’t what is wanted!

There are also many infra-red lines and some in the orange, yellow, and green regions of the spectrum as well.

The helium does not participate in the lasing (light emitting) process but is used to couple energy from the discharge to the neon through collisions with the neon atoms. This pumps up the neon to a higher energy state resulting in a population inversion meaning that more atoms in the higher energy state than the ground or equilibrium state.

Helium-Neon Excitation and Lasing Process
Helium-Neon Excitation and Lasing Process

 

It turns out that the upper level of the transition that produces he 632.8 nm line (as well as the other visible He-Ne lasing lines) has an energy level that almost exactly matches the energy level of helium’s lowest excited state. The vibrational coupling between these two states s highly efficient.

  1. A DC electrical discharge or RF field excites He atoms to the 2s energy state.
  2. Collisions efficiently transfer energy raising Ne atoms to the 3s2 energy state. Note the relatively high energy levels involved – over 20 eV for the upper energy states.
  3. Stimulated emission (lasing) causes a drop to one of several Ne 2p states.
  4. Radiative decay (spontaneous emission) drops Ne from the terminal lasing state to the 1s state.
  5. Collisions with the tube wall drops Ne from the 1s state to the Ground state.

For 632.8 nm, one mirror will be highly reflective at 632.8 nm (typically 99.9 percent or better). This is the “High Reflector” or HR. The other mirror will have a typical reflectivity of 99 percent at 632.8 nm. This is the “Output Coupler” or OC from which the useful beam emerges. In order to suppress lasing at other wavelengths, the mirrors will generally be designed to have lower reflectivity there. (Though given the low gain of all the He-Ne lasing lines, especially the “other colour” lines, this isn’t much of a problem at 632.8 nm.)

The rate at which (4) and (5) can take place ultimately limits the power of a He-Ne laser and explains why increasing the excitation (1) actually reduces power above some optimum level.

The gas mixture must be mostly helium (typically 5:1 to 10:1, He:Ne), so that helium atoms can be excited. The excited helium atoms collide with neon atoms, exciting some of them to the state from which they can radiate at 632.8 nm. Without helium, the neon atoms would be excited mostly to lower excited states responsible for non-laser lines. And the gas mixture has to be super pure as any contamination results in excitation of rogue atoms (like H, O, and N) to lower energy states where all that will happen is that they will glow like a poorly made neon sign.

A neon laser with no helium can be constructed but it is much more difficult and the output power will be much lower without this means of energy coupling. Therefore, a He-Ne laser that has lost enough of its helium (e.g., due to diffusion through the seals or glass) will most likely not lase at all since the pumping efficiency will be too low.

However, pure neon will lase superradiantly in a narrow tube (e.g., 40 cm long x 1 mm ID) in the orange (611.9 nm) and yellow (594.1 nm) with orange being the strongest. Superradiant means that no mirrors are used although the addition of a Fabry-Perot cavity (e.g., mirrors!) does improve the lateral coherence and output power. This from a paper entitled: “Super-Radiant Yellow and Orange Laser Transitions in Pure Neon” by H. G. Heard and J. Peterson, Proceedings of the IEEE, Oct. 1964, vol. #52, page #1258. The authors used a pulsed high voltage power supply for excitation (they didn’t attempt to operate the system in CW mode but speculate that it should be possible).

(From: Steve Roberts.)

“Various IR lines will lase in pure neon, and even the 632.8 nm line will lase, but it takes a different pressure and a much longer tube. 632.8 nm also shows up with neon-argon, neon-oxygen, and other mixtures. Just about everything on the periodic table will lase, given the right excitation. See “The CRC Handbook of Lasers” or one of the many compendiums of lasing lines available in larger libraries. These are usually 4 volume sets of books the size of a big phone book just full of every published journal article on lasing action observed. It’s a shame that out of these many thousands and thousands of lasing lines, only 7 different types of lasers are under mainstream use.

There are many possible transitions in neon from the excited state to a lower energy state that can result in laser action. (Only the three found most commonly in commercial He-Ne lasers are shown in the diagram, above.) The most important (from our perspective) are listed below:

Notes:

 

  • Output Wavelength is approximate. In addition to slight variations due to actual lasing conditions (single mode, multimode, doppler broadening, etc.), some references don’t even agree on some of these values to the 4 or 5 significant digits shown.
  • He-Ne Laser Name is what would be likely to be found in a catalogue or spec. sheet. All those that have an entry in this column are readily available commercially.
  • Perceived Beam Colour is how it would appear when spread out and projected onto a white screen. Of course, depending on the revision level of your eyeballs, this may vary someone from individual to individual. 🙂
  • Lasing Transition uses the so-called “Paschen Notation” and indicates the electron shells of the neon atom energy states between which the stimulated emission takes place.
  • Typical Gain (%/m) shows the percent increase in light intensity due to stimulated emission at this wavelength inside the laser tube’s bore. This is the single pass gain and will be affected by tube construction, gas fill ratio and pressure, discharge current, and other factors. The first column is from various sources. The second column is from Hecht, “The Laser Guide Book”. However, a newer text: Mark Csele, “Fundamentals of light sources and lasers” (ISBN 0-471-47660-9, Wiley-Interscience, 2004) lists the typical gain as 1.2 to 1.5 at 633 nm. And measurements by myself and others seem to show that this slightly higher value may be more accurate, at least under some conditions.
  • Gain at 1,523 nm may be similar to that of 543.5 nm – about 0.5%/m. Gain at 3,391 nm is by far the highest of any – possibly more than 100%/m. I know of one particular He-Ne laser operating at this wavelength that used an OC with a reflectivity of only 60% with a bore less than 0.4m long. Yet, the output power of the largest 3,391 nm commercial He-Ne laser is still only a fraction of that at 632.8 nm.

Maximum Power shows the highest output power lasers commercially available in a TEM00 beam for each wavelength. The first number is rated power while the number in () is achieved output power for a particularly lively tube. Lasers operating with multiple (spatial) modes (non-TEM00) may have somewhat higher output power.

The most common and least expensive He-Ne laser by far is the one called ‘red’ at 632.8 nm. However, all the others with named ‘colours’ are readily available with green probably being second in popularity due to its increased visibility near the peak of the of the human eye’s response curve (555 nm). And, with some He-Ne lasers with insufficiently narrow-band mirrors, you may see 640 nm red as a weak output along with the normal 632.8 nm red because of its relatively high gain. There are even tunable He-Ne lasers capable of outputting any one of up to 5 or more wavelengths by turning a knob. While we normally don’t think of a He-Ne laser as producing an infra-red (and invisible) beam, the IR spectral lines are quite strong – in some cases more so than the visible lines – and He-Ne lasers at all of these wavelengths (and others) are commercially available.

The first gas laser developed in the early 1960s was an HeNe laser operated at 1,152.3 nm. In fact, the IR line at 3,391.3 is so strong that a HeNe laser operating in ‘superradiant’ mode – without mirrors – can be built for this wavelength and commercial 3,391.3 nm HeNe lasers may use an output mirror with a reflectivity of less than 50 percent. Contrast this to the most common 632.8 nm (red) He-Ne laser which requires very high reflectivity mirrors (often over 99 percent) and extreme care to minimize losses or it won’t function at all.

When the He-Ne gas mixture is excited, all possible transitions occur at a steady rate due to spontaneous emission. However, most of the photons are emitted with a random direction and phase, and only light at one of these wavelengths is usually desired in the laser beam. At this point, we have basically the glow of a neon sign with some helium mixed in!

To turn spontaneous emission into the stimulated emission of a laser, a way of selectively amplifying one of these wavelengths is needed and providing feedback so that a sustained oscillation can be maintained. This may be accomplished by locating the discharge between a pair of mirrors forming what is known as a Fabry-Perot resonator or cavity. One mirror is totally reflective and the other is partially reflective to allow the beam to escape.

One mirror may be perfectly flat (planar) or both may be spherical with a typical Radius of Curvature (RoC = 2 * focal length) slightly longer that the length of the cavity (L) or even longer. Where both mirrors have an RoC equal to L, the configuration is called ‘confocal’ (the focii of the two mirrors are coincident), but it is marginall stable, so the RoCs will be at least slightly longer than L. A cavity with two planar mirrors is borderline stable and essentially impossible to align or maintain in alignment over time, so it is never used in He-Ne lasers (but is in some pulsed solid state and other lasers). Curved mirrors result in an easier to align more stable configuration but are more expensive than planar mirrors to manufacture and are not as efficient since less of the lasing medium volume is used (think of the shape of the beam inside the bore). The confocal arrangement represents a good compromise between a true spherical cavity (r = 1/2 * L) which is easiest to align but least efficient and one with plane parallel mirrors (f = infinity) which is most difficult to align but uses the maximum volume of the lasing medium. (But as noted above, for a practical confocal cavity, RoCs slightly longer than L are used to assure stability.)

These mirrors are normally made so that the two mirrors together has peak reflectivity at the desired laser wavelength. (For technical reasons, it’s sometimes easier to make mirrors like cliffs – high reflectivity that drops to low reflectivity at a given wavelength, in either direction – than to guarantee a particular peak reflectivity.) When a spontaneously emitted photon resulting from the transition corresponding to this peak happens to be emitted in a direction nearly parallel to the long axis of the tube, it stimulates additional transitions in excited atoms. These atoms then emit photons at the same wavelength and with the same direction and phase. The photons bounce back and forth in the resonant cavity stimulating additional photon emission. Each pass through the discharge results in amplification – gain – of the light. If the gain due to stimulated emission exceeds the losses due to imperfect mirrors and other factors, the intensity builds up and a coherent beam of laser light emerges via the partially reflecting mirror at one end. With the proper discharge power, the excitation and emission exactly balance and a maximum strength continuous stable output beam is produced.

Spontaneously emitted photons that are not parallel to the axis of the tube will miss the mirrors entirely or will result in stimulated photons that are reflected only a couple of times before they are lost out the sides of the tube. Those that occur at the wrong wavelength will be reflected poorly if at all by the mirrors and any light at these wavelengths will die out as well.

Summary of the He-Ne Lasing Process

The He-Ne laser is a 4 level laser (see the table above for the specific energy level transitions for the common wavelengths):

  • Collisions with excited helium atoms raise the neon atoms from level 1 (ground state) to level 4 (which is the 3s state for visible wavelengths).
  • The visible lasing transitions are from the 3s to various 2p states (depending on wavelength) or level 3.
  • The neon atoms then decay rapidly to the 1s state or level 2.
  • Return to the ground state or level 1 is aided by collisions with the He-Ne laser tube’s bore/capillary walls.

For most common IR wavelengths, level 4 is the 2s state and level 3 are various 2p states. However, the very strong 3.93 um line originates from the 3s state just like the visible wavelengths – and is the reason it competes with them in long He-Ne tubes and must be suppressed to optimize visible output.

The ‘s’ states of neon have about 10 times the lifetime of the ‘p’ states and thus support the population inversion since a neon atom can hang around in the 2s state long enough for stimulated emission to take place. However, the limiting effect is the decay back to level 1, the ground state, since the 1s state also has a long lifetime. Thus, one wants a narrow bore to facilitate collisions with its walls. But this results in increased losses. Modern He-Ne lasers operate at a compromise among several contradictory requirements which is one reason that their maximum output power is relatively low.

Approximate Reference Values for the Red (632.8 nm) He-Ne Laser

Here are some common values and relationships that may come in handy when doing calculations. These are not the most exact since they may depend on other factors like the precise gas-fill and environmental conditions but are generally good enough for government work. 🙂

  • Wavelength: 632.8 nm.
  • Optical Frequency: 474 THz.
  • Gain Bandwidth of Neon: 1.6 GHz or 2.136 nm.
  • 1 nm at 632.8 nm: 749 GHz.
  • 1 GHz at 632.8 nm: 1.335 nm.

Longitudinal Modes of Operation

The physical dimensions of the Fabry-Perot resonator impose some additional constraints on the resulting beam characteristics.

While it is commonly believed that the 632.8 nm (for example) transition is a sharp peak, it is actually a Gaussian – bell shaped – curve. (Strictly speaking, it is something called a “Voigt distribution” which is a combination of Gaussian and Lorentzian – but that’s for the advanced course. Gaussian is close enough for this discussion since the discrepancy only shows up way out in the tails of the curve.) In order for a linear or (Fabry-Perot) cavity to resonate strongly, a standing wave pattern must exist. This will only occur when an integral number of half wavelengths fit between the two mirrors. This restricts possible axial or longitudinal modes of oscillation to:

Where:

  • L is the distance between the mirrors (m).
  • W denotes the possible wavelengths of oscillation (m).
  • n is a large integer (order of 948,000 for W around 632.8 nm, L = .3 m).
  • F denotes the possible frequencies of oscillation (Hz).
  • c is the speed of light (approximately 300 million m/s).

The laser will not operate with just any wavelength – it must satisfy this equation. Therefore, the output will not usually be a single peak at 632.8 nm but a series of peaks around 632.8 nm spaced c/(2*L) Hz apart. Longer cavities result in closer mode spacing and a larger number of modes since the gain won’t fall off as rapidly as the modes move away from the peak. For example, a cavity length of 150 mm results in a longitudinal mode spacing of about 1 GHz; L = 300 mm results in about 500 MHz. The strongest spectral lines in the output will be nearest the combined peak of the lasing medium and mirror reflectivity but many others will still be present. This is called multimode operation.

Think of the vibrating string of a violin or piano. Being fixed at both ends, it can only sustain oscillations where an integer number of cycles fits on the string. In the case of a string, n can equal 1 (fundamental) and 2, 3, 4, 5 (harmonics or overtones). Due to the tension and stiffness of the string, only small integer values for n are present with a significant amplitude. For a He-Ne laser, the distribution of the selected neon spectral line and shape of the reflectivity function of the mirrors with respect to wavelength determine which values of n are present and the effective gain of each one. And n will be much greater than 1!

For a typical HeNe laser tube, possible values of n will form a series of very large numbers like 948,161, 948,162, 948,163, 948,164,…. rather than 1, 2, 3, 4. 🙂 A typical gain function showing the emission curve of the excited neon multiplied by the mode structure of the Fabry-Perot resonator and the reflectivity curve of the mirrors may look something like the following:

Or, see the following for some slightly more aesthetically pleasing diagrams of the longitudinal modes of random polarized He-Ne lasers. 🙂

Longitudinal Modes of Typical Random Polarized 1 mW HeNe Laser
Longitudinal Modes of Typical Random Polarized 1 mW He-Ne Laser
Longitudinal Modes of Typical Random Polarized 3 mW HeNe Laser
Longitudinal Modes of Typical Random Polarized 3 mW He-Ne Laser
Longitudinal Modes of Typical Random Polarized 8 mW HeNe Laser
Longitudinal Modes of Typical Random Polarized 8 mW He-Ne Laser
Longitudinal Modes of Typical Random Polarized 30 mW HeNe Laser
Longitudinal Modes of Typical Random Polarized 30 mW He-Ne Laser

Mode Sweep

Since the mode locations are determined by the physical spacing of the mirrors, as the tube warms up and expands, these spectral line frequencies are going to drift downward (toward longer wavelengths). However, since the reflectivity of the mirrors as a function of wavelength is quite broad (for all practical purposes, a constant), new lines will fill in from above and the overall shape of the function doesn’t change.

In the diagrams above, a single arbitrary mode position is shown, but for well behaved lasers, the lasing lines will move smoothly through the gain curve as the laser warms up. This is called by various names including “mode sweep” and “mode cycling”. While present with most lasers, the effects are quite striking with low to medium power He-Ne lasers due to their relatively narrow neon gain bandwidth (which is only a small multiple of the longitudinal mode spacing in low to medium power He-Ne lasers), the rather fortuitous phenomenon that for red (633 nm) He-Ne lasers at least, adjacent longitudinal modes tend to be orthogonally polarized, and nearly ideal behaviour in other respects with the Physics mostly cooperating. (Murphy has seen the LASER DANGER signs and stays away!) Much more on all this below (except perhaps for Murphy).

In the nice diagram above 🙂 of the 8 mW laser, there are 5 longitudinal cavity modes that see gain above the lasing threshold (the right-most just barely). These become lasing modes (red and blue) producing a total output power of somewhat over 8 mW in this specific example. For the 30 mW laser, there are twice as many lasing modes one half the distance apart, and each mode has more power. Interestingly, adjacent modes in a so-called “random polarized” red (632.8 nm) He-Ne laser are almost always orthogonally polarized, with the polarization axes fixed relative to the tube. (Here, one of them is arbitrarily referenced as 0 degrees, more on this later). As the distance between the mirrors is increased, the number of oscillating modes increases as well, though the actual power in each mode increases only slightly.

Mode Sweep of 8 mW Random Polarized He-Ne Laser
Mode Sweep of 8 mW Random Polarized He-Ne Laser

One complete cycle (red or blue) represents a change in cavity length of one wavelength (at 633 nm) and a change in optical frequency of 2 times the mode spacing of c/2L. The additional factor of 2 arises because the adjacent modes of the red (633 nm) HeNe are orthogonally polarized. This is not true with most other lasers and even HeNe lasers at other wavelengths. Note that while the profile of the mode sweep is affected by the neon gain curve, the period is NOT directly related to it, only c/2L.

However, note that as HeNe lasers get longer, mode competition results in greater and greater instability, so don’t expect to see a nice orderly march with a Spectra-Physics 127 (39 inch cavity). In fact while the envelope of the modes will generally follow the gain curve, each mode will be jumping up and down in a quasi-chaotic dance! Instability may appear in the display of a Scanning Fabry-Perot Interferometer (SFPI) when viewing the longitudinal modes of a 633 nm HeNe with tubes rated at 7 to 10 mW. 5 mW lasers are usually quite clean while 35 mW lasers can be a real mess.

For very short HeNe tubes, the width of the gain curve may be similar to or even narrower than the spacing between modes. With those, the output power will become very low or go to zero during portions of the mode sweep. Very few HeNe lasers were produced with cavity lengths where this would be an issue since maximum output power would be very low. The only one I know of was the Spectra-Physics 119 stabilized laser with a 100 mm cavity length (mode spacing of 1.5 GHz). The very short cavity was required to provide special characteristics for this system.

In fact, it’s often possible to go so far as to identify a specific manufacturer and even model of a HeNe laser tube based solely on the plots of its polarized mode sweep, providing a sort of “fingerprint” for lasers. 🙂 For example, the type of tube installed in a Zygo or Teletrac/Axsys stabilized laser can be determined without opening the case!

He-Ne Laser Mode Sweep Fingerprints
He-Ne Laser Mode Sweep Fingerprints

These tubes are all physically similar yet have dramatically different mode sweep plots. And, it’s often possible to determine key information about the health of a laser tube by comparing its mode sweep with that of a new one. Over most of its life, the general shape will remain the same, but as the power declines, in addition to the total height of the plot decreasing, the amplitude of the variation (i.e., the AC component) relative to the total will increase. However, near end-of-life when power is way down and fewer modes are oscillating, the distinctions will tend to disappear.

For very long tubes like the 30 mW one in the example above where there are many longitudinal modes, the actual appearance of mode sweep may be rather chaotic as power shifts among the modes in a random dance. When I first observed this behaviour with a Melles Griot 05-LHP-928 (35 mW) He-Ne producing over 40 mW, I thought it might have been defective in some way despite the high power. But two other healthy samples behaved in a similar manner. So, don’t expect to see nice well behaved marching modes for these high power lasers. There is often a hint of instability even in shorter tubes though it may be subtle – a few percent variation in the peak amplitudes not attributable to other causes like normal movement under the gain curve or power supply ripple.

The effects of mode sweep are more dramatic with short low pressure carbon dioxide (CO2) lasers because for a given resonator length, the ratio of wavelengths (10,600 nm for CO2 compared to 632.8 nm for He-Ne means that the longitudinal mode spacing is 16.7 times larger). In these cases, the laser output will turn on and off as it heats up and the distance between the mirrors increases due to thermal expansion. For this to happen in a 632.8 nm He-Ne would require the tube to be less than about 75 mm (3 inches) in length.

A linearly polarized He-Ne laser would have the same longitudinal mode spacing, but all the lasing modes would have the same polarization orientation (red or blue) as shown in the diagrams and animations, above.

Longitudinal Modes of Typical Linearly Polarized 8 mW He-Ne Laser
Longitudinal Modes of Typical Linearly Polarized 8 mW He-Ne Laser

So, someone with red/blue color-blindness (if there is such a thing) would see the diagrams for all them as being linearly polarized!

A label on the polarized laser will indicate the plane or orientation of polarization of the output beam. For a random polarized He-Ne laser, a polarizer oriented at 45 degrees with respect to the plane of polarization would produce an output with respect to mode sweep that is similar to that of a linearly polarized laser, except that even with an ideal polarizer, the output power would be cut in half.

Now for some actual numbers: The Doppler-broadened gain curve for neon in a red (632.8 nm) He-Ne laser has a Full Width Half Maximum (FWHM, where the gain is at least half the peak value) on the order of 1.5 or 1.6 GHz. So, for a 500 mm long (high gain) tube with its mode spacing of about 300 MHz (similar to what is depicted above), 5 or 6 lines may be active simultaneously and oscillation will always be sustained (though there would be some variation in output power as various modes sweep by and compete for attention). However, for a little 10 cm tube, the mode spacing is about 1,500 MHz. If this laser were to be really unlucky (i.e., the distance between mirrors was exactly wrong) the cavity resonance might not fall in a portion of the gain curve with enough gain to even lase at all! Or, as the tube heats up and expands, the laser would go on and off. There are very few commercial He-Ne laser tubes that short. It is possible to widen the gain curve somewhat by using a mixture of neon isotopes (Ne20 and Ne22) rather than a single one since the location of their peak gain differ slightly. This would allow a smaller cavity to lase reliably and/or reduce amplitude variations from mode sweeping in all size He-Ne lasers. The actual lasing threshold will also determine the effective width of the neon gain curve over which lasing occurs, so it may be wider than the FWHM.

A high speed silicon photodiode and oscilloscope or RF spectrum analyzer can be used to view the frequencies associated with the longitudinal modes of a He-Ne laser. The clearest demonstration would be using a short tube where at most two longitudinal modes are active. This will result in a single difference frequency when both modes are lasing. A polarized tube is best as it forces both modes to have the same polarization as a photodiode will not detect the difference frequencies for orthogonally polarized modes. Adjacent longitudinal modes of random polarized tubes are almost always orthogonally polarized (for a 633 nm He-Ne at least). But, adding a polarizer at 45 degrees to the polarization axes can compensate for this with a slight loss in signal strength. Without a polarizer, the beat frequencies of a random polarized laser will tend to be at multiples of twice the mode spacing since only those modes with the same polarization orientation beat with each-other in the photodiode. (If measured very accurately, it will be seen that these frequencies will not generally be exactly at multiples of the mode spacing based on c/2L and will vary slightly during mode sweep. The is due to mode pulling or pushing effects, reserved for the advanced course!)

Passive stabilization (using a structure made of a combination of materials with a very low or net zero coefficient of thermal expansion or a temperature regulator) or active stabilization (using optical feedback and piezo or magnetic actuators to move the mirrors, or a heating element to control the length of the entire structure) can compensate for these effects. However, the added expense is only justified for high performance lab quality lasers or industrial applications like interferometric based precision measurement systems – you won’t find these enhancements on the common cheap He-Ne tubes found in barcode scanners.

Thus, a typical HeNe laser is not monochromatic though the effective spectral line width is very narrow compared to common light sources. Additional effort is needed to produce a truly monochromatic source operating in a single longitudinal mode. One way to do this is to introduce another adjustable resonator called an etalon into the beam path inside the cavity. A typical etalon consists of a clear optical plate with parallel surfaces. Partial reflections from its two surfaces make it act as a weak Fabry-Perot resonator with a set of modes of its own. Then, only modes which have the same optical frequency in both resonators will produce enough gain to sustain laser output.

The longitudinal mode structure of an optional intra-cavity etalon might look like the following (not to scale):

Notice that since the distance between the two surfaces of the etalon is much less than the distance between the main mirrors, the peaks are much further apart (even more so than shown). (The etalon’s index of refraction also gets involved here but that is just a detail.) By adjusting the angle of the etalon, its peaks will shift left or right (since the effective distance between its two surfaces changes) so that one spectral line can be selected to be coincident with a peak in the main gain function. This will result in single mode operation. The side peaks of the etalon (-1, +1 and beyond) will may coincide with weak peaks in the main gain function shown above but their combined amplitude (product) is insufficient to contribute to laser output.

Intracavity Etalon for Line Selection in a Single Mode He-Ne Laser
Intracavity Etalon for Line Selection in a Single Mode He-Ne Laser

This example is based on the same 30 mW laser as in the diagram in the section: Longitudinal Modes of Operation. Adding an etalon inside the cavity introduces an additional loss function with peaks every GHz or so. (Note that such an etalon would be about 15 cm long, so the plasma tube for this laser needs to be short enough to allow for that much space between it and one of the mirrors, but that’s just a detail!) Only where the product of the original net (round trip) gain and the etalon transmission is above one will the laser lase. For this example, there is only place where a cavity mode and etalon mode coincide – just to the left of centre of the neon gain curve peak. And, now that there is only a single mode oscillating, it will have an output power of over 15 mW, rather than the ~3 mW or less in each of several multiple modes. There is always some loss in adding an etalon, so the full 30+ mW originally present isn’t usually possible, though the ~50 percent reduction in output power shown here may be excessive.

(From: Prof Harvey Rutt (h.rutt@ecs.soton.ac.uk).)

The standard, small He-Ne laser normally lases on only one transition, the well known red line at about 632.8 nm.

The He-Ne gain curve is inhomogeneously Doppler-broadened with a gain bandwidth of around 1.5 GHz (at 632.8 nm). (The width of the Doppler-broadened gain curve depends on the lasing wavelength. At 3,391 nm, it is only about 310 MHz.) For a typical laser, say 30 cm long, the axial modes are separated by about 500 MHz. Typically, two or three axial modes are above threshold, in fact as the laser length drifts you typically get two modes (placed symmetrically about line centre) or three modes (one near centre, one either side) cyclically, and a slow periodic power drift results. Shorter lasers, less modes, more power variation unless stabilized. But it needs a huge He-Ne laser to get ten modes, and since they are closer of course they still only spread over the 1.5 GHz line width.

Most He-Ne lasers which do not contain a Brewster window or internal Brewster plate are randomly polarized; adjacent modes tend to be of alternating orthogonal polarizations. (Note that this is not necessarily true for He-Ne lasers operating at wavelengths other than 632.8 nm and/or can be overridden with a transverse magnetic field, see below.

Some frequency stabilized HeNe lasers are NOT single mode, but have two, and the stabilization acts to keep them symmetrical about line centre – i.e., both are half a mode spacing off line centre. A polariser will then split off one of them or a polarizing beamsplitter will separate the two.

(From: Sam.)

The party line is that adjacent modes in a He-Ne laser will be of orthogonal polarization. However, I’ve seen samples of small (e.g., 5 or 6 inch) random polarized tubes only supporting 2 active modes where this is not the case – they output a polarized beam that remains stable with warmup and in any case, applying a strong transverse magnetic field will override the natural polarization. So, it’s not a strong effect. Only if everything inside the tube is reasonably symmetric, will the modes alternate. Modes may also remain one polarization as they move through part of the gain curve and then abruptly – and repeatably – flip polarization. But the majority of tubes are well behaved in this regard.

Resonator Length and Mode Hopping

Here are some additional comments that address the common fear of the novice laser enthusiast that the resonator length has to be stabilized to the nm or else the laser will blink off.

(Portions from: Steve Roberts.)

Flames expected, as I’m ignoring some of the physics and am trying to explain some of this based on what I observe, aligning and adjusting cavities on He-Ne and argon ion lasers as part of repairing them. Anyone who only goes by the textbooks has missed out on the fun, obviously having never had to work on an external mirror resonator. It can be quite a education!

Due to the complex number of possible paths down the typical gain medium, you will see lasing as long as the mirrors are reasonably aligned. The cavity spacing is not always that critical and will change anyway as the mirror mounts are adjusted (there will always be some unavoidable translation even if only the angle is supposed to be changed). No, lasers don’t really flash on and off in interferometric nulls as you translate the mirrors – they instead change lasing modes. They will find another workable path. You will in some cases see this as a change in intensity but it is more properly observed on a optical spectrum analyzer as a change in mode beating. Eventually you can translate them far apart enough that lasing ceases, but this is a function of your optics not the resonator expansion.

I have seen what you fear in some cases by adding a third mirror to a two mirror cavity with a low gain medium such as He-Ne where the third mirror can be positioned in such a way to kill many possible modes. This usually occurs when I use a He-Ne laser to align an argon laser’s mirrors and the HeNe laser will flicker from back reflections. See the section: External Mirror Laser Cleaning and Alignment Techniques. But unless you have a extremely unstable resonator design, translation will just cause mode hopping, this becomes important on a frequency stabilized or mode locked laser if you have a precision lab application. Otherwise, most commercial lasers are not length stabilized in the least. There are equations and techniques for determining if you have a stable optical design – stable in this case meaning it will support lasing over a broad range of transverse and longitudinal modes. For examples see any text by A. E. Siegman or Koechner. If your library doesn’t have any similar texts, find a book on microwave waveguides. It might aid you in visualizing what is going on.

Either an intracavity etalon or active stabilization systems are usually used on single frequency systems anyway, by either translating the mirror on piezos or by pulling on mirror supports with small electromagnets, or in the case of smaller units, heaters to change the cavity length on internal mirror tubes. An etalon is basically a precision flat glass plate in the lasing path between the mirrors, its length is changed by a oven and it acts as a mode filter.

Length stabilization to the 50 or 100 nm you might have expected to be needed would be gross overkill anyhow, and would be impossible to achieve in practice by stabilizing the resonator alone. Depending on the end use of the product, most lasers are simply built with a low expansion resonator of graphite composite or Invar, although in many products a simple aluminium block or L shape is used, a few rare cases use rods made of two different materials designed to compensate by one short high expansion rod moving the mirror mount in opposition to the main expansion. A small fraction of a millimeter is a more reasonable specification.

(From: Prof Harvey Rutt (h.rutt@ecs.soton.ac.uk).)

The basic idea, that the laser can only work at the frequencies where an integral number of half waves fit in the cavity, is perfectly correct. The separation between adjacent modes is just 1/(2*L) where L is the cavity length in cm. From this we get the separation in ‘wavenumbers’. One wavenumber is 30 GHz, so in more usual units it is just 30 GHz/(2*L). Or, to make it easy, in a 50 cm long laser the modes are 300 MHz apart. That is not very far optically.

The laser operates by some molecule, gas, ion in a crystal, etc. making a transition between two levels. But those levels are not perfectly ‘sharp’; we say they are ‘broadened’. The reason can be many things:

  • In a gas – Doppler (or temperature) broadening. The molecules move about randomly, and the light is Doppler shifted a random amount.
  • Collision (pressure) broadening. Collisions either relax or dephase the state – i.e., ‘mess it up’ and broaden it!
  • In a solid various things can happen, but for example in a glass different laser ions are in slightly different positions, and this causes them to have slightly different energies.

In any case no transition is *perfectly* sharp, the fact that it has a finite lifetime gives it a certain width, but this is not often the real limit, something else is usually more important.

These broadening mechanisms ‘blur out’ the line – we see optical gain over that *range* of frequencies, the gain bandwidth.

An example is carbon dioxide. The ‘natural width’ is very small, of order Hz. The Doppler width at 300 °K is about 70 MHz. The collision-broadened width increases about 7 MHz/Torr; so well below 10 Torr the width is Doppler-limited, ~70 MHz; above 10 Torr pressure broadened (e.g. ~700 MHz at 100 Torr).

If I take a typical He-Ne laser it might ‘blur’ out over a GHz or so – **more** than that 300 MHz mode spacing – so there are *always* two or thee modes within the ‘gain bandwidth’ and it will always lase. For a glass laser there might be *thousands* of modes, because the glass gain is very wide indeed.

But there *are* cases that go the other way. For carbon dioxide, at low pressure, the line is Doppler-broadened and about 70 MHz wide, much **LESS** than that 300 MHz mode spacing. So short carbon dioxide lasers really do turn on and off as the cavity length changes, and you have to ‘tune’ the cavity length to get a mode inside the gain width. This mainly happens with short, gas lasers in the infrared.

For a *high pressure* CO2 laser at 760 Torr (1atm), the line width is several GHz, much more than the mode spacing, so the effect disappears.

Observing Longitudinal Modes of a He-Ne Laser

Monitoring the output power of any He-Ne laser while it’s warming up will show a variation in output power due to longitudinal mode cycling. There is even a specification called the “Mode Sweep Percentage” which indicates how large the variation is in relation to the output power. For short tubes, the power fluctuations can approach 20 percent; for long tubes, they may be less than 2 percent.

There are many ways to actually “see” the modes of a laser including the use of an instrument called a Scanning Fabry-Perot Interferometer. However, for a short tube with only 1 or 2 modes, it’s quite straightforward to interpret what’s going on from the output power and polarization alone. All that’s needed is a photodiode and multimeter (or continuous reading laser power meter), and polarizing filter. (A lens from a pair of polarized Sun glasses or a photographic polarizing filter will do.) The power monitor can be set up in the output beam and the polarizing filter in the waste beam from the HR mirror. Alternatively, a non-polarizing beamsplitter can be used to provide the two beams. Adding a polarizing beamsplitter oriented so that it separates the two polarization orientations in one of the beams can simplify the interpretation of the polarization changes.

Changing the orientation of the polarizer will affect the amplitude of the intensity variations. For most red He-Ne lasers, the longitudinal modes will generally remain at two fixed orthogonal orientations, with adjacent modes usually being orthogonal to each other. As the tube heats and the cavity length increases, the modes march along under the gain curve with those at one end disappearing and new ones appearing at the other end as described above. But for well behaved tubes, they don’t flip polarization. When the polarizer is oriented at 45 degrees to the polarization axes of the tube, the reading will remain constant. When aligned with the polarization axes of the tube, the reading will fluctuate the most.

As a specific example, consider an He-Ne laser tube with a mirror spacing of 120 mm (about 4.75 inches, one of the shortest commercially available laser tubes). This corresponds to a mode spacing of about 1.25 GHz – rather close to the FWHM of 1.5 to 1.6 GHz for the neon gain bandwidth. With this tube, at most 2 modes will be oscillating at any given time. When the output power and polarization is monitored while the tube is warming up, a very distinctive behaviour will be observed. One might think that it should be a periodic variation in output power with a simple sinusoidal or similar characteristic. However, there will actually be two peaks for each cycle: A large one corresponding to when there is a single lasing mode at the centre of the gain curve, and a smaller one when there are two modes symmetric around the centre of the gain curve. For most tubes, the polarization of adjacent modes is orthogonal and will remain fixed with the mode. So, as the modes cycle under the gain curve successive large peaks will have opposite polarization. The small peaks will have equal components of both polarizations. Even though two modes are oscillating, the gain for each one is so much closer to the lasing threshold that their combined power is still lower than for the single mode at the peak of the gain curve. There may also be rather sudden changes in output power as modes on the tails of the gain curve come and go. However, for some tubes which are affectionately called “flippers”, the polarization of the modes will tend to suddenly change orientation as they move through the gain curve. This should also be apparent when viewing the beam through a polarizing filter.

Waveforms and RF Spectrum of Longitudinal Modes

While the beam from a healthy He-Ne laser appears by eye to be constant (except possibly for the normal variation in output power during mode sweep), only a single frequency laser has an output which is truly DC. With a high speed photodiode and basic test equipment, a great deal of information can be determined as a result of the interaction among the multiple longitudinal modes (also called axial modes) that are present in all but the shortest He-Ne lasers (or stabilized single frequency lasers). OK, well perhaps this requires some not quite so basic test equipment like a high speed oscilloscope and/or RF spectrum analyzer. 🙂 While these instruments may not be something you have handy, if you’re friendly with someone in a research lab at a local college or university, they may have may be able to help and then everyone could learn a lot from some simple experiments! 🙂

The photodiode (PD) must have a frequency response that extends beyond at least the longitudinal mode spacing of the laser. A fancy costly one may not be essential, only that the PD is quite small. One with a 1 GHz response is typically around 1 mm square, with the frequency response being roughly inversely proportional to area. Candidate PDs may turn up in all sorts of equipment, even old optical mice. The PD should be back-biased with a few volts to improve frequency response and set up to drive into a 50 ohm load terminating at the scope input. Basing the circuit on something like the Thorlabs DET10A would be perfect. (Search for this on the Thorlabs Web site. The spec sheet will have the circuit diagram.)

The first approach is to view the resulting mode beating on a fast oscilloscope. For a random polarized laser, a linear polarizer will be required in front of the PD oriented at 45 degrees to the principle polarization axes of the laser to force adjacent modes that are usually orthogonal to have the same polarization at the PD. The adjacent longitudinal modes will then produce a beat equal to their difference frequency. There will also be weaker beats from all other combinations of modes. Common HeNe lasers have a fundamental mode spacing of between 1.5 GHz (for a tiny 0.5 mW barcode scanner tube, around 10 cm between mirrors) and 161 MHz (for a 35 mW SP-127, around 95 cm between mirrors).

Typical Longitudinal Mode Beat Waveforms of Melles Griot 05-LHP-151 He-Ne Laser
Typical Longitudinal Mode Beat Waveforms of Melles Griot 05-LHP-151 He-Ne Laser

This laser is rated 5 mW with a mode spacing of 438 MHz (around 58 cm between mirrors). The waveforms were taken using a Thorlabs DET210 photodetector and my special edition laser-zapped Tektronix 2467 oscilloscope – formerly resident in the test department of a major laser manufacturer – evident from the 5 unsightly black blobs on the lower part of the screen where the CRT phosphor has been blown away by a high power pulsed laser! 🙂 While the fundamental can usually be seen, information about any higher difference frequencies is hard to interpret. And even this relatively fast scope doesn’t have much sensitivity beyond the 438 MHz fundamental. The screen shots are in no particular order in the montage other than to make the sequence somewhat pleasing. 🙂 This is further complicated by higher order effects like mode pulling, which slightly shift the positions of the modes based on their location relative to the centre of the neon gain curve. Thus, beyond confirming that the mode spacing is as expected, not much more can be easily determined and switching to the frequency domain will be more fruitful.

The output from the PD may also be applied to an RF spectrum analyzer, there will be significant power detected at the longitudinal mode spacing and its harmonics (hundreds of MHz or more) due to beating between longitudinal modes, as well as under 1 MHz (due to second order beats and mode pulling).

RF Spectra of Melles Griot 05-LHP-151 He-Ne Laser During Mode Sweep
RF Spectra of Melles Griot 05-LHP-151 He-Ne Laser During Mode Sweep

The above image shows the primary beat signal for the same laser head using a Thorlabs DET210 1 GHz silicon photodetector and an HP 8590L RF spectrum analyzer. (As with the scope, for a random polarized laser, a polarizer would need to be placed in front of the PD oriented at 45 degrees to the polarization axes to detect adjacent beats.) The centre frequency is around 437 MHz and the span is 1 MHz. (Each box is 100 kHz.) (The spec’d value for the mode spacing of this laser is 438 MHz but it’s possible the spectrum analyzer is in need of calibration! Otherwise, complain to Melles Griot!) The sequence of screen shots show about half the full mode sweep cycle.

If there were no mode pulling, the display would always look like the one in the upper left corner (or even narrower) – a single frequency. However, the individual modes move slightly compared to the cavity resonances, so the spectrum spreads out as a function of the position of the modes on the neon gain curve.

Interestingly, the display remains where there is a single narrow peak for longer than could be accounted for based on the normal speed with which the frequencies are changing. In fact, it’s impossible to capture a situation where the peak is just slightly wider – it snaps from a FWHM of about 1/5 box (top left in composite photo) to approximately 1 box (top centre) and vice-versa. Nothing in between ever appears. This suggests that there is a self-locking process taking place, as mentioned in the previous section.

When set for a frequency range covering 0 to 200 kHz, peaks are present similar to what appears on the right side of those shown above. But a linear He-Ne laser power supply had to be used to avoid seeing the ripple frequency and harmonics of the switchmode brick overlaid on the beats! There are multiple strong beats at around 874 MHz as well, 2 times the mode spacing. They vary a way similar way as the others. This makes sense since there are are 3 longitudinal modes oscillating most of the time, with 4 modes for a brief period during mode sweep. The spectrum analyzer also claims there are weak peaks at around 1,311 MHz and 1,748 MHz during most of the mode sweep cycle, not simply that period where the self mode-locking takes place. However, it’s not clear where these originate, or if they are even real. To be direct, the one at 1,748 MHz would require 5 modes to produce a beat at 4 times the mode spacing of 437 MHz. But there are never 5 modes present, let alone for most of the cycle. Perhaps they are the sum of second-order beats. Or, they could simply be an artefact of the analyzer, perhaps leakage from an internal mixer.

Typical Longitudinal Mode Beat Waveforms of JDS Uniphase 1145P He-Ne Laser
Typical Longitudinal Mode Beat Waveforms of JDS Uniphase 1145P He-Ne Laser

The above image shows scope display for a JDS Uniphase 1145P, with a mode spacing of 438 MHz (around 34 cm between mirrors). The additional complexity is due both to the lower beat frequencies (and thus better response of the scope) as well as the greater number of modes oscillating. An RF spectrum of this laser would have many more peaks closer together, but would look generally similar to that of the 5 mW laser.

Typical Longitudinal Mode Beat Waveforms of Melles Griot 05-LHP-121 He-Ne Laser
Typical Longitudinal Mode Beat Waveforms of Melles Griot 05-LHP-121 He-Ne Laser

Mode spacing of 687 MHz (around 22 cm between mirrors). With only 3 longitudinal modes oscillating (and stressing the bandwidth capabilities of the poor scope), the display is a fairly clean sine wave. The only obvious difference during mode sweep is that the amplitude changes slightly. However, most of the time, it is a relatively clean sine wave and for a higher power healthier tube, the reduction in amplitude is not that great as in this example.

Transverse Modes of Operation

Lasers can also operate in various transverse modes. Laser specifications will usually refer to the TEM00 mode. This means “Transverse Electromagnetic Mode 0,0” and results in a single beam. The long narrow bore of a typical HeNe laser forces this mode of oscillation. With a wide bore multiple sub-beams can emerge from the same cavity in two dimensions. The TEM mode numbers (TEMxy) denote the number (minus one) or configuration of the sub-beams.

Here is a rough idea of what transverse modes might look like for a rectangular cavity:

I have only shown the rectangular case because that’s the only one I could draw in ASCII!

Other (non-cartesian) patterns of modes will be produced depending on bore configuration, dimensions, and operating conditions. These may have TEMxy coordinates in cylindrical space (radial/angular), or a mixture of rectangular and cylindrical modes, or something else!

To achieve high power from a He-Ne laser, the tube may be designed with a wider but shorter bore which results in transverse multimode output. Since these tubes can be smaller for a given output power, they may also be somewhat less expensive than a similar power TEM00 type. As a source of bright light – for laser shows, for example – such a laser may be acceptable. However, the lower beam quality makes them unsuitable for holography or most serious optical experimentation or research. An example of a high power multimode He-Ne laser head is the Melles Griot 05-LHR-831 which has a rated output power of 25 mW. Compared to their 05-LHR-827 which is a 25 mW TEM00 laser head, the multimode laser is about 2/3rds of the length and runs on about 3/5ths of the operating voltage at lower current.

(Note that it is easy in principle to convert the output of a TEM00 laser into multimode by using a length of fiber-optic cable with lenses at each end to focus the beam into it and collimate the beam coming out. If the core diameter of the fiber is greater than that needed for the fiber itself to be single mode, then the result will be that multiple modes will propagate inside and the output will be multimode. To assure single mode propagation at 632.8 nm with the index of refraction of a typical glass fiber, a 4 um or smaller core is needed. The actual core diameter of the fiber will determine how many modes are actually generated. A core diameter of 10 um will result in a few modes while one of 125 um will produce dozens of modes. Why this would be desired is another matter.) However, all these modes will be exactly the same wavelength since they originate from a single TEM00 beam.

Sometimes, laser companies don’t quite get it right either and a laser tube that is supposed to be TEM00 may actually be multi-transverse mode all the time or whenever it feels like it (e.g., after warmup). I have a 13.5 mW Aerotech tube that is supposed to be TEM00 but produces a beam that has an outer torus (doughnut shape) with a bright spot in the middle. I’ve also seen an apparently factory-new Uniphase green He-Ne laser that produces a similar doughnut beam. Both of these are probably the result of one or both mirrors having a radius of curvature that is too short for the bore diameter. They may have been manufacturing goofups. Everyone can have a bad day, even if it results in a bunch of dud lasers. 🙂 Good for us though. Everyone (well everyone who cares!) has seen a nice TEM00 He-Ne laser. How many have one that does three wavelengths with different mode structures! 🙂

Note that the mode structure implies nothing about the polarization of the beam. Single mode (TEM00) and multimode lasers can be either linearly polarized or randomly polarized depending on the design and for the multimode case, each sub-mode can have its own polarization characteristics. HeNe (and other) lasers will be linearly polarized if there is a Brewster window or Brewster plate inside the cavity. The majority of HeNe laser tubes produce a TEM00 beam which has random polarization. For internal mirror tubes, linear polarization may be an extra cost option. External mirror HeNe lasers also generally produce a TEM00 beam but are linearly polarized since the ends of the tube are terminated with Brewster windows.

A fast photodiode (PD) and oscilloscope or RF spectrum analyzer can be used to view the frequencies associated with transverse modes. The transverse difference frequencies are very low compared to the longitudinal mode spacing so a really high speed PD isn’t needed. A response of a few MHz should be sufficient. Typically less than 2 mm square silicon PD will have an adequate frequency response if back biased. But the modes do have to overlap on the detector so it may be necessary to spread the beam of a multimode He-Ne laser using a lens. A polarized tube is best as it forces the modes to have the same polarization (a PD will not detect the difference frequencies for orthogonally polarized modes). But, adding a polarizer can partially compensate for this, though the polarization may drift with a randomly polarized laser.

Multi-Transverse Mode He-Ne Lasers

As noted, most He-Ne lasers are designed to operate with a single transverse (spatial) mode or TEM00. However, to obtain the highest power for a given tube size or by a goof-up in design, a higher order mode structure may be produced. A non-TEM00 mode may be present if:

  • The bore is too short.
  • The bore is too large in diameter.
  • The mirror RoC is too short.
  • The mirror is too far from the bore-end (same effect as bore being too short).

All of these are really somewhat equivalent and simply mean that more than one mode fits inside the available active mode volume.

  • For a laser designed to be multimode, a low order mode pattern is typical, though it may not look like the examples in textbooks. Mode patterns that resemble hexagonal close-packed honey combs are often the rule rather than the exception since the circular bore doesn’t really favour Cartesian modes like TEM11 or TEM22. And tubes designed to be multimode will probably have higher order modes than TEM01 or TEM10. Multimode He-Ne lasers typically have 50 to 100 percent more output power for their length than equivalent lasers operating TEM00.
  • For a laser with a very wide bore like one using the Melles Griot 05-LHB-570 one-Brewster laser tube and a short RoC mirror, a high order mode structure will be produced with a dozen or more individual spots in a more or less random (possibly sort of hexagonal) pattern.Where there is access to the inside of the cavity (as with a one-Brewster tube), a laser that operates multimode can be forced to operate TEM00 with a stop (aperture) between the external mirror and tube-end. However, there will be a (possibly substantial) reduction is output power. Where both mirrors are external, it may be possible to substitute longer RoC mirrors to force TEM00 mode (again at the expense of some output power).
  • For a laser that is supposed to be TEM00 but due to a design error isn’t, a TEM01 or TEM10 pattern is typical or it may produce a beam shaped like a doughnut (torus) with or without a spot in the middle. I have several long Aerotech He-Ne lasers heads rated 12 mW (actual output power around 13.5 mW) that produce a beam like this. This was either by design, or an “oops” and the heads were relabelled with an “M” indicating multimode.
  • Sometimes, slight misalignment of the mirrors will produce a multimode (probably TEM01 or TEM10) beam in a laser that otherwise operates reliably TEM00. A warped or misaligned bore may also do this.

Note that a speck of dirt or dust on the inside of a mirror or window (if present), or damage to an optical surface, can result in a multi-transverse mode beam even if the bore and mirror parameters are correct for TEM00 operation. Unfortunately, convincing a bit of dust to move out of the way isn’t always easy on the inside of an internal mirror He-Ne laser tube! Yes, though not common, it can happen. This is one reason not to store tubes vertically. I’ve heard of people successfully using a Tesla (Oudin) coil to charge up the errant dust particle, causing it to just out of the way via electrostatic repulsion. Your mileage may vary. 🙂

Coherence Length of HeNe Lasers

Common He-Ne lasers have a coherence length of around 10 to 30 cm. By adding an etalon inside the cavity to suppress all but one longitudinal mode, coherences lengths of 100s of meters are possible. Naturally, such He-Ne lasers are much more expensive and are more likely to be found in optics research labs – not mass produced applications. However, slightly less exotic and expensive stabilized He-Ne lasers are readily available which oscillate on two orthogonal longitudinal modes and locked so they are in a fixed position. When one mode is blocked with a polarizer, the resulting beam is then (nearly) single frequency with a coherence length of hundreds of meters – much longer than can even be measured without a great deal of effort and expense.

The following actually applies to all lasers using Fabry-Perot cavities operating with multiple longitudinal modes. It was in response to the question: “Why does the coherence length of a He-Ne laser tend to be about the same as the tube length?” The answer is that the coherence period is equal to the tube length but the useful coherence length is generally less (except for the special case above of a single mode).

(From: Mattias Pierrou.)

In a He-Ne laser you typically have only a few (but more than one) longitudinal modes. These cavity modes must fulfil the standing-wave criterion which states that must be an integer number of half wavelengths between the mirrors. In the frequency domain this means that the ‘distance’ between two modes is delta nu = c/(2L), where L is the length of the laser.

The beat frequency between the modes gives rise to a periodic variation in the temporal coherence with period 2L/c, i.e. full coherence is obtained between two beams with a path-difference of an n*2L (n integer).

If you have only one frequency, the coherence length is infinite (that is, if you neglect the spectral width of this mode which otherwise limit the coherence length). If you have two modes, the coherence varies harmonically (like a sinus curve).

The more modes you have in the laser, the shorter is the regions (path-length differences) of good coherence, but the period is still the same.

You can try this by setting up a Michelson interferometer and start with equal arm-lengths which of course gives good coherence. Then increase the length of one arm until the visibility of the fringes disappear. This should occur for a path-difference slightly less than 2L (remember that the path-difference is twice the arm-length difference!). If there are only two modes is the laser the zero visibility of fringes should occur at exactly 2L. Now continue to increase the path-difference until you reach 4L (arm-length difference of 2L). You should again see the fringes clearly due to the restored coherence between the beams.

Ripple, Noise, and Other Artifacts in HeNe Lasers

While one normally thinks of a He-Ne laser as a constant or “Continuous Wave” (CW) source, this is far from the case over a wide range of time scales from nanoseconds to hours. Only to our long obsolete Mark I eyeballs does a typical He-Ne laser really look like the DC equivalent of light. 🙂

Some of these artefacts result from implementation but others are fundamental to the lasing process. The following apply to normal He-Ne lasers (not those involving Zeeman splitting or something more exotic):

  • Mode sweep (seconds to hours):
  • Longitudinal mode beating (less than 100 MHz to 1.5 GHz):
  • Transverse mode beating (1 MHz to 100s of MHz):
  • Plasma oscillations (100 kHz to several MHz):
  • Plasma instability:
  • Higher order mode pulling (1 kHz to 1 MHz):
  • Mirror birefringence (100 kHz to 1 MHz):
  • HV power supply line frequency ripple (50/60 Hz and harmonics):
  • HV power supply switching frequency ripple (20 to 100 kHz and harmonics):
  • Mode flipping (0.1 s to minutes):

The closest to a constant output would probably be an intensity stabilized He-Ne operating on a single longitudinal mode, often called “single frequency” (which is close but even that is not totally accurate), with a highly filtered He-Ne laser HV power supply.

Longitudinal Mode Pulling

While introductory textbooks may state that lasers oscillate on multiples of the cavity resonance frequency, c/2L, it turns out that this is actually not true in most cases. (The exceptions would be where the gain curve is essentially flat but that’s another story.) Longitudinal modes that aren’t exactly centered on the gain curve will be at frequencies very slightly offset from these, pulled toward the center of the gain curve with those that are farthest away seeing the most shift. This is a well known effect called “mode pulling” with highly developed theory to back it up. (Mode pulling isn’t unique to lasers. For example, a quartz crystal oscillator can be tuned over a small range using an external capacitor even though its mechanical resonance frequency differs from the output frequency.)

Although the math can get to be rather hairy, one way of thinking of mode pulling is that the cavity bandwidth has a finite extent which depends primarily on the reflectivity of the mirrors and cavity length. So, if the net gain is greater slightly off to one side due to the position of the gain curve relative to the cavity resonance, the lasing line will be shifted in that direction.

When the laser beam hits a high speed photodetector like a photodiode, which is a non-linear (square law) device, in addition to the DC power term, there are the primary difference frequencies which are close to multiples of c/2L (but not exactly due to mode pulling), but also the differences of the difference frequencies – the second order intermodulation products – which will be at (relatively) low frequencies compared to c/2L. As the cavity length changes and the lasing modes drift across the gain curve, the mode pulling effect on each one varies slightly. But, small differences between large numbers can result in dramatic changes in these second order terms, rapidly rising and falling in frequency, and coming and going as modes drop off one end of the gain curve and appear at the other. The amplitude of the second order beat will be much lower than that of the primary beat but is still detectable with a spectrum analyzer, or in some cases with an audio amplifier.

For a He-Ne laser, the range of second order frequencies is typically in the 1 kHz to 100s of kHz range while for a solid state laser it will be in the MHz to 10s or 100s of MHz range. Note that there will generally not be any beat in the range from 0 Hz to some minimum frequency (e.g., 1 kHz or so in the case of the He-Ne laser) as would be expected when the modes are almost symmetric on either side of the gain curve where there would be very low second order frequencies. Apparently, a self mode-locking effect occurs to force these to be exactly zero frequency over a small range of mode positions. This behaviour can easily be observed in the mode beat RF spectrum of a medium power (e.g., 5 mW) He-Ne laser. See the next section.

For these second order beat frequencies to be present, the laser has to be able to oscillate on at least 3 longitudinal modes simultaneously. (With only 2 modes, there will be only a single difference frequency.) The Doppler-broadened gain curve of neon for the He-Ne laser is about 1.5 GHz Full Width Half Maximum (FWHM) at 632.8 nm. To get 3 modes requires the modes to be less than about 500 MHz apart implying a c/2L tube length of about 30 cm or more – typical of a 5 mW or more (rated) He-Ne laser. It should be polarized to force all modes to be of the same polarization – orthogonal polarizations do not mix in a photodetector. For a randomly polarized laser which typically produces alternating polarizations for adjacent modes, a longer tube length would be required to guarantee enough same-polarized modes and/or a polarizer at 45 degrees to the beam polarizations could be added (but this would cut the power to the photodiode by 50 percent or more).

This effect can be demonstrated using a medium length He-Ne laser, high speed photodiode, and audio amplifier. Initially when the laser is turned on and is heating up and expanding the fastest, they may sound like clicks or pops or just non-random noise. As the expansion slows down, more distinct chirps and other interesting sounds will appear. The complexity of the symphony will also depend on the tube length and thus how many modes are oscillating.

A more precise way to look at mode pulling would be to monitor the beat frequencies produced by a high speed photodiode using an RF spectrum analyzer. By expanding the region around c/2L, the changes during mode sweep will be clearly evident. There will be smooth movement as well as sudden shifts corresponding to mode hops. I even did this by beating not a single laser, but two identical stabilized He-Ne lasers against each-other. With two modes from each laser, there are then as many as 6 beat frequencies if 45 degree polarizers are placed in front of each laser and they are then combined in a non-polarizing beam-splitter. I’ll leave analysis of this behaviour as an exercise for the student. It is at first a bit confusing, but with some thought, makes perfect sense. Simply concentrating on the mode pulling of each laser’s longitudinal mode where one laser was locked and the other was allowed to mode sweep yielded a shift of about 500 kHz.

(From: Roithner Lasertechnik (office@roithner-laser.com).)

You can “listen” to a single mode He-Ne tube: Take an X-rated photodiode and an AC power amplifier – guide a small part of the He-Ne laser beam to the photodiode (don’t let it saturate!) – and listen to the “chirping oscillations” during warming up with a speaker. Hint: There are no birds inside the tube. 😉 But it sounds similar! Looks like sin(x)/x.

Low Level Oscillation due to Mirror Birefringence

This is a phenomenon whereby a low level oscillation in output power at hundreds of kHz is present during part of the mode sweep. It’s not something you would see by eye or likely run into by accident, as the variation is typically only around 1 percent of the total power of the tube. But it is in the category of “interesting”. 🙂 In fact, the oscillation was detected only because the spectrum generated by an optical instrument using a laser with this affliction as a wavelength reference was being corrupted by spikes at frequencies that should not have been there. It would go unnoticed by at least 99.999% of the users of He-Ne lasers. 😉

For the following, refer to [download id=”5602″] and click on the last slide to enter the animation. Though slightly shorter, the tube simulated in the animation will have mode sweep similar to that of the tubes in question, with no more than 3 modes present at any time. The red and blue modes denote the two orthogonal polarization axes of the tube called “p” and “s”.

  • The tubes in which these low level oscillations have been observed are all between around 9.0 and 10.5 inches (approximately 225 to 260 mm) in length with random polarization. These have at most 3 modes. It may be present in longer tubes with more modes but this has not been confirmed. Tubes with fewer than 3 modes are immune.
  • So far, only the Zygo 7701/2 and another unidentified Zygo tube, and the Siemens/LASOS LGR-7621s have unequivocally exhibited these oscillations. Tests with the Melles Griot 05-LHR-038 and 05-LHR-117, Spectra-Physics 088-2, and Siemens LGR-7631A resulted in no detectable oscillation even though these tubes are physically similar. When a tube exhibits oscillations, all samples of the same model will do so as well. At least until contradicted. 🙂
  • The oscillation will be present ONLY where 3 longitudinal modes are present – there are 2 blue modes on either side of a red mode, or 2 red modes on either side of a blue mode in the animation. Most of the time, it will appear instantly as soon as a third mode pokes its head above the noise. But in some instances, there will be a delay, and then appear instantly. (Not ramp up to any degree.)
  • The phase of the oscillation is opposite for p and s polarization and their amplitude is similar. Thus, unless only p or only s is selected with a linear polarizer, little or no oscillation may be detected. This means that the p modes are changing in amplitude 180 degrees out of phase with respect to the s modes. And this has been confirmed by observing the p and s oscillations simultaneously using a Polarizing Beam-Splitter (PBS) and two biased photodiodes, while also viewing the longitudinal modes on a Scanning Fabry-Perot Interferometer (SFPI). This would then seem to be some sort of mode competition between the p modes and s modes. (I’ve heard that this opposite phase may not be true with every sample of the same model where the oscillations occur but until I see it with my own eyes, I’ll continue to make the claim!)
  • The p-p amplitude of the oscillation is only on the order of 1 percent of the total output power of the tube. (See why I said you probably wouldn’t see this!) For a tube outputting 3.5 mW total with 2 to 2.5 mW peak in each polarization, this ends up being about 10 mV p-p from the photodiodes. Its amplitude varies somewhat, peaking near the center of the period in which the oscillation is present. The variation may be small or as much as 2:1 depending on the specific laser tube, but does NOT track the amplitude of either of the side modes. The signal appears almost instantly at a minimum of 1/2 its maximum.
  • The frequency of the oscillation is typically between 200 and 600 kHz and differs for each sample of the laser tube (even of the identical model) and possibly depending on whether a p or s mode is in the center (meaning the orientation is a factor). Thus, it is dependent on a physical characteristic of the tube. It also depends on the temperature of the tube to some degree. (No pun….) Here are some *very* rough estimates of the frequencies ranges for several tubes:

    Interestingly, both oscillation frequencies for the Zygo Unknown model tubes were similar, and in one case identical within the uncertainty of my measurements. This was also the only sample of those tubes that I had added “wedge” to the HR mirror since they lacked it for some reason. So possibly the slight back-reflections from the outer surface of the mirror substrate do have some minor effect.

    Additional frequencies at around 1.95 MHz were seen on some of these tubes but they were at much lower levels, and possibly NOT correlated with the presence of 3 longitudinal modes. Another mystery.

  • Except for where the oscillation nearly abruptly appears or disappears (which can have a huge change), the frequency increases or decreases more or less monotonically by up to 10s of percent during the period in which it is present. Whether it increases or decreases depends on if the p or s polarization is in the center, another indication of a physical dependence on tube construction. The monotonicity also indicates an asymmetry in the behaviour with respect to the gain curve or something related to it. Note that the LASOS 7621s and Zygo 7701/2s only varied by 15 to 30 kHz while some of the unknown Zygo tubes varied by almost 200 kHz.

Since the precise behaviour depends on whether the p and s polarization is in the center, and polarization axes are locked to tube orientation, the current hypothesis is that these result from (or are at least affected by) mirror birefringence. Mirror birefringence results from mirror coating processes that are not perfectly symmetric due a crystalline structure or whatever. The result in an effective depth of reflection – and thus cavity length – that depends on orientation, with a typical variation of a fraction of 1 nm.

1 nm of cavity length change at 633 nm for a tube with a cavity length of 9 inches (around 225 mm) represents a frequency change of approximately 2 MHz. So, the observed shifts being in the 100s of kHz would be consistent with p and s modes being shifted off of normal c/2L cavity resonances by a fraction of 1 nm, resulting in some sort or low level mode competition. Perhaps the LASOS and Zygo tubes differ in whether 1 or both mirrors have significant birefringence. But exactly how this all works beyond the above statments would be total hand waving, as if it isn’t already. 😉

Not all coating processes exhibit birefringence but it’s quite possible those used in most common He-Ne laser tubes do since they tend to have fixed polarization axes. And there can also be birefringence resulting from other asymmetries in the tube construction, though they may be smaller. Known exceptions with very low birefringence are REO (based on their own claims and that where fixed polarization axes are required as with most stabilized He-Ne lasers, REO tubes must be more complex to get around this “feature”) and HP/Agilent Zeeman He-Ne tubes (which have very peculiar mode sweep without their Zeeman magnets). Because REO and HP/Agilent tubes are so strange to begin with, it would not be possible to test them for this type of oscillation. Nor is there any easy way of determining if those tubes that don’t exhibit the oscillations have lower or no birefringence. But there must be some asymmetries because they all have fixed polarization orientation.

In coming to the conclusion of mirror birefringence or something related, the following have been ruled out:

  • Higher order longitudinal mode beating: While the primary longitudinal modes differ in frequency by close to cavity mode spacing of c/2L, they aren’t precisely c/2L due to mode pulling effects, which can result in them being off by frequencies in the 100s of kHz range. Then the second order beats – the beats of the beats – could have a difference frequency in this range. However, this would not explain the opposite phase or how a single mode could have the oscillation. And, it would not explain why the low level oscillation is absent from other similar tubes.
  • Transverse mode beating: Not only would it be extremely unlikely for all of these TEM00 tubes to have significant higher order transverse modes, but an explanation involving them would also not be able to account for the opposite phase behavior or the oscillation from a single longitudinal mode. LASOS tube ID #2 did have a non-TEM00 mode of about 2 percent of total power that appeared for a portion of the mode sweep cycle, but it’s occurrence did not coincide with the low level oscillation. LASOS tube ID #1 had a barely detectable non-TEM00 mode of about 0.05 percent, too small to be a factor. Any non-TEM00 modes in the other tubes were even smaller or non-existent.
  • Zeeman splitting: There are no magnets or magnetized material in the vicinity. Also, the amplitude of the oscillation is a maximum when a polarizer passes the entire center mode leaving no opportunity to combine two sub-modes in the PD. The mode itself could be split somehow into two sub-modes that cannot be resolved on the SFPI, but (1) there is no basic principle to support this, (2) it doesn’t explain how the side modes have the same frequency, and (3) that they are out of phase.
  • Plasma oscillations: While these may occur in the 100s of kHz range, they do not depend on mode position. And in addition, varying the power supply current has essentially no effect on the observed behaviour with respect to the low level oscillations.
  • Harmonics of the power supply ripple: Multiple power supplies have been tested with these tubes and there was absolutely no difference, as well as having no correlation to mode position.
  • Back-reflections: This is sort of grasping at optical straws, but to rule it out, I added wedge to the HR mirror on one Zygo tube that didn’t have it. This minimizes reflections from the uncoated outer surface of the mirror substrate from getting back into the cavity. As expected, there was no change.

While I believe the same phenomenon is responsible for these oscillations in LASOS and Zygo tubes, there are differences. Notably with the Zygo tubes, the frequency changes by almost 2:1 compared to only 20 kHz or so for the LASOS tubes. On one sample, ranging from around 200 kHz to 360 kHz. And compared to the LASOS tube where the two frequencies differed by almost 2:1 (around 280 and 500 kHz) they are similar enough for the Zygo tube that they may in fact be the same, but alternately increasing and decreasing depending on whether a p or s mode is in the center.

I’m sticking with mirror birefringence for now. It may be a feature, not a bug. 🙂 Specifically, that a higher birefringence coating on one or both mirrors is used to lock the polarization orientation, required to be able to use these tubes in stabilized He-Ne lasers, though I’m not sure LASOS and Zygo are that sophisticated!

The test to reproduce this phenomenon is relatively simple and doesn’t require fancy expensive instrumentation. The main components are a polarizer or polarizing beam-splitter, a biased silicon photodiode (almost any type will do using a circuit similar to what’s in a Thorlabs DET210 or DET10A (Google will find it), and an oscilloscope (almost any type since the frequencies involved are under 1 MHz). Terminate the output in 2k to 5k ohms and set the scope for a vertical sensitivity of a few mV/division, AC-coupled, and a sweep speed of a few µs/division. The tubes should be red (633 nm), random polarized, and healthy. (I have no idea what happens with other colour tubes!) They should be between 8 and 10 inches in overall length. Shorter tubes will have only 2 modes at most. Longer tubes with more modes may work, but that is left as an exercise for the student. 🙂 Since the signal is so low level – around 10mV even from a tube producing 3 or 4 mW, eliminating other sources of ripple and noise can be a challenge. Specifically, the current ripple from the He-Ne laser power supply may overwhelm and bury the low level oscillation signal. A highly filtered linear supply is best though some modern switchmode “bricks” have decently low ripple. And an external ripple reducer can be added to these. The photodiode will also need to be blocked from room light as the variation in intensity from lamp ballasts will be picked up. Power everything up and look for a clear oscillation in the 100s of kHz range that comes and goes, at a decreasing rate as the tube warms up. Rotate the tube over 45 degrees to align for maximum signal. If you have an SFPI, use a non-polarizing beam-splitter to sample a portion of the tube’s output for it to show how the oscillation correlates with the number of modes and their position. As noted above, only selected tubes exhibit this phenomenon and unfortunately, they are not the most commonly available ones. So your mileage – and success – may vary. 🙂

What is Mode Locking?

The normal output of a He-Ne or other CW laser is a more or less constant intensity beam. Although there may be long term variations in output power as well as short term optical noise and ripple from the power supply, these are small compared to the average intensity. Mode locking is a technique which converts this CW beam to a periodic series of very short pulses with a length anywhere from picoseconds to a fraction of a nanosecond. The separation of the pulses is equal to the time required for light to make one round trip around the laser cavity and the pulse repetition rate (PRF) will then be: c/(2*l). For example, a laser resonator with a distance of 30 cm (1 foot) between mirrors, would have a mode locked PRF of about 500 MHz.

Mode locking is implemented by mounting one of the mirrors of the laser cavity on a piezo-electric or magnetic driver controlled by a feedback loop which phase locks it with respect to the optically sensed output beam.

Without mode locking, all the modes oscillate independently of one another with random phases. However, with the mode locked laser, all the cavity modes are forced to be in phase at one point within the cavity. The constructive interference at this point produces a short duration, high power pulse. Destructive interference produces a power of almost zero at all other points within the cavity. The mode locked pulse then bounces between the two laser mirrors, and a portion passes through the output coupler on each pass.

As a practical matter, you probably won’t run into a mode locked He-Ne laser at a garage sale!

Cavity Dumped Pulsed He-Ne Laser

Here’s another one that won’t turn up at a swap meet. Inside the cavity of a typical He-Ne laser, the circulating power is 50 to 1,000 times the output power. If only all those photons could be accessed! Well, it turns out there is a way to do this sort of, at least in principle and for a short time. It’s called “cavity dumping”. The idea is use a high speed optical switch to briefly divert the Intra-Cavity (IC) beam outside the cavity. This sounds simple, right? 🙂 There are just a couple of problems. With the low gain of the typical He-Ne laser, any optics inside the cavity has to either be at the Brewster angle or have very good AR-coated surfaces so as not to significantly impact circulating power, or kill lasing entirely. And since any practical He-Ne laser is limited in size perhaps 2 meters at most, the switching has to take place in nanoseconds to get any significant fraction of the IC power to exit the laser.

The optical switch is the key to making this work. Either it has to actually deflect the beam or change its polarization so some other optical element will then reflect it out of the cavity. There are devices like Kerr cells and Pockels cells that could potentially be fast enough but they require high voltage to operate and may have excessive losses. Other approaches use an Acousto-Optic Modulator (AOM) as a deflector to divert the IC beam just enough to be reflected out of the cavity. However, AOMs don’t operate instantaneously since they depend on a high frequency acoustic wave to propagate in their crystal. Even a high performance AOM would require 10s or even 100s of nanoseconds to switch states.

I’m sure a literature search would turn up some mouldy papers describing the cavity dumping technique with a HeNe laser, but a “proof of concept” experiment was performed recently by Kevin Zheng, a very talented high school student, while at the Stony Brook Laser Teaching Center. See Kevin’s Research Journal and Poster. While the performance wasn’t that fabulous (forget any ideas of a hole burning HeNe laser!), just being able to get this work at all with relatively limited resources is impressive.

He-Ne Laser Output Power Fluctuation During Warmup

While not generally visible by eye alone except possibly for very short or tired (low gain) He-Ne lasers, there is a quasi-periodic variation of output power with time. For the typical He-Ne laser tube shortly after turn-on, the frequency is quite rapid (a cycle every few seconds) and gradually slows down as the tube temperature reaches a steady state value (after a half hour or more).

Note that while the frequency of the power variations in output power of a He-Ne laser goes to beyond the GHz range, the following deals with what can be seen by human eyeballs with the aid of only a photodiode and multimeter or chart recorder (or a PC with a data aquisition module).

Here is a plot of the measured output power of mid-size (probably around 5 mW) He-Ne laser tube from power-on to 20 minutes:

Typical He-Ne Laser Output Power Versus Time During Warmup
Typical He-Ne Laser Output Power Versus Time During Warmup

(Plot courtesy of Ryan Haanappel). (Though typically, the output power starts out at a much higher value, often above 75 percent of its value after full warmup. But there are exceptions.) Many more plots can be found later in this section.

Examining the actual plot of output power versus time such as shown below:

He-Ne Laser Output Power Fluctuation During Warmup
He-Ne Laser Output Power Fluctuation During Warmup

(or careful observation of laser power meter readings) of a He-Ne laser reveals that the curve is not simple but may include several types of behaviour:

  • Long term trend in output power: With a laser that is in good condition, this is a generally increasing function until it levels off after warmup. The dominant effect is that as the laser tube heats, various parts expand and the laser approaches optimal alignment (which should have been the way it was originally adjusted during manufacture). If the mirror alignment is not quite correct, power may go up and then down, or just down, and/or may never reach rated power. If the cause is alignment, gently pressing side-ways on one of the mirror mounts at the correct angle with the correct force (with an insulated tool!) should result in near maximum power even when just powered on.There is also usually an increase of power due to the heating of the laser tube (independent of thermal expansion effects) as well. But this may be only a fraction of the effects of alignment and is related to the increase in internal temperature and pressure.In addition, especially with soft-seal tubes, there may be a power increase as the cathode, acting as a weak getter, removes contaminants from circulation that may have accumulated from a period of non-use. Or depending on how far gone they are, the power may go down as various parts outgas from the heat!Depending on the particular laser, the initial output power can be very low even where the final output power exceeds rated power. Striking examples can be found in a non-negligible percentage of long JDS Uniphase He-Ne lasers like the 1145P. With these, a cold power of 1 or 2 mW for a laser that reaches 24+ mW after 20 minutes isn’t unheard of. The dominant cause is a change in mirror alignment.
  • Short term variations in output power: As the laser tube heats and expands, the longitudinal modes of the laser drift across the 1.5 GHz neon gain curve. The output power varies depending on where they are and may change suddenly as a mode drops off one end or appears at the other. For a 6 inch tube (c/2L=0.5 GHz), there are 1 or 2 active modes; for a 24 inch tube (c/2L=125 MHz), there may be 8 or 10 active modes. The short tube will usually have much more dramatic variations in power due to this mode cycling. Specifications range from 20 percent (for 5 inch tubes) to less than 2 percent for long ones. For a short random polarized tube, the polarized modes may vary by 100 percent. Note that the variations may not be of a single frequency but often exhibit the double-dip behaviour shown in the plot, above. This is probably due to the number of modes oscillating and how they are centered on the gain curve. There may also be a slight difference on alternate cycles due to the polarizations of adjacent modes seeing slightly different gain.These effects are collectively called “mode sweep” or “mode cycling”. Plotting and analyzing this behaviour for various tubes under a variety of conditions can be quite fascinating. More in the next section.
  • Medium term variations in output power: (These are generally less common with lasers that are properly designed and manufactured.) There are two common types of medium term effects:
    1. IR Mode competition: This is generally only a problem with higher power lasers. It is usually at the high gain 3.39 um mid-IR He-Ne lasing wavelength and may result in an additional variation in output power. While longer tubes generally are designed with mirror coatings highly transparent at the 3.39 um wavelength and/or with IR suppression magnets, their effect isn’t always perfect. These power variations will be at a frequency 0.633/3.39 (for 633 nm, red He-Ne lasers) of the fundamental frequency of the primary mode cycling, above. The effect will be negligible for red He-Ne lasers of less than 15 or 20 mW but may appear in relatively short “other colour” (e.g., yellow) He-Ne lasers due to the low gain of the lasing wavelength. A simple test is to carefully place a few reasonably powerful magnets at several locations near the tube. If the problem is mode competition, the amplitude of the variations should be reduced and output power at the design wavelength may increase by 10 or 20 percent or more. Modern He-Ne lasers rarely suffer from IR mode competition.
    2. Non-wedged mirror substrates: Another source for power variations on a similar time scale is a lack of wedge in the HR and/or OC mirror glass substrates. Wedge means that the two surfaces are ground at a slight angle. Without wedge, the mirror coating and the uncoated outer surface (HR) or AR-coated outer surface (OC) form an etalon whose transmission varies as the glass expands during warmup due to constructive and destructive interference within the mirror glass. The result is that the power of the waste beam from the HR mirror may vary periodically by an amount much larger than that of the mode sweep specification, and it doesn’t track the power of the main beam as would be expected. Lack of wedge for the HR mirror is particularly nasty since the approximately 4 percent Fresnel reflection from the outer suface is enough to vary the transmission through the HR – and thus the waste beam power – by a ratio of up to 2.25:1. Waste beam power variation due to lack of wedge for the OC mirror is less severe since the AR coating results in less reflection but still may be 10 percent or more. While most applications don’t care what the waste beam does, there may also be ripples in the main beam of 1 or 2 percent. These will be superimposed on all the other power variations described above. For an enclosed cylindrical laser head, there may be up to 10 or more of these power variation cycles while a bare tube will go through fewer cycles because its temperature increase is not as great. These small power variations may be considered normal behaviour for short tubes where it is much less than those due to mode sweep, and no one (at least almost no one!) cares what the waste beam does. Mass produced barcode scanner tubes – built for low cost, not highest performance – are most likely to have this problem but many of them not too bad. Higher quality tubes will have both made with wedged substrates. Plots of power output during warmup for a few typical cases are also shown below.

Goofups in design and manufacturing can result in various combinations of these and other effects, though for the most part, He-Ne laser companies generally know what they are doing! 🙂 But see the plots below for both normal and abnormal behaviour, and a link near the end of the section for a case study of one dramatic example of an “oops”. 🙂

Plots of HeNe Laser Power Output and Polarized Modes During Warmup

Here are some plots of power output versus time for a variety of typical He-Ne laser tubes and heads from nearly the shortest available through mid-size. (For longer tubes, the appearance will be very similar, but with even a smaller short term fluctuation in power.) The shape of the plots is mostly the result of what’s called “mode sweep” or “mode cycling” as the longitudinal modes of the laser move with respect to the neon gain curve due to thermal expansion of the laser cavity. However, where the plot covers a long time (e.g., most of the warmup period), there will generally be an increasing trend in output power due to other factors as noted above.

Most of these are from Melles Griot but the behaviour of lasers from other manufacturers will be relatively similar, though the detailed shape of the individual polarized modes (more below) can differ significantly. The majority are healthy samples but a few show some rather dramatic peculiarities. There are also plots of a Coherent model 200 and Hewlett Packard model 5517A frequency stabilized He-Ne lasers from power-on to locking.

Plots such as these are almost like fingerprints for He-Ne lasers. Many of the physical characteristics of the laser can be determined by their appearance, and some features are unique to a particular model or manufacturer.

For most of the plots, my “instrumentation” consisted of a pair of $2 photodiode feeding two of the analog inputs of a DATAQ RS232 Chart Recorder Starter Kit attached to my ancient 486DX-75 Kiwi laptop running Win95. The photodiodes are reverse biased by 30VDC from a +/-15VDC power supply with a variable load resistor to set the calibration. The output is taken between the junction of the resistor and the photodiode, and power supply common (0 VDC). One channel is shown below:

The values shown were selected for lasers with a maximum power output of around 1 mW. For higher power lasers, R2+R3 can be decreased or an attenuation filter can be placed in the beam. The later is preferred to avoid shifting the 0 mW reference level, and is what I did for most of the plots.

The capacitor across the input is intended to minimize noise pickup. The resulting filter rolls off at around 0.1 Hz. For reasonably well behaved He-Ne lasers, even during the initial warmup period, this bandwidth is more than adequate. The sampling rate for all the plots is at least 10 Hz to allow for averaging since the A/D seems to have an uncertainty of about 2 LSBs.

In most cases, the two photodiodes are positioned at the outputs of a Polarizing Beam-Splitter (PBS) cube and the laser tube is oriented so that they are aligned with its natural polarization axes.

For monitoring power from the waste beam (which is much lower), a dedicated beam sampler assembly was constructed, which along with a photodiode preamp, enabled power levels as low as a few uW to fully utilize the 20 V p-p range of the A/D.

Some of the plots have been acquired with the same photodiodes, but feeding a dual channel preamp and also a summer tp compute the total power without requiring a separate photodiode channel. (Of course, for this to be meaningful, the photodiodes and premaps have to be set up so the two channels have equal gain.) The premap results in lower noise in the plots especially for low power lasers.

And as of 2011, I’ve “upgraded” to USB versions of the DATAQ device (DI-158U and DI-145) and laptops that are only 10 years old. 🙂 The original DATAQ RS232 module died and the Kiwi laptop doesn’t have USB and is falling apart (though is still usable). The PDs are now each attached to a general purpose trans-impedance amp rather than the simple bias network. [See the section: Sam’s Photodiode Preamp 1 (SG-PP1).] And in addition to channels 1 and 2, the outputs also feed a pair of resistors and a pot to adjust balance to channel 3 so their sum (which would usually be total power) is always present.

Although some of these plots aren’t as nicely annotated as the one above, zero power is near the bottom of the plot so relative power variations can still be easily seen (who cares about absolute power anyhow!) and the time/division is indicated. The plots are arranged by increasing laser tube length.

For the following, “Total” means all the power in the beam; “Polarized” means a polarizing beam-splitter is used to separate the two orthogonally polarized modes with either one or both plotted. (This is Only done for random polarized lasers.) The scale factor for the “polarized” plot has been adjusted so that the peak amplitude is approximately the same as for the “total” plot for ease of viewing. However, it should be understood, that the sum of the power in the two orthogonal polarizations must add up to the total power. All are red (632.8 nm) HeNe lasers unless otherwise noted.

Note: I have “edited” (doctored?) some of the plots to clean up unsightly randomness and other blemishes, mostly due excessive electrical noise at low optical power levels. However, the important features are unchanged.

  • Plot of Melles Griot 05-LHR-007 He-Ne Laser Tube During Warmup.
    Plot of Melles Griot 05-LHR-007 He-Ne Laser Tube During Warmup

    This is the shortest commercial HeNe laser I know of with a total length of about 4-5/8 inches. The rated output power is 0.5 mW but this sample produces about 0.8 mW. Only 2 longitudinal modes will be oscillating with a mode sweep of about 10 percent. The large peaks correspond to a single mode being at the center of the gain curve. If the distance between the mirrors were much shorter, it wouldn’t be possible for even 2 modes to coexist and the output would turn off for a portion of the mode cycle. Note that the actual tube tested was a Siemens 007 but it has identical specs to the Melles Griot 05-LHR-007 so I figured it’s better to be consistent. 🙂 It was necessary to construct a tent over this (and other) bare tubes to even get this far without random air currents affecting the temperature too much. (The peaks beyond 20 minutes where this and the next run terminated were unrecognizable!) An enclosed laser head would take much longer to stabilize but be more tolerant of ambient conditions.

  • Plot of Melles Griot 05-LHR-007 He-Ne Laser Tube During Warmup (Polarized)
    Plot of Melles Griot 05-LHR-007 He-Ne Laser Tube During Warmup (Polarized)

    This is the same tube but with a non-polarizing beamsplitter followed by orthogonal polarizing filters inserted in the beam. The orientation of the polarizing filters is adjusted for minimum transmission when its mode is not present since as can be seen, the power actually goes to 0 mW for about half the period of each polarized mode. Alternate similar height peaks on the total power plot correspond to the same mode polarization. A careful examination will confirm that they actually alternate very slightly in amplitude due to minor variations in gain as a function of polarization. (I have adjusted the scale factors to make the plot looks similar.) The reason why the peak spacing on the two plots differs is that the tube was likely not quite at the same temperature when each run was started.

  • Plot of Melles Griot 05-LHR-640 He-Ne Laser Tube During Warmup
    Plot of Melles Griot 05-LHR-640 He-Ne Laser Tube During Warmup

    The 05-LHR-640 is very nearly second shortest commercial HeNe laser tube as shown below

    Melles Griot 05-LHR-640 He-Ne Laser Tube
    Melles Griot 05-LHR-640 He-Ne Laser Tube

    It is only about 5 inches in total length and as with the 05-LHR-007, only 2 longitudinal modes are oscillating. The rated output power is 0.5 mW but this sample produces about 1.2 mW. As can be seen in this plot, the “mode sweep percentage” is still rather modest – about 5 to 7 percent. The specification for this tube allows for up to 20 percent. This bare He-Ne laser tube has nearly fully stabilized in under 20 minutes.

  • Plot of Melles Griot 05-LHR-640 He-Ne Laser Tube During Warmup (Polarized)
    Plot of Melles Griot 05-LHR-640 He-Ne Laser Tube During Warmup (Polarized)

    . This is the same tube with the polarized modes separately plotted. Similar comments apply for this tube as for the 05-LHR-007, above.

  • Plot of Melles Griot 05-LHR-640 He-Ne Laser Tube During Warmup (Polarized)
    Plot of Melles Griot 05-LHR-640 He-Ne Laser Tube During Warmup (Polarized)

    Above shows the two polarized modes and total power in a laser with a cavity length of about 7 inches. This is just about at the point where 3 modes can barely lase simultaneously when one is centered on the neon gain curve.

  • Plot of Melles Griot 05-LHR-640 He-Ne Laser Tube During Warmup (Polarized)
    Plot of Melles Griot 05-LHR-640 He-Ne Laser Tube During Warmup (Polarized)

    This uses a slightly longer tube – almost 8 inches – which probably supports three simultaneous lasing modes. The rated output power is 1.5 mW but this sample produces about 2.0 mW. Since the 05-LHP-131 is a polarized laser, the polarization of all modes in the output beam is the same. As the length of the laser tube increases, the amplitude of the short term power variations will tend to decrease – for this laser head, it is under 2 percent. This is actually quite good – well below the 10 percent in the specifications. Being an enclosed laser head, even after 30 minutes, the power hasn’t fully stabilized.

  • Plot of Spectra-Physics 088 He-Ne Laser Tube During Warmup
    Plot of Spectra-Physics 088 He-Ne Laser Tube During Warmup

    This is a slightly longer random polarized tube, about 8.5 inches between mirrors. In addition to having been used by the hundreds of thousands in barcode scanners peaking during the 1980s, tube like this was used in the Spectra-Physics 117 and SP-117A (and similar Melles Griot 05-STP-901) stabilized HeNe laser. Note the well behaved mode sweep with smoothly varying polarization components and no flipping. A closeup is shown below

    Plot of Spectra-Physics 088 He-Ne Laser Tube During Warmup (Detail)
    Plot of Spectra-Physics 088 He-Ne Laser Tube During Warmup (Detail)
  • Plot of Siemens LGR-7641 He-Ne Laser Tube With Variable Waste Beam Power During Warmup (Uncorrected)
    Plot of Siemens LGR-7641 He-Ne Laser Tube With Variable Waste Beam Power During Warmup (Uncorrected)

    While nearly identical in length to the SP-088, note the dramatic difference in the shape of the mode waveforms. Each is nearly a perfect triangle wave like the Melles Griot 05-LHR-911, above. This is especially evident near the end of the warmup period but it is very similar throughout. This shape seems to be characteristic of all these Siemens tubes as I’ve tested several with essentially the same mode waveforms. The mode shape of the Uniphase 098, another barcode scanner tube, is identical. The resonator length of the 088 and 098 is virtually identical, while that of the LGR-7641 is about 1/8″ longer. The cause is unknown but based on this, it doesn’t seem to be related to the size. A wild guess would be that it has something to do with the isotopic purity (or lack thereof) or ratio of the gas-fill resulting in a wider neon gain curve curve so that as with the 05-LHR-911, 3 longitudinal modes can just barely lase simultaneously when one is centered.However, the dramatic variation in mode amplitude over the course of warmup is an artefact of the way that data is being collected for this run and a peculiarity of the tube that doesn’t noticeably affect its useful output. Rather than using the output beam, the P and S Modes are taken from the waste beam leaking through the HR mirror at the back of the laser. The Total Power (Waste) is then simply the sum (in an op-amp) of the modes. Compare this to the Total Power (Output) curve, which was measured from the main beam. The cause of the rear beam power variation is interference from multiple internal reflections in the HR mirror glass – between the HR coated inner surface and the uncoated outer surface. The result is a weak Fabry-Perot etalon which varies the effective reflectance of the HR mirror. It doesn’t take much: A change from 99.975% to 99.95% would double the waste beam power – from about 15 uW to 30 uW. The 15 uW lost from the main beam power of about 1 mW is almost undetectable on the plot. The HR mirror glass is apparently not wedged on these tubes so the surfaces are very parallel. And indeed there was no ghost beam next to the waste beam as would be the case if wedge was present. The cause was confirmed by putting a dab of 5 minute Epoxy on the outer surface of the mirror. The Epoxy is smooth and clear enough to pass sufficient power for the photodiodes (though it is reduced), but the Epoxy surface is lumpy enough to greatly reduce the power variation. Why? The glass and Epoxy are fairly closely index matched so that the dominant reflection is no longer from the planar glass surface but from the lumpy surface of the Epoxy. There is minimal reflection directly back along the optical axis and thus minimal etalon effect resulting in a reduction of power variation from nearly 100 percent to under 10 percent. Using Norland 65 UV cure optical cement to glue an angled plate to the HR mirror reduced the ripples even more as shown below.

    Plot of Siemens LGR-7641 He-Ne Laser Tube With Variable Waste Beam Power During Warmup (Uncorrected)
    Plot of Siemens LGR-7641 He-Ne Laser Tube With Variable Waste Beam Power During Warmup (Uncorrected)

    .

  • Plot of Uniphase 098 He-Ne Laser Tube With Waste Beam Power Variation During Warmup (Bare, Uncorrected)
    Plot of Uniphase 098 He-Ne Laser Tube With Waste Beam Power Variation During Warmup (Bare, Uncorrected)

    is another similar (basically interchangeable) barcode scanner tube with the same malady as the LGK-7641: No HR wedge and large variation in waste beam power due to etalon effects. Insulating the same tube by installing it in a head cylinder allows for several cycles of the waste beam variation as shown below:

    Plot of Uniphase 098 He-Ne Laser Tube With Waste Beam Power Variation During Warmup (Insulated, Uncorrected)
    Plot of Uniphase 098 He-Ne Laser Tube With Waste Beam Power Variation During Warmup (Insulated, Uncorrected)

    A close examination of the Total Power (Measured) shows small dips representing the power being stolen by the waste beam from main beam! The measured output power is about 1 mW. The amplitude of the waste beam power variation for this tube is from around 5 uW to 10 uW.

  • Plot of Melles Griot 05-LHR-006 He-Ne Laser Tube #1 With Waste Beam Power Variation During Warmup (Insulated, Uncorrected)
    Plot of Melles Griot 05-LHR-006 He-Ne Laser Tube #1 With Waste Beam Power Variation During Warmup (Insulated, Uncorrected)

    and

    Plot of Melles Griot 05-LHR-006 He-Ne Laser Tube #2 With Waste Beam Power Variation During Warmup (Insulated, Uncorrected)
    Plot of Melles Griot 05-LHR-006 He-Ne Laser Tube #2 With Waste Beam Power Variation During Warmup (Insulated, Uncorrected)

    are examples of common short (6 inch) Melles Griot barcode scanner tubes with varying degrees of the same problem. #1 has nearly the theoretical maximum waste beam power variation ratio of 2.25:1.

  • Plot of Melles Griot 05-LHR-006 He-Ne Laser Tube With Minimal Waste Beam Power Variation During Warmup (Insulated, Uncorrected)
    Plot of Melles Griot 05-LHR-006 He-Ne Laser Tube With Minimal Waste Beam Power Variation During Warmup (Insulated, Uncorrected)

    shows the behaviour of another virtually identical short (6 inch) tube with a small amount of wedge. But it’s enough to virtually eliminate power fluctuations in the waste beam. The residual ripples may actually be due to lack of wedge in the OC mirror and adding an angled plate to the OC mirror with optical cement actually made the ripples larger as shown below

    Plot of Melles Griot 05-LHR-006 He-Ne Laser Tube With Moderate Waste Beam Power Variation During Warmup Due to Messed Up OC AR Coating (Insulated, Uncorrected)
    Plot of Melles Griot 05-LHR-006 He-Ne Laser Tube With Moderate Waste Beam Power Variation During Warmup Due to Messed Up OC AR Coating (Insulated, Uncorrected)

    . This is somewhat as expected since it’s not possible to index match to an AR-coated surface without removing the AR coating. So, the reflections there would increase.

  • Plot of Uniphase 1007 He-Ne Laser Tube With Minimal Waste Beam Power Variation During Warmup (Insulated, Uncorrected)
    Plot of Uniphase 1007 He-Ne Laser Tube With Minimal Waste Beam Power Variation During Warmup (Insulated, Uncorrected)

    has even less. But another Uniphase tube had among the worst case as shown in

    Plot of Uniphase 1007 He-Ne Laser Tube With Large Waste Beam Power Variation During Warmup (Insulated, Uncorrected)
    Plot of Uniphase 1007 He-Ne Laser Tube With Large Waste Beam Power Variation During Warmup (Insulated, Uncorrected)

    These were identical model numbers used in the identical barcode scanners.

  • Plot of Melles Griot 05-LHR-151 He-Ne Laser Head During Warmup
    Plot of Melles Griot 05-LHR-151 He-Ne Laser Head During Warmup

    This is a very common medium size HeNe laser with a tube about 13 inches in length so 4 or 5 modes are oscillating. The rated output power is 5 mW but this sample produces about 7.5 mW. The power fluctuations are virtually undetectable on these plots – well under 1 percent.

  • Plot of Melles Griot 05-LHR-151 He-Ne Laser Head During Warmup (Polarized)
    Plot of Melles Griot 05-LHR-151 He-Ne Laser Head During Warmup (Polarized)

    This is the same laser head but with the two orthogonal polarizitions separated (as described for the shorter tubes, above) and oriented for maximum variation (“ripple”). They are plotted separately to reduce clutter. Since there are always modes of both polarization present regardless of polarizer orientation, the output power in doesn’t go to zero as with the shorter laser but their ripple is almost perfectly complementary. As expected, the size of the fluctuations in each polarization – 5 to 10 percent – is more in line with the total power behavior of a laser with only 2 or 3 modes. Even this amplitude seems remarkable given the almost perfectly smooth behavior of the total (randomly polarized) power. If the plots are examined very carefully, it will be noted that their envelopes are not identical – there is a very subtle slow variation over the course of the warmup period. This may be attributed to a small rotation of the polarization axes as the tube expands. With some samples of these lasers, it can be much more dramatic including polarization flips whenever it feels like it. But such behavior is still considered normal since for a random polarized laser, only the total power really matters, not any peculiar gyrations the modes may go through.

  • Plot of Normal Melles Griot 05-LYR-173 He-Ne Laser Head During Warmup
    Plot of Normal Melles Griot 05-LYR-173 He-Ne Laser Head During Warmup

    This is a typical yellow (594.1 nm) HeNe medium-long HeNe laser. The rated output power is 2.0 mW but this sample produces about 4.1 mW. Due to the low gain of the yellow lasing line, the amplitude of the power fluctuations is somewhat greater than for even the slightly shorter 05-LHR-151 red laser, above.

    Plot of Melles Griot 05-LYR-173 He-Ne Laser Head During Warmup (Polarized)
    Plot of Melles Griot 05-LYR-173 He-Ne Laser Head During Warmup (Polarized)

    The same laser with a polarizing filter in the beam. The fluctuations are larger as expected both because of the fewer modes in the polarized beam, and the lower gain of the 594.1 nm lasing line.

  • Not all lasers are manufactured properly. For example, one sample of a laser similar to the 05-LYR-171 exhibits a slow large amplitude oscillation in power. Compare:
    Plot of Variable Melles Griot 05-LYR-171 He-Ne Laser Head During Warmup
    Plot of Variable Melles Griot 05-LYR-171 He-Ne Laser Head During Warmup

    and

    Plot of Variable Melles Griot 05-LYR-171 He-Ne Laser Head During Warmup (Polarized)
    Plot of Variable Melles Griot 05-LYR-171 He-Ne Laser Head During Warmup (Polarized)

    with the plots above. The plots in blue are for the normal output beam from the front (OC) of the laser. The plots in red are for the excessively large waste beam from the rear (HR) of the laser – a clue to the part of the cause of the power oscillations. That has to be one spectacular screwup. I wonder how many laser heads were built that way. 🙂

  • Plot of Coherent Model 200 Stabilized He-Ne Laser Head During Warmup
    Plot of Coherent Model 200 Stabilized He-Ne Laser Head During Warmup

    . Finally, here is how a laser with active mode stabilization behaves. This laser is designed to provide a single longitudinal mode output with a frequency stability on the order of 1 MHz. Since the laser head has optics to separate the modes with orthogonal polarization, the raw beam already varies by more than 2:1 in output power without any additional polarizer. Yes, that is the actual spread – the vertical scale hasn’t been stretched! The actual HeNe laser tube inside is a specially selected Melles Griot 05-LHR-120, which by itself would have a normal mode sweep with a small ripple. From a cold start to lock takes about 20 minutes.

    Plot of Coherent Model 200 Stabilized He-Ne Laser Head Near End of Warmup
    Plot of Coherent Model 200 Stabilized He-Ne Laser Head Near End of Warmup

    This plot zooms in on the last two cycles. Notice that there is a slight distortion on the rising part of the second cycle in the plot. That is probably when the active feedback is switched on. Before then, the heater is simply running at a constant current to bring the tube up to operating temperature. It only takes less than one full additional cycle to achieve lock. The amplitude is then quite stable (uncertainty of less than 0.5 percent on the plot), but the frequency stability which is d(power)*slope(frequency/power), will be under 0.125 percent of the mode spacing of around 750 MHz, so less than 1 MHz.

  • Plot of Hewlett Packard Model 5517C Stabilized Laser During Warmup
    Plot of Hewlett Packard Model 5517C Stabilized Laser During Warm up

    Above shows how another even more highly stabilized (or at least more expensive!) laser behaves. Note that the entire warm up period from laser on to locked is only around 3.5 minutes because the heater for the active mode control is inside the laser tube, wrapped directly around the bore. The control algorithm during warm up is also a bit more sophisticated, pausing periodically to determine the “mirror spacing rod” temperature by measuring the heater resistance, and entering a “fine adjust” mode about half way through. In fact, from the relative shapes of the red and blue mode cycles, it can be seen that for this particular laser, during most of the time from power on (a cold start) to lock, the tube is heating (about 75 cycles), but it switches to steady cooling (about 6 cycles) just before locking.

  • Plot of Hewlett Packard Model 5517C Stabilized Laser Near End of Warmup
    Plot of Hewlett Packard Model 5517C Stabilized Laser Near End of Warm up

    Above shows the 5 mode cycles just before locking and the final transition to the locked state. The peculiar shape of these Zeeman-split modes is clearly evident in this expanded view.The actual beat frequency is shown for the last few cycles and after locking in both these plots. This is the actual measured frequency captured along with the F1 and F2 modes, and total output power. (Showing the frequency plot earlier would be a mess.) The beat only appears for a small percentage of the mode cycles with some variation during the time it is present. The warm up and locking algorithm is partially responsible for the distorted nature of these plots compared to those for “normal” unstabilized He-Ne lasers or even other common stabilized He-Ne lasers due to the periodic pauses and switching from heating to cooling that may occur. However, the peculiar shape of the mode cycles themselves is due to the fact that these are not linearly polarized modes as with all the previous lasers. Rather, they are Zeeman-split modes distorted by a magnetic field and include (mostly) components differing in frequency by at most a few MHz, rather than the normal longitudinal mode spacing, which is 1.2 GHz for this laser.

  • Plot of "Flipper" Aerotech OEM1R He-Ne Laser Head During Warmup
    Plot of “Flipper” Aerotech OEM1R He-Ne Laser Head During Warmup

    This is a very naughty laser. 🙁 🙂 As can be seen, for most of the mode cycles during the warm up period, rather than the two orthogonal polarizations (called P and S) changing smoothly as they cycle, each one moves to a distinct point and then instantaneously swaps places with the other one. Tubes with flipper behaviour will generally not be useful for a stabilized He-Ne laser but may be perfectly satisfactory when simply used as a light source without polarizing optics.However, near the very end of the warm up period (measured in terms of mode cycles, not time) something very interesting occurs: The tube seems to have reverted to being well behaved! This only happens when the tube is approaching thermal equilibrium where each complete mode cycle is taking over 90 seconds. There are perhaps 3 or 4 beyond what is on the plot but the tube temperature is so close to its final value that any disturbance like moving near the laser head will disrupt the sequence. This behaviour is consistent from run to run. The cause is unknown, nor is it known whether the tube would continue to behave if stabilization was attempted. But it might since the operating temperature will be somewhat above the natural point of thermal equilibrium.

    Plot of "Flipper" Aerotech OEM1R He-Ne Laser Head During First Part of Warmup
    Plot of “Flipper” Aerotech OEM1R He-Ne Laser Head During First Part of Warmup

    Above is a close up of the mode variations when flipping. The shapes are nearly identical from the start of warm up until the transition to normal behaviour. Also note that the frequency of the mode cycles for a flipper is double that of a normal tube – each mode would normally be what resulted from tracing the continuous curve and not taking the discontinuities as is evident below:

    Plot of "Flipper" Aerotech OEM1R He-Ne Laser Head During First Part of Warmup (Combined)
    Plot of “Flipper” Aerotech OEM1R He-Ne Laser Head During First Part of Warmup (Combined)

    So following red-blue-red, etc., ignoring the green lines.

    Plot of "Flipper" Aerotech OEM1R He-Ne Laser Head at Transition to Normal Behaviour (Combined)
    Plot of “Flipper” Aerotech OEM1R He-Ne Laser Head at Transition to Normal Behaviour (Combined)

    Above is a closeup of the point where flipping ceases. Note that the “envelope” of the mode plot is virtually unchanged at this point but the green transitions have disappeared. At the transition point, the period of a full mode sweep cycle is about 80 seconds. There are then an additional 10 full cycles (only 4 or 5 are shown) requiring about an hour until thermal equilibrium.

  • Plot of "Flipper" Aerotech OEM1R He-Ne Laser Head During Warmup
    Plot of “Flipper” Aerotech OEM1R He-Ne Laser Head During Warmup

    Above is an example of consistent flipper behavior. The character of the plot does not change from power-on to full warmup. There is a consistent flip at the same point in the mode sweep cycle. Interestingly, there is a slight asymmetry in the mode sweep envelope, unusual for most HeNe lasers. Whether this has any profound cosmic significance is unknown. 😉 These tubes were found in some barcode scanners due to their physical robustness – They could fall on the floor – or probably be used as hammers – without sustaining any damage! See the section: Metrologic Steel-Ceramic Hard-Seal He-Ne Laser Tubes.

These have all been high quality HeNe lasers and except as noted, have relatively predictable mode performance. For information and plots for a really ill-mannered beast, see the section: Far East HeNe Laser Tubes.

Mode Competition in Short He-Ne Lasers

If you haven’t been wondering why some of the output power plots are so strange, you should be. 🙂

The primary reason that the output power in any give longitudinal mode doesn’t vary in a nice smooth (Gaussian) manner is due to mode competition. If not for mode competition, the gain would not saturate and be the same for all modes. Everyone would thus trace out the envelope of the neon gain curve. However, since the lasing modes are actually competing for a limited resource – the atoms in the upper lasing state – whenever there are more than one mode present, they have to be nice and share. This is most dramatic when only 2 or 3 modes are present since each one has a large fraction of the total output power. With those, the shapes of the envelopes of the polarized output power curves can be decidedly non-Gaussian. And for Zeeman-split lasers, downright weird. But once the various regions are understood – where there are 1, 2, 3, or more modes competing – then the resulting shapes make more sense:

1 mode: The output power will change smoothly during mode sweep roughly following the profile of the Gaussian neon gain curve (minus the lasing threshold). The only way a real laser could be single mode throughout mode sweep would be either for the cavity to be around 10 cm or less (in which case lasing may cease entirely for a part of mode sweep) or for there to be an additional means of forcing SLM operation (such as an etalon inside the cavity). But slightly longer tubes will operate with a Single mode over a portion of mode sweep with 2 modes for the remainder.

Plot of Mode Sweep of Typical 1 mW Random Polarized He-Ne Laser Tube shows the appearance for a Melles Griot 05-LHR-007, the shortest modern laser tube I’m aware of. Over approximately 50 percent of the mode sweep cycle, it is pure single mode with power sharing during the remainder.

2 modes: When a second mode appears, it will start eating into the power of the first mode. Where the modes are balanced on either side of the neon gain curve, their power will be equal. Between these 2 points, they will share power. The total output power may remain relatively constant or increase slightly when equal (usually up to around 20 percent). Tubes with a cavity length of 12 to 16 cm will operate with 1 or 2 modes.

3 modes: When a third mode appears, it will start eating into the power of the other two. The relative and total power will depend on their location on the neon gain curve and is at the very least, not intuitively predictable. 🙂 Tubes with a cavity length of 20 to 25 cm will operate with 2 or 3 modes during mode sweep.

Plot of Mode Sweep of Typical 3 mW Random Polarized He-Ne Laser Tube shows the appearance for a Spectra-Physics 088 (same as the Melles Griot 05-LHR-088) used in the SP-117/A/B/C and Melles Griot 05-STP-901 stabilized lasers. It is similar a common barcode scanner tube. At the peaks of the polarized modes (minimum for total power), there are 2 modes. Where the polarized modes cross, there are 3 modes. The overall shape of the mode sweep depends on many factors including the exact length of the cavity which determines where it switches from 2 to 3 modes.

4 or more modes: The same general rules apply, but since the contribution of each mode is smaller, the effects of mode competition are also smaller and more difficult to see and interpret.

Inhomogeneous Broadening in Neon and Mode Sweep

The shape of the neon gain curve is by now familiar, but what does it really mean? The popular notion of it being the result of some magical process is fine as a first step, but doesn’t help in attempting to understand how it is affected by wavelength, or for explaining phenomena like the Lamb Dip.

What is really being depicted in the gain curve is a combination of a curve derived from what’s called the “natural line width of neon” which is homogeneously broadened, and the distribution of atomic velocities of excited neon atoms as they translate into a distribution of Doppler shifts in optical frequency.

Ignoring Special Relativity (which is acceptable for the velocities involved), the Doppler shift in optical frequency is equal to the relative velocity of the excited atom divided by the speed of light multiplied by the optical frequency or:

Where:

  • Δf is the optical frequency shift.
  • f0 is the original optical frequency.
  • va is the velocity of an atom in the upper lasing energy state relative to a photon traveling along the axis of the laser tube.
  • c is the speed of light.

At any temperature above absolute zero, all atoms are in motion and have a probabilistic distribution of velocities (speed and direction), which all contribute to the Doppler broadening. For a Fabry-Perot (linear) cavity, the photons traveling in either direction “experience” the relative speed of the excited atoms. Stimulated emission will only occur when the Doppler-shifted energy of the photon matches a possible lasing transition of an excited atom. The width of the Doppler broadening is directly proportional to optical frequency, but it is also affected by other factors including temperature and pressure, since these impact the distribution of atomic velocities. The shape of the Doppler broadening curve is then the result of the aggregate of the motion of all the atoms available for stimulated emission. And the width of the inhomogeneously broadened neon gain curve is the width due to homogeneous line-width of neon plus the inhomogeneous Doppler broadening. Since they are added like independent noise souces using the square-root of the sum of the squares, the increase in neon gain bandwidth due to the homogeneous line-width is quite small (just over 5 percent even at 3,391 nm). Thus, the change is close to 1/5th even if the homogeneous part is ignored.

Assuming the FWHM value of 1.6 GHz for the entire inhomogeneously Doppler-broadened gain bandwidth of the common red wavelength of 632.8 nm, at the mid-IR wavelength of 3,391 nm it is only 315 MHz. And at the green wavelength of 543.5 nm it is about 1.86 GHz. The optical frequency difference between cavity modes (c/2L) is only dependent on cavity length and the speed of light. Thus, the number of lasing modes possible for a given cavity length decreases as the gain bandwidth becomes narrower at longer wavelengths.

Note that the lasing modes themselves will have a very narrow bandwidth – possibly as small as 5 kHz or even lower for a laser operating with a single mode. At that point, physical vibrations, laser power supply noise, and other external effects are the limiting factors, not the theoretical minimum bandwidth for the HeNe laser which is under 1 Hz! (Schawlow-Townes linewidth). I originally thought that finding values for the bandwidth of commercial HeNe lasers would be straightforward, but it seems to be near impossible. The only specifications I am aware of from a laser manufacturer are in Laboratory for Science brochures. The best is for their model 220 Ultra Stable HeNe laser, which lists 5 kHz over a period of 1 second. But the value for the type of HeNe laser tube that used to be found in barcode scanners may not be all that much greater if it is mounted to minimize vibrations and driven with a well filtered HeNe laser power supply.

One would expect that with the much smaller gain bandwidth at 3,391 nm of 315 MHz, there would be fewer longitudinal modes oscillating compared to 632.8 nm. Or equivalently, a laser tube would need to be much longer for the same number of modes to fit within the FWHM of 315 MHz. But because of the very high gain at 3,391 nm, the lasing threshold will be lower and thus the effective gain bandwidth of the neon gain curve is going to be wider. I do not know by how much, but with a potential gain over 40 times that of the 632.8 nm transition, it could be very significant. There might even be more modes than at 632.8nm.

Due to the longer wavelength, mode sweep for a laser tube at 3,391nm will have a complete cycle that is over 5 times as long as one at 632.8nm. These same numbers would apply to mode competition at 3,391 nm interfering and stealing power from a 632.8nm laser.

Number of Longitudinal Modes at Other He-Ne Wavelengths

As described above, the gain bandwidth of neon is roughly inversely proportional to the wavelength (or proportion to the frequency) of the lasing transition. However, this assumes that the lasing threshold is at the same location relative to the peak of the neon gain curve, often specified as the Full Width Half Maximum or FWHM. At 632.8nm, this turns out (not coincidentally!) to be reasonable and results in the expected number of lasing modes and mode sweep plots to go along with them.

For very low gain wavelengths like green (543.5nm) and yellow (594.1nm) – which may have 1/10th the gain or less compared to the common red (632.8nm) wavelength, the lasing threshold will be far higher on the roughly Gaussian shaped gain curve, where it is narrower. So, while the FWHM of the neon gain curve may be slightly wider at these wavelengths, fewer modes will be oscillating because of the narrowing due to the higher lasing threshold. However, until the lasing threshold approaches the peak of the gain curve, the reduction in number of modes won’t be that dramatic. And every effort is made to eliminate losses inside the cavity for these low gain lasers, so in fact, the lasing threshold may not even get that high relative to the peak during the expected life of the laser.

For very high gain wavelengths, the reverse will happen. There’s really only one – the mid-IR transition at 3,391nm which behaves more like a solid state laser with a gain over 40 times that of 632.8nm. The lasing threshold will be much lower on the gain curve extending the useful region well out into the tails of the distribution. In this situation, many more modes could end up oscillating than would be accounted for by the much narrower FWHM of the neon gain curve of 315MHz – roughly 1/5th the width compared to 632.8nm. If calculations based solely on this small gain bandwidth were valid, a 75cm 3,391nm laser would have a similar number of longitudinal modes to a 14 cm 632.8nm He-Ne where there are only 1 or 2 active modes at any given time. Since 3,391nm lasers much shorter than 75 cm are commercially available and don’t have dramatic variations in output power with mode sweep, this must not be the case. For example, REO has one with a cavity length of less than 50cm and maximum power variation of 5 percent, which implies that there are several longitudinal modes always present.

Here are results so far:

  • 543.5 nm (green): TBD.
  • 594.1 nm (yellow): TBD.
  • 604.6 nm (orange): TBD.
  • 611.9 nm (orange): TBD.
  • 632.8 nm (red): See other info below and in the sections starting with Inexpensive Home-Built Frequency or Intensity Stabilized HeNe Laser.
  • 1,152 nm (near-IR): TBD. Other than my rebuilt SP-119 laser head, a sample of one of these may be difficult to find. The only thing that can be said about the IR SP-119 is that it is short enough that lasing ceases entirely for a portion of the mode sweep.
  • 1,523 nm (near-IR): Initial testing of a Melles Griot 05-LIR-150 with a cavity length of 34.2 cm and a strategically placed magnet seem to show that its behavior is similar to that of a 632.8 nm laser with a cavity length of 20 or 25 cm. But, the amplitude of the two polarizations are not equal implying that it is probably operating at least in part as a transverse Zeeman laser, which isn’t that surprising given the magnet. However, with 3 strategically placed magnets, the behavior reverts back to what would be expected of a 633 nm tube of 20 or 25 cm with two pure orthogonally polarized modes separated by the longitudinal mode spacing of the tube are present for most of mode sweep with just a hint of a third mode when one is near the center of the neon gain curve. So, it would look like:
    Longitudinal Modes of Random Polarized 1 mW IR (1,523 nm) He-Ne Laser
    Longitudinal Modes of Random Polarized 1 mW IR (1,523 nm) He-Ne Laser

    which is the same diagram as

    Longitudinal Modes of Typical Random Polarized 1 mW He-Ne Laser
    Longitudinal Modes of Typical Random Polarized 1 mW He-Ne Laser

    with different numbers.) With my $2 SFPI modified for 1,5XX nm operation (replaced PD with cut-open germanium transistor photodiode), I have confirmed that the modes of the 05-LIR-151 are also similar in number and appearance to those of a 20 to 25 cm 632.8 nm laser. There are 2 modes most of the time with 3 appearing briefly when a mode is close to the center of the gain curve.

  • 3,391 nm (mid-IR): TBD, maybe.

Intensity Stability of He-Ne Lasers

There are at least three kinds of intensity variations present with He-Ne (or other gas) lasers: long term as various longitudinal modes compete for attention, short term due power supply ripple or discharge instability, and beat frequencies between modes that are active.

Common internal mirror He-Ne laser tubes include a specification called “Mode Cycling Percent” or something similar. This relates to the amount of intensity variation resulting from changes in longitudinal modes due to thermal expansion. Typical values range from 20 percent for a small (e.g., 6 inch, 1mW) tube to 2 percent or less for a long (e.g., 15 inch, 10mW) tube. These take place over the course of a few seconds or minutes and are very obvious using any sort of laser power meter or optical sensor. Even the unaided eyeball may detect a 20 percent change. The more modes that can be active simulataneously, the closer those that are active can be to the same output power on the gain curve. Very short tubes or those with low gain (other wavelengths than 632.8nm or due to age/use or poor design) may vary widely in output intensity or even cycle on and off due to mode cycling. (Note that since the polarization for each mode may be different, reflecting the beam of one of these He-Ne lasers from a non-metallic reflective surface (which acts somewhat as a polarizaer) can result in a large variation in brightness as the dominant polarization changes orientation over time.) Trading off between tube size and mode cycling intensity variations is one reason that He-Ne tubes with otherwise similar power output and beam characteristics come in various lengths.

There are also stabilized He-Ne lasers which use optical feedback to maintain the output intensity with a less than 1 percent variation. (They usually also have a frequency stabilized mode but can’t do both at the same time.) An alternative to doing it in the laser is to have an external AO modulator or other type of variable attenuator in a feedback loop monitoring optical output power. See the next section for more info.

Short term changes in intensity may result from power supply ripple and would thus be at the frequency related to the power line or inverter. These can be minimized with careful power supply design.

Intensity variations at 100s of MHz or GHz rates result from beats between the various longitudinal modes that may be simultaneously active in the cavity. For most common applications, these can be ignored since they will be removed by typical sensor systems unless designed specifically to respond to these high beat frequencies.

Also see the section: Amplitude Noise.

Stabilized Single Frequency He-Ne Lasers

The common red (633 nm) He-Ne laser, while highly monochromatic, generally does not produce just a single frequency (or equivalently, wavelength) of light. As noted in the section: Longitudinal Modes of Operation, several closely spaced frequencies will generally be active at the same time and their precise values and intensities will change over time. For many applications, this doesn’t matter. However, for others, it makes such a laser useless.

If you have, say, $5,000 to spend, you can buy a red (633nm) He-Ne laser that actually produces a single frequency with specifications guaranteed stable for days and that don’t change over a wide temperature range. While the operation of such a He-Ne laser is basically the same as the one in a barcode scanner (and in fact may use the identical model He-Ne laser tube!), several additional enhancements are needed to eliminate mode sweep and select a single output frequency. Simply constructing the laser cavity of low thermal expansion materials isn’t enough when dealing with distances on the order of a fraction of a wavelength of light! Active feedback is needed. The most common implementation of these lasers starts with a short red (632.8 nm) tube that can only oscillate on at most 3 longitudinal modes. (For technical reasons, stabilized lasers at the other common visible and IR He-Ne wavelengths are more difficult to implement and are much less common. More on this below.) It then adds optical feedback to keep them in a fixed location on the He-Ne gain curve by precisely adjusting the distance between the mirrors over a range of about 1/2 the lasing wavelength. This is most often done with a heating coil (inside or outside the tube), but a PieZo Transducer (PZT, an expensive version of the beeper element in a digital watch) may also be used. The PZT reduces the time for the system to stabilize to a few seconds, compared to up to 30 minutes for the heater. But, for a laser that will be left on continuously, this probably doesn’t matter. Some lasers use a means of cooling in addition to the heater like a piezo fan, probably to allow the laser to run stably over a wider temperature range. And a few including the Melles Griot 05-STP-909/910/911/912 (originally based on the Aerotech Syncrolase 100) use a miniature RF induction heater surrounding the HR mirror mount to control only its length, not that of the entire tube. With direct heating of such a small mass, the response is quite fast. This also makes for a more compact package than a full tube heater.

Many schemes work well and it’s amazing how dirt simple these really are considering their hefty price tags! It’s easy to build perfectly usable systems from a common surplus HeNe laser tube and a few common junk parts.

The common ones are listed below:

Note that an etalon inside the laser cavity could also be used to select out a single longitudinal mode. For high power lasers which would require long tubes supporting many modes, this would be needed with both the overall mirror spacing and etalon being feedback controlled. But for low power lasers (e.g. 1 to 3 mW), the use of a short tube to limit the number of modes in conjunction with basic feedback control is a much less complex lower cost approach.

Stabilized lasers (or anything that needs to be regulated to some precision) can be classified as two types. The technique is “intrinsic” – basically derived from an internal reference – if what is used to regulate the device is a fundamental property of its construction – the laser physics in this case. It is “extrinsic” if some external reference is used. Most commercial stabilized HeNe lasers are of the first type since they exploit the known and essentially fixed frequency/wavelength and shape of the neon gain curve in the E/M spectrum. Additional techniques may be used to further reduce the uncertainty.

Most common commercial stabilized HeNe lasers are red at 633 nm, partially because of all the available HeNe wavelengths with a single frequency output power of less than 2 mW. Systems like this are both relatively easy to implement and generally useful for a wide range of applications. The approaches usually fall into one of two subclasses:

  1. One or Two Mode stabilized systems: These use random polarized HeNe laser tubes that are short enough that only a few modes will oscillate at the same time. Adjacent modes of a random polarized HeNe laser tube are almost always orthogonally polarized. So, where two modes are oscillating, separate signals corresponding to the amplitude of each mode can be easily obtained by feeding a pair of photodiodes from a polarizing beamsplitter. (If a tube has modes that aren’t orthogonally polarized or that behave strangely, it gets recycled into another application or the dumpster.) The signals may be obtained from the waste beam out of the HR mirror of the laser or by sampling a portion of the output beam. Either one or both of the photodiode signals can then be used for the feedback loop depending on whether intensity or frequency stability is most important. Note that under some conditions, up to 3 or even 4 modes may be permissible in a tube that is to be used for these purposes. More below.
    • Where the best frequency stability is desired, the ratio of the mode signals (usually made 1:1) is used in the feedback loop. This results in better absolute frequency stability since this ratio is independent of the actual output power, which may change as the tube warms up and ages due to use. With a ratio of 1:1, the two modes are parked equally spaced on either side of the gain curve. Even if the tube oscillates on 3 modes if one is near the center of the gain curve (1 strong one and 2 weak ones), there will only be 2 modes when stabilized. The overall approach is shown below:
      Dual-Mode Single-Frequency Stabilized He-Ne Laser
      Dual-Mode Single-Frequency Stabilized He-Ne Laser

      Commercial examples include the Coherent 200, Spectra-Physics 117/A/B/C (and identical Melles Griot 05-STP-901), REO SHL. Axsys/Teletrac 150, and many others.Some inexpensive (this is relative!) stabilized HeNe lasers only use a single mode for frequency locking. When on the slope, this will be reasonably stable after warmup once the output power has reached equilibrium.

    • When the best intensity stability with a polarized output is desired, the signal from a single mode (one photodiode channel) is compared to a reference voltage and this becomes the error signal in a feedback loop to put its mode near the center of the gain curve. Even if the tube oscillates on up to 4 modes if there are two on either side of the gain curve, with one near the center of the gain curve when stabilized, there will be at most 2 weaker modes on the tails of the gain curve. Since these will be orthogonally polarized to the dominant center mode, they can be blocked by the output polarizer. The overall approach is shown below:
      Dual-Mode Single-Frequency Stabilized He-Ne Laser
      Dual-Mode Single-Frequency Stabilized He-Ne Laser

      Commercial examples include the Spectra-Physics 117A (and identical Melles Griot 05-STP-901), and REO SHL.

    • When the best intensity stability of the total output (without regard to polarization) is desired, a non-polarizing beam sampler is used or the signals from the two photodiode channels are summed and compared to the reference. I am not aware of any commercial lasers using this approach.
  2. Zeeman split systems: A magnetic field is used to create a pair of lasing modes that differ from each other by a relatively small frequency. The stable optical frequency along with the Zeeman difference frequency are used for a variety of metrology applications. These may be classified as either axial or transverse based on the orientation of the magnetic field:
    • Axial: Like the single mode systems described above, the tube length is such that only a single longitudinal mode will oscillate. However, a powerful axial magnetic field splits this single mode into two sub-modes with counterrotating circular polarization states. When passed through a polarizer at the output, this results in a beat frequency in the 100s of kHz to several MHz range (depending on the magnetic field strength and other factors) which may be used to derive the stabilization feedback signal and is also key to the measurement technique for which these are designed. The overall approach is shown below:
      Dual-Mode Stabilized Axial Zeeman-Split Dual-Frequency He-Ne Laser.
      Dual-Mode Stabilized Axial Zeeman-Split Dual-Frequency He-Ne Laser.

      Commercial examples include the HP/Agilent 5501B, 5517, 5518A, and 5519A/B (though the heater is actually *inside* the tube for these); Excel 1001; Zygo 7705; and others.

    • Transverse: Like the two mode systems described above, the tube length is such that a pair of modes can oscillate when straddling the gain curve but only a single mode when at the peak. A moderate transverse magnetic field in conjunction with the natural birefringence of the mirror system results in a beam frequency in the 10s to 100s of kHz range. Since the beat frequency varies slightly with the mode position, it may be used in a PLL feedback loop for frequency stabilization. One example is the Laboratory for Science model 220.

Most commercial stabilized He-Ne lasers for general laboratory applications are of type (1) and operate with 2 orthogonal modes for frequency stabilization, though some use 1 mode for intensity stabilization (or can select between them with a switch). (Regardless, only a single longitudinal mode – thus a single optical frequency – may be allowed to exit the laser, the other being blocked with a polarizer.) These include the Coherent 200, Spectra-Physics 117 and 117A (and the identical Melles Griot 05-STP-901), many from Zygo, and various models from REO, Thorlabs, and others. For example, in the Melles Griot 05-STP-901 frequency and intensity stabilized He-Ne lasers (no longer in production), the laser cavity permits a pair of orthogonal polarized longitudinal modes to be active and can provide very precise control by straddling these on either side of the gain curve (frequency stabilized mode) or a single longitudinal mode that is also used for the output on one side of the gain curve (intensity stabilized mode). Those from other companies are generally similar.

All the interferometry lasers manufactured by Agilent (formerly Hewlett Packard), Excel, and one model from Zygo (the 7705) are of type (2). While lasers from Teletrac/Axsys, Optodyne, Renishaw, and others are type (1).

And there are hybrid approaches. For example, the Zygo 7701/2/12/14 lasers generate and lock a single frequency via dual mode stabilization, But it is split into two using an Acoutso-Optic Modulator (AOM) rather than the Zeeman effect.

For some photos of the (quite simple) Zeeman split stabilized He-Ne tube used in the Hewlett-Packard 5517 laser head, see the Laser Equipment Gallery (Version 1.86 or higher) under “Assorted Helium-Neon Lasers”. And for more information on these lasers, see the sections starting with: Hewlett-Packard/Agilent Stabilized HeNe Lasers.

It isn’t really possible to convert an inexpensive HeNe tube that operates on many longitudinal modes into a single frequency laser. Adding temperature control could reduce the tendency for mode hopping or polarization changes, and the addition of powerful magnets can force a polarized beam. But, selecting out a single longitudinal mode would be difficult without access to the inside of the tube. However, if the HeNe tube is short enough that the mode spacing exceeds about 1/2 the Doppler-broadened gain bandwidth for neon (about 1.5 GHz), it will oscillate on at most 2 longitudinal modes at any given time and these will each be linearly polarized and usually orthogonal to each-other. Then, stabilization is possible using very simple hardware. In fact, even if the mode spacing is a bit smaller – down to 500 or 600 MHz – then only 2 modes will be present most of the time but 3 may pop up if one is close to the center of the gain curve. This, too, is an acceptable situation since the tube can be stabilized with the modes straddling the gain curve and then only 2 modes will oscillate. For intensity stabilization, 4 modes may even be permitted. Note that while the modes of a random polarized and linearly polarized tube are similar (except for polarization), a random polarized tube is desirable to be able to use a tube that supports 2 modes with the benefits they provide, while being able to eliminate the second mode from the output.

It may be possible with a combination of what can be done externally, as well as control of discharge current, to force a situation where gain is adequate for only 1 or 2 modes even for a longer tube. Whether this could ever be a reliable long term approach for a HeNe tube that normally oscillates in many longitudinal modes is questionable. What I don’t think will have much success are optical approaches such as feeding light back in through the output mirror. Doing this would likely have the exact opposite of the desired effect but may work in special cases (it’s called injection locking and is used with great success for other applications).

Coherent, Melles Griot, Spectra-Physics, and others will sell you a small stand-alone stabilized HeNe laser for $5,000 or so and Agilant (HP) and others have interferometers and other similar equipment which includes this type of laser (and are even more expensive!). Other manufacturers includ Zygo, Teletrac, Nikon, Micro-g Solutions, SIOS, NEOARK, and REO. The lab lasers that I’ve seen all use short HeNe tubes with thermal feedback control of the resonator length and all operate at the red HeNe wavelength (632.8xxxxxx nm to 8 or more significant figures). The Spectra-Physics model 117A/118A laser actually uses a lowly SP088-2 tube similar to those in older grocery store barcode checkout scanners as its heart. A tube like this is visible below:

Spectra-Physics Model 117 OEM Stabilized He-Ne Laser Assembly
Spectra-Physics Model 117 OEM Stabilized He-Ne Laser Assembly

However, some do employ a custom tube with the heater inside to greatly speed up response and reduce heat dissipation to the outside. A stabilized HeNe laser for green or other color visible HeNe wavelength or one of the IR wavelengths is also possible using the same techniques.

As noted above, the actual stabilization mechanism for the general purpose stabilized lasers may be the ratio of amplitudes of two longitudinal modes (which is better for frequency stabilization) or the amplitude of one mode (which is better for intensity stabilization). These are usually stable to within a few parts in 109. However, the frequency drift when intensity stabilized is still not much – probably less than 1 part in 108. Output power variation may be 0.2 percent if intensity stabilized and 1 percent if frequency stabilized. Some allow either method to be selected via a switch, as well as providing for an external tuning input to vary the frequency over several hundred MHz. (However, due to the thermal control most often used, the response time is not exactly fast.)

The Zeeman split interferometer lasers may lock the difference frequency to a crystal clock, though most seem to use the basic polarized modes for stabilization, with the Zeeman beat used only as the reference for the interferometer. A few do lock the Zeeman frequency to a PLL. One of these was the Laboratory for Science Model 220. (Laboratory for Science is now out of business).

More sophisticated schemes with even better precision and lower long term drift may lock to the “Lamb Dip” at the center of the neon gain curve or to one of the hyperfine absorption lines of an iodine vapor other type of gas cell, achieving stabilities on the order of 1 part in 1010 or even better.

Due to the performance, simplicity, reliability, and relatively low cost of stabilized HeNe lasers, they are still often the preferred frequency reference for many applications. As noted, a typical system might go for $5,000. While this may seem high, it is small compared to many other technologies. The cost is not the result of expensive components or complex manufacturing, but more to the relatively limited number of units produced. If stabilized HeNe lasers were as popular as laser pointers, they would probably cost under $100

Digital Control of Stabilized He-Ne Lasers?

These types of lasers have been designed using simple analog techniques for over 35 years. So why change? A few op-amps, a monostable or two, and a handful of discrete parts is sufficient for any conceivable level of performance in a mode-stabilized HeNe laser. There are at most two signals that need to be monitored (the polarization modes) with the objective of maintaining them equal or in a fixed ratio. Yet, I’ve seen at least 3 examples of dual polarization mode stabilized He-Ne lasers that have gone from a simple analog approach to a much more complex digital approach, apparently with no obvious technical justification:

  • HP/Agilent 5517: Xylinx or similar FPGA.
  • Zygo 7702: Motorola 68HC11 microprocessor.
  • Teletrac/Axsys: Microchip PIC16C73A-20/SP PIC.

All are basic mode stabilized He-Ne lasers. The 5517 is a Zeeman-split laser but the stabilization is mode-based.

The redesign in each case must have cost a fortune. Since none of these lasers had many adjustments in their analog designs, ease of manufacturing is probably not the justification. And there is no need for preventive maintenance as components age – lasers like this will run for years on-end without any adjustments. Cost of components is also not a viable excuse as jelly bean op-amps and other common parts are adequate for any of these lasers. Nor do any require an external computer interface like more complex lasers.

However, one obvious benefit from the company’s point of view is serviceability, or lack thereof for anyone not supported by the manufacturer. The new designs are virtually impossible to troubleshoot and repair without detailed service information, and possibly support software. Unless the problem is obvious like a broken wire or blown fuse, attempting to find an electronic fault in these high density surface mount PCBs controlled by firmware programs is just about impossible. And Marketing can promote the “benefits” of digital technology, as bogus as that may be here. If anything, the additional electrical noise from digital signals is a detriment. Digital has to be better, right? 🙂

Iodine Stabilized He-Ne Lasers

Unlike the more common He-Ne stabilized lasers like those that lock to some intrinsic feature of the lasing process like the neon gain curve, an Iodine Stabilized HeNe Laser (ISHL) uses a external gas cell containing iodine vapor, so that a line in the iodine absorption spectrum is used as the reference wavelength. In principle, this provides an improvement in long term wavelength accuracy of 1 to 2 orders of magnitude – down to 0.1 parts per billion, corresponding to a few 10s of kHz – or better.

An ISHL operating on the common red (633 nm) wavelength consists of a He-Ne laser tube with one or two Brewster windows, a gas cell containing iodine at low pressure, and at least one external mirror on a PieZo Transducer (PZT) for fine cavity length control. The iodine cell needs to be installed inside the laser cavity to benefit from the high intra-cavity circulating power as the sensitivity in the vicinity of 633 nm is very low. However, when operating on the green (543.5 nm) wavelength, the cell can be external despite the lower power generally achievable with green, because the sensitivity is higher.

The basic principles of operation for an ISHL are rather straightforward: The iodine (or actually I2) has a very complex absorption spectra with hundreds of absorption lines. A very small portion of it is shown below:

Iodine Absorption Spectrum Near 532 nm
Iodine Absorption Spectrum Near 532 nm

By dithering the laser cavity length via a PZT, a lock-in amplifier (also known as a phase sensitive detector or synchronous demodulator) can maintain the wavelength at the very center of any selected absorption peak (or dip, depending on your point of view!). The challenging part is to be able to reliably select a specific absorption line to lock to. So, although locking to a given line is fairly simple, the overall electronics can get to be quite complex if automatic line selection is desired, though nowadays, an embedded microcomputer does the line selection.

Here are some photos of an iodine stabilized laser based on the classic NIST (National Institute of Standards and Technology, formerly the National Bureau of Standards) design originally described in the paper: Howard P. Layer, “A Portable Iodine Stabilized Helium-Neon Laser, “IEEE Trans. on Inst. and Meas, IM-29, pp358-361, 1980. The photos are actually of two different samples of the NIST design. The first one is of a complete laser head while the others are of a physically similar resonator only where it’s easier to see the individual components.

  • Iodine Stabilized He-Ne Laser Head
    Iodine Stabilized He-Ne Laser Head

    The overall appearance is unremarkable with a shutter at the front (the round black thing) and several cables coming out the back (hidden). Leveling “feet” would often be installed be installed in the cast tabs for precise alignment. It is not known if this was a commercial product or built by NIST or perhaps even Hewlett Packard based on the NIST design. But there was an Agilent inventory sticker on the cover, so perhaps this very laser was used to certify HP/Agilent metrology lasers like the 5517A! 🙂 In fact, the base of this laser bears a striking resemblence to the 5517A (though the dimensions don’t match). It’s a combination of a cast and machined assembly, clearly not made for a one time research project. It may in fact be a Frazier Model 100 FISL (or the NIST version they copied) as the head looks identical to the Frazier laser down to the pattern of holes in its cover. 🙂

  • Iodine Stabilized He-Ne Laser Head With Cover Removed
    Iodine Stabilized He-Ne Laser Head With Cover Removed

    The glow of the Melles Griot 05-LHB-290 two-Brewster HeNe laser tube can be seen within the resonator structure.

  • Iodine Stabilized He-Ne Laser Resonator - Overall View
    Iodine Stabilized He-Ne Laser Resonator – Overall View

    The resonator is a rather massive metal structure about 18 inches long.

  • Iodine Stabilized HeNe Laser Resonator - Visible Portion of Two-Brewster He-Ne Laser Tube
    Iodine Stabilized HeNe Laser Resonator – Visible Portion of Two-Brewster He-Ne Laser Tube

    Most of the Melles Griot 05-LHB-290 two-Brewster tube is hidden, but it is mounted via compression O-ring fittings with the high voltage supplied via the BNC connector. The gray blobby thing houses the ballast resistors.

  • Iodine Stabilized HeNe Laser Resonator - Visible Portion of Two-Brewster He-Ne Laser Tube
    Iodine Stabilized HeNe Laser Resonator – Visible Portion of Two-Brewster He-Ne Laser Tube

    The iodine cell is mounted via compression O-ring fittings between the two-Brewster HeNe laser tube and one of the mirrors. The gold connectors (1 of 2 are visible) are for temperature control of the iodine cell, and possibly a photodiode for monitoring the fluorescence.

  • Iodine Absorption Cell Showing Fluorescence From Green He-Ne Laser Beam
    Iodine Absorption Cell Showing Fluorescence From Green He-Ne Laser Beam

    This shows the same iodine cell having been removed from the ISHL resonator, being excited by a separate green HeNe laser. The yellow-green (with some red) fluorescence inside the iodine cell means some green light is being absorbed and would show up as a reduction in transmitted beam power. (Fluorescence from a 633 nm beam would be in the IR and boring.)

  • Iodine Stabilized He-Ne Laser Resonator - Photodiode and Beam Sampler
    Iodine Stabilized He-Ne Laser Resonator – Photodiode and Beam Sampler

    This has an angled plate to provide a small portion of the output beam to a silicon photodiode. Both mirrors are mounted on PZTs for cavity length control and dither (though it’s not clear why a single PZT wouldn’t suffice for both functions).

Although the laser head does not presently lase, I am hopeful that it will someday. The discharge color of the HeNe laser tube is normal and there is no visible brown crud in the bore indicating that it should be healthy. The iodine cell still has iodine in it based on its response to a green (532 nm) DPSS laser pointer beam. This thing has probably been sitting on a warehouse for years, if not decades (next to the lost Ark), so the non-lasing condition isn’t exactly a surprise. However, there seemed to be some type of contamination inside one of the B-windows. So, it may require a replacement 05-LHB-290. I do have one that lases, though it’s a bit weak. However, the NIST paper states that the reflectivity of the OC mirror is only 93 percent, presumably to force single longitudinal mode operation by reducing gain, but this also dramatically reduces output power. And the tube would need to be quite healthy to lase at all. Replacing that mirror with a 99 percent OC might be an option. Then mirror alignment or some other means could be used to force SLM. It would seem like a more logical solution to force SLM would be to add a PZT-controlled etalon that tracks cavity length tuning. Then, the output power would be close to the maximum available from the tube – 5 to 10 times higher than this design produces. But I’ve not seen that anywhere. The paper also states that the laser tube and cavity are 20 and 30 cm long, respectively. On my samples, they are at least 25 and 35 cm. And, their laser tube appears to not be a Melles Griot 05-LHB-290. So perhaps the original prototype was not identical to the versions later reproduced by Frazier (and others), though it’s quite clear that Frazier copied nearly every aspect of the laser design down to the controller-in-a-scope and its front panel layout and labeling. 😉

More on ISHLs:

And multi-wavelength iodine stabilized He-Ne laser have also been built. See: “A Tunable Iodine Stabilized He-Ne Laser at Wavelengths 543 nm, 605 nm, and 612 nm”, J. Hu, T. Ahola, K. Riski, and E. Ikonen, Digest of the 1998 Conference on Precision Electromagnetic Measurements, July 6-10, 1998, IEEE Cat. No. 98CH36254. This one used the tube from a PMS/REO LSTP-1010 5 color tunable HeNe laser with a pair of PieZo Transducers (PZTs) behind the rear mirror (tuning prism) and a lock-in amplifier for feedback control. For these wavelengths, the iodine cell can be outside the cavity, but notice that the red wavelength, 633 nm, is not included. Multi-Wavelength Iodine Stabilized HeNe Laser

The only modification to the laser itself was to add a pair of PZT cylinders between the back of the tuning prism and its mount so that the cavity length could be tuned electronically. The iodine cell and laser power detector are external to the cavity.

What I found curious with this (as well as the NIST laser) is that the laser cavity is way too long to restrict the laser to single longitudinal mode operation as would be required for the system to be useful. The authors of the paper don’t appear to address this, nor have I found it mentioned elsewhere.

So I performed a quick experiment using a REO tunable HeNe laser. As expected, with the power in each wavelength maximized, there are multiple longitudinal modes oscillating. And also as expected, there would be a range of the mode sweep cycle where the output would be pure SLM if either the Wavelength Selector or Transverse adjustment were set so as to reduce output power below a specific value, differing for each wavelength as follows:

These values are very approximate and don’t necessarily mean that the laser can be tuned over any significant range and remain SLM as is required to be useful to lock to an I2 line – that would require even lower power. The 543.5 nm SLM power may be somewhat higher than 240 µW but that’s as much as my laser wanted to put out at the time. It would appear that 594.1 nm would be a very usable wavelength at higher power, but apparently the authors did not find a suitable I2 absorption transition at that wavelength, or at 632.8 nm either. The latter is rather strange as we know that there are more than a half dozen suitable I2 lines within the normal 632.8 nm gain bandwidth to which the Frazier and NIST lasers can be locked.

The NIST (and presumably Frazier) ISHLs use an OC reflectance of only 93 percent to raise the lasing threshold and force SLM operation. (Common red HeNe lasers of this size typically have an OC reflectance of 99 percent.) This option is not available for the multi-wavelength ISHL since the authors used a stock PMS/REO tunable laser tube which has a relatively high reflectance (much greater than 99 percent) internal OC.

Assuming this analysis with respect to usable SLM power to be correct, it does explain why direct locked ISHLs typically have very low power. To achieve higher power, some companies offer what is known as an “offset-locked iodine stabilized HeNe laser”. With these, a normal SLM HeNe laser with a typical output power of 1 to 2 mW (at 632.8 nm) has its optical frequency phase locked to the lower power ISHL. Implementation is actually easier than it sounds but nonetheless is left as an exercise for the motivated student. 😉

Stabilized He-Ne Lasers at Other Wavelengths

All types of schemes for stabilizing red (633 nm) He-Ne lasers have been developed, but most of those that are commonly used in commercial stabilized He-Ne tubes are based on monitoring of one or both polarized modes in the output or waste beams and locking their position to the neon gain curve. For well behaved so-called “random polarized” 633 nm HeNe laser tubes, adjacent modes are generally orthogonally polarized. So, to assure a single mode (single frequency) output, the tube simply has to be short enough that at the lock position, either one mode or two polarized modes are present. In the latter case, a polarizer at the output can block the unwanted mode.

While it might be assumed that exactly the same approach could be taken for “other color” lasers, this turns out not usually be the case. The principle reason is that the nice behavior that has been counted on to keep the lasers well mannered may not be present. So while the tube will still have a pair of orthogonal axes of polarization, adjacent longitudinal modes will not necessarily be orthogonal and/or even have a consistent relative polarization – they may flip like a banshee.

So, where it is desired to implement a stabilized HeNe laser at other wavelengths (visible or IR), the polarization may be the primary issue, but there are a number of other complications including differences in the neon gain bandwidth and generally much lower power:

  1. Orthogonal polarization: For the 633 nm HeNe laser, the Physics has cooperated (or Murphy took a millisecond off) with adjacent modes being orthogonally polarized. Since this is not necessarily true at other wavelengths, the use of a short tube may be required so that only a single mode is permitted at the lock point. For example, to assure that only a single mode can oscillate at 543.5 nm would require a tube less than about 12.5 cm in length, which would have an extremely low output power if it could be made to work at all – probably well under 0.1 mW.
  2. Neon gain bandwidth: The width of the inhomogeneously-broadened neon gain curve depends on optical frequency and is roughly equal to [633 nm /(Lasing Wavelength) * 1.6 GHz + 100 MHz] where the addition uses the sum of the squares. For most purposes, Doppler broadening dominates and the added 100 MHz term can be ignored since its contribution will be small. Thus, the length of the tube must be selected based on wavelength to assure that only the desired number of longitudinal modes can oscillate. Of course, this may directly conflict with the need for output power! For example, at 633 nm, a tube with a cavity length of 225 mm (667 MHz mode spacing) will allow at most 3 longitudinal modes to oscillate. At 1,523 nm, the gain bandwidth will less than 1/2 of what it is at 633 nm and may be insufficient for even 2 modes to see enough gain, resulting in the output actually going off during part of mode sweep.However, FWHM or other definition of the gain bandwidth has to be adjusted depending on the actual gain and losses of the tube. For example, the mid-IR 3,391 nm line has a gain over 40 times that of the 633 nm red line, so the lasing threshold will be much lower effectively widening the gain curve. And the gain at 544 nm (green) is roughly 1/20th of that at 633 nm.
  3. Power output: The gain and/or efficiency for most of the non-red wavelengths is much lower than for 633 nm. Normally, this can be handled using a longer tube. But that directly conflicts with (1) for the green (543,5 nm), yellow (594.1 nm), and orange (604.6 or 611.9 nm) wavelengths since these tubes need to be shorter than even for red.

Various tricks may be used to stabilize HeNe lasers at other wavelengths but in general, it’s often not as easy! Also see the section: A Stabilized HeNe Laser at 1,523 nm.

Back-Reflections and HeNe Lasers

Back-reflections of a laser’s output directly back to it is inherently destabilizing for most lasers, and in some cases even potentially destructive. Many factors determine what effects back-reflections will have including the type of laser, and optics between the laser cavity (inside the laser or external) and the source of the reflections.

HeNe lasers are particularly sensitive to back-reflections, though no damage is ever likely to occur. However, the instantaneous polarization state and amplitude of the longitudinal modes will be affected. These effects may not be noticeable for common HeNe lasers without using fancy instruments since they occur at nanosecond time scales. For these lasers, average output power from the laser will not be affected but for random-polarized HeNe lasers, the intensity of any portion of the beam passed through optics that affect polarization may fluctuate dramatically.

Suffice it so say that one should avoid back-reflections to HeNe lasers, but especially for stabilized HeNes. Even the reflection from a piece of fresh transparent tape in the beam may cause the laser to lose lock. What happens is that when a mode swaps polarization, the controller will attempt to relock but that may require several seconds or longer. Some lasers may indicate their unhappiness by flashing the READY or LOCK indicators, or in the case of the Spectra-Physics 117A and Melles Griot 05-STP-901, making clicking noises. 🙂

The best way avoid such instabilities is to arrange the setup so that there are no back-reflections. 😉 The HP/Agilent interferometer configurations used for metrology applications shown in Most Common Hewlett Packard/Agilent Interferometers are nearly perfect. With their high quality Polarizing Beam-Splitters (PBSs), there are virtually no back-reflections directly to the laser. The next best solution where this is unavoidable is to add an optical isolator at the output of the laser. A Faraday isolator is best but very expensive. For a beam with a single linear polarization, adding a PBS cube and Quarter Wave Plate (QWP) will redirect any reflections downstream that have not had a polarization change off to the side. In many applications, this is sufficient. But in some cases, two Faraday isolators in series are needed to fully tame the HeNe beast. 😉

Reverse Incremental Efficiency of HeNe laser?

You say: “Huh, what?”. 😉 Until recently, it never occurred to me to even think about how the HeNe lasing process and electrical input might be related other than that the HeNe laser is extremely inefficient. Then someone asked the obvious question: “Does the power input to the laser depend on the output power in the beam?”. With a bit of thought, it should be obvious for there to be some relationship. But even for other types of lasers, this is not something that is often considered. The slope efficiency is an important measurement for any laser, being how the laser output changes as a function of the electrical (or other) input. For example, with a laser diode, all that is needed is to measure the input electrical power and output optical power at two points where lasing is occurring and calculate the ratio of the differences. But this is from input to output. For a HeNe laser, such measurements can be done over a portion of the range where the power supply is stable resulting in a typical value of 0.3 mW/W or 0.3 percent, similar to the pathetic absolute efficiency for the HeNe laser!

But what we want here is the opposite – how the input power is affected by the laser output, which I’ll call the “Reverse Incremental Efficiency” or RIE. In other words, compare the input power with the laser operating normally and with the output suppressed, for example, by misaligning a mirror. For a HeNe laser, would there be a detectable change in input power if this were done? With a normal constant current HeNe laser power supply, the result should be a change in tube voltage. If for want of a better term, the “reverse slope efficiency” were 100 percent, then “spoiling” the beam of a 1 mW laser should result in a reduction of 1 mW in power consumed by the tube.

So I did an experiment using a high-mileage JDS Uniphase 1145P laser head with a Melles Griot 05-LPL-915 power supply set at 6.5 mA. The lasing was spoiled using a tube-type Nylon mirror adjuster pushing on the OC mirror mount to kill lasing in a totally reversible manner. Measurements were made while the laser was warming up and outputting 12 mW and then once fully warmed up and outputting 19 mW. The results were rather intriguing:

ΔPo is the output power, ΔVt is the change in tube voltage from 0 mW to ΔPo, and ΔPt is the corresponding change in the tube’s power consumption.

At first, my measurements were made with a DMM with only 4 digits of resolution and it appeared as though the the RIE might be exactly 50 percent, which could have had some cosmic significance. 🙂 But it wasn’t to be. With the full 5 digits of a Fluke 87, while the RIE isn’t far from 50 percent, it isn’t 50.00000000%. Too bad. But what this does say is that the incremental efficiency of getting coherent photons out the front of a HeNe laser once it’s running at the normal voltage and current and outputting near rated power is order of 50 percent, not a miniscule value like that 0.3 percent! Note that the results depend on whether the laser is running at reduced and full power. If this had been some obscure effect of mechanical stress on the discharge voltage, then the change in tube voltage would be about the same at both output powers. And pushing on the mirror mount beyond where lasing ceases has no effect on tube voltage. At least until it breaks off. 🙂

To further confirm that this is a true lasing effect, I repeated the experiment with a Melles Griot 05-LHB-570 one-Brewster laser where lasing could be suppressed simply by poking something in the cavity between the tube and OC mirror:

Even at this much lower output power, the RIE is still fairly high, though uncertainly is greater due to the much lower power and corresponding change in tube voltage.

Then, I did multiple sample points while a like-new 1145P head was warming up:

Just when I thought this was making some sense, these data appear to show an unexpected very non-linear relationship. Most of the voltage change occurs between 0 mW a few mW, and it is then nearly constant, perhaps due to the gain saturating. There is still significant uncertainty as the measured values for both absolute tube voltage and the voltage difference fluctuate over time.

And finally on the same head when fully warmed up with a stable 24 mW of output power undisturbed, with controlled misalignment of the OC mirror to generate a few intermediate values:

These are generally similar to the measurements during warmup. The last two full power entries reflect the variation that may be present even when the laser is in thermal equilibrium. Even so, there can be small changes in the longitudinal mode positions and thus relative efficiencies of the lasing lines or something. 🙂

A reference to this phenomenon can be found on page 38 of an old NASA report: An Experimental and Theoretical Investigation of Striations in a HeNe Laser. (If this link should decay, simply search for the title.) I’m sure there are many more in depth studies but locating them is left as an exercise for the student. 🙂

On-line Introductions to HeNe Lasers

There are a number of Web sites with laser information and tutorials.

  • One of the best so far is the CORD Laser/Electro-Optics Technology Series, Cord Communications, 324 Kelly Drive, P.O. Box 21206, Waco, Texas 76702-1206.In particular:
    • Module 1-10 Helium-Neon Gas Laser–A Case Study goes into considerable detail on the theory as well as some more practical information related to HeNe lasers.
    • Module 3-1 Power Sources for CW Lasers deals with HeNe laser power supplies.
    • Module 4-2 Gas Laser Power Supplies has more on HeNe laser power supplies (some redundancy with Module 3-1).

    See the section: On-Line Introduction to Lasers for the current status and on-line links to these courses, and additional CORD LEOT modules and other courses relevant to the theory, construction, and power supplies for these and other types of lasers.

  • The HeNe Laser Manual by Elden Peterson of Voltex, Inc. has a variety of practical information on HeNe lasers including characteristics and power supply considerations. This is a nice concise treatment of the practical aspects of HeNe lasers and power supplies and recommended for those who would like the “short course” before (or in place of) diving in head-first to the material that follows. 🙂 There is also: “HeNe Lasers: Their Quirks and Quarks” by Keith Schmidt, referenced in this manual, which I haven’t seen but sounds interesting.
  • MEOS GmbH was a developer of laser educational materials and equipment (among other things) but now appears to be gone for good. They had the lab/study manuals for their courses on a wide variety of laser related topics. While designed to be used in conjunction with the laboratory apparatus which they sell, these manuals include a great deal of useful information and procedures that can be applied in general.As of Summer 2012, MEOS has stopped development and support of these kits. (In fact, the company doesn’t seem to exist anymore, at least not doing anything remotely related to photonics.) However the creator of the experiments and author of the manuals has been acquired by LD Didactic (Leybold) and is continuing this line, which is represented by Klinger in US. The updated manuals are now available for free download at the Leybold Ld Didactic Web Site.Several modules would be of particular interest for HeNe lasers. Unfortunately, the on-line manuals (in PDF format) have disappeared from the MEOS Web site. But I have found and archived most of MEOS manuals. (The ones above may be slightly different.)
  • The Helium-Neon Laser (Department of Physics, Middlebury College) is the lab procedure for setting up a external mirror HeNe laser but also includes some basic information.
  • 1979-1980 Metrologic Catalog and Laser Handbook had general information on how a HeNe laser works and details of HeNe laser tube fabrication on pages 34 to 39. The manufacturing process is for Metrologic’s “hard-seal metal ceramic” HeNe laser tubes which never caught on and were discontinued after a few years, but is interesting nontheless.
  • Also see the section: General Laser Information and Tutorial Sites for other sites that may be worth visiting.
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6-Point Ignition Transformer

Ignition Transformer
Ignition Transformer

Here’s a quick teardown of an ignition transformer, used on gas fired ovens & hobs.  This unit takes mains 240v AC & uses a transformer to step the voltage to several kV, at a low current to ignite the burners.

Bottom
Bottom

The transformer section is completely potted in Epoxy resin for insulation, but the driver circuitry is exposed, with a pair of leads from the primary winding exposed

Driver PCB
Driver PCB

The drive is very simple. The incoming AC flows through a series resistor through a half-wave rectifier to charge up a 2.2µF film capacitor. Once the voltage on the capacitor reaches a certain level, a DIAC in series with the transformer primary fires, discharging the capacitor through the primary.
The current spike induces a very high voltage on the secondary winding, this then arcs across a gap in the gas flow to start ignition.

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Boating: Drydock Time – The Inspection

Drydock
Drydock

It’s that time again, so the boat is out of the water for it’s 3-yearly maintenance. Some things over the past few months have been bugging me, namely a pronounced vibration in the running gear while underway. (Issue was easy to spot here!).

10-Ton Jack
10-Ton Jack

nb Tanya Louise being a very odd vessel, she has quite a significant keel, so once the dock was drained, some manual jacking was required to get her level on the blocks. Without this extra work there is such a pronounced heel that it’s impossible to do anything on board.

Chocks
Chocks

On the opposite side, wooded blocks are placed for the bottom of the hull to rest against. Jacking up a 58-ft 25-ton boat by hand onto some timbers was nerve-wracking to say the very least!

The bottom of the hull has already been jet-washed to remove 3-year’s worth of slime, weed growth & the old blacking. First job is to get a fresh coat of paint on.

Running Gear
Running Gear

Looking under the hull shows the reason for the high level of vibration – the prop shaft has actually *worn through* the bearing & stern tube, to the extent that there’s not much left of the assembly! The only thing holding the shaft in place at this stage is the stuffing box inside the boat & the shaft coupling to the hydraulic motor.
, stern tube,
A replacement standard-issue Cutless bearing will be fitted, after the remains of the old tube are cut back to make room. To facilitate mounting the bearing, a custom stainless P bracket is being made at a local engineers, for me to weld onto the bottom of the hull.

(Surprised we didn’t lose the shaft, lucky that I kept pestering to get her out of the water!).

More to come as work progresses!

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Digital Angle Gauge

Front
Front

Here’s a useful tool for the kit, a digital angle gauge/protractor. These use a silicon sensor to show the number of degrees the unit is out of level.

Magnets!
Magnets!

Magnets are provided in the base, so the tool can attach to any ferrous surface.

Battery Box
Battery Box

Power is provided by a single AAA cell.

Main PCB
Main PCB

Removing the rear cover reveals the brains of the unit, and there’s not much to it at all. The main microcontroller is a CoB-type device, so no part numbers available from that one.

Sensing Element
Sensing Element

The IC to the left of the main microcontroller is the sensing element. There’s no markings on this inclinometer IC so I’m not sure of the specs, but it will be a 3D-MEMS device of some sort.

Power Supply
Power Supply

The other side of the PCB has the power supply for the logic, and a serial EEPROM, probably storing calibration data.

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HP SureStore DAT40 Tape Drive

DDS4 Tape Drive
DDS4 Tape Drive

Magnetic tape is the medium of choice for my offline backups & archives, as it’s got an amazing level of durability when in storage. (LTO Has a 30 year archival rating).
For the smaller stuff, like backing up the web server this very site runs on, another format seemed to suit better. Above is a HP DDS4 tape drive, which will store up to 40GB on a cassette compressed.
I picked this format since I already had some tapes, so it made sense.

Data Plate
Data Plate

Here’s the info for those who want to know. It’s an older generation drive, mainly since the current generation of tape backup drives are hideously expensive, while the older ones are cheap & plentiful. Unfortunately the older generation of drives are all parallel SCSI, which can be a expensive & awkward to set up. Luckily I already have other parallel SCSI devices, so the support infrastructure for this drive was already in place.

Option Switches
Option Switches

On the bottom of the drive is a bank of DIP switches, according to the manual these are for setting the drive for various flavours of UNIX operating systems. However it doesn’t go into what they actually change.

Controller PCB
Controller PCB

The bottom of the drive has the control PCB. The large IC on the left is the SCSI interface, I’ve seen this exact same chip on other SCSI tape drives. Centre is a SoC, like so many of these, not much information available.

Drive Frame
Drive Frame

Removing the board doesn’t reveal much else, just the bottom of the frame with the tape spool motors on the right, capstan motor bottom centre. The bottom of the head drum motor is just peeping through the plastic top centre.

Head Drum
Head Drum

Here’s the head drum itself. These drives use a helical-scan flying head system, like old VHS tape decks. The top of the capstan motor is on the bottom right.

Cleaning Brush
Cleaning Brush

Hidden just under the tape transport frame is the head cleaning brush. I’m not sure exactly what this is made of, but it seems to be plastic.

Loading Motor
Loading Motor

A single small DC motor with a worm drive handles all tape loading tasks. The PCB to the bottom left of the motor holds several break-beam sensors that tell the drive what position the transport is in.

Tape Transport Mech
Tape Transport Mech

Here’s the overall tape transport. The PCB on top of the head drum is a novel idea: it’s sole purpose in life is to act as a substrate for solder blobs, used for balancing. As this drum spins at 11,400RPM when a DDS4 tape is in the drive, any slight imbalance would cause destructive vibration.

Tape Transport
Tape Transport

Here’s the drive active & writing a tape. (A daily backup of this web server actually). The green head cleaning brush can be better seen here. The drive constantly reads back what it writes to the tape, and if it detects an error, applies this brush momentarily to the drum to clean any shed oxide off the heads. The tape itself is threaded over all the guides, around the drum, then through the capstan & pinch roller.

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IC Decapping: The Process

As I’ve been posting some photos of decapped ICs lately, I thought I’d share the process I use personally for those that might want to give it a go 😉

The usual method for removing the epoxy package from the silicon is to use hot, concentrated Nitric Acid. Besides the obvious risks of having hot acids around, the decomposition products of the acid, namely NO² (Nitrogen Dioxide) & NO (Nitrogen Oxide), are toxic and corrosive. So until I can get the required fume hood together to make sure I’m not going to corrode the place away, I’ll leave this process to proper labs ;).

The method I use is heat based, using a Propane torch to destroy the epoxy package, without damaging the Silicon die too much.

TMS57002 Audio DSP
TMS57002 Audio DSP

I start off, obviously, with a desoldered IC, the one above an old audio DSP from TI. I usually desolder en-masse for this with a heat gun, stripping the entire board in one go.

FLAMES!
FLAMES!

Next is to apply the torch to the IC. A bit of practice is required here to get the heat level & time exactly right, overheating will cause the die to oxidize & blacken or residual epoxy to stick to the surface.
I usually apply the torch until the package just about stops emitting it’s own yellow flames, meaning the epoxy is almost completely burned away. I also keep the torch flame away from the centre of the IC, where the die is located.
Breathing the fumes from this process isn’t recommended, no doubt besides the obvious soot, the burning plastic will be emitting many compounds not brilliant for Human health!
Once the IC is roasted to taste, it’s quenched in cold water for a few seconds. Sometimes this causes such a high thermal shock that the leadframe cracks off the epoxy around the die perfectly.

All Your Die Belong To Us
All Your Die Belong To Us

Now that the epoxy has been destroyed, it breaks apart easily, and is picked away until I uncover the die itself. (It’s the silver bit in the middle of the left half). The heat from the torch usually destroys the Silver epoxy holding the die to the leadframe, and can be removed easily from the remaining package.

Decapped
Decapped

BGA packages are usually the easiest to decap, flip-chip packages are a total pain due to the solder balls being on the front side of the die, I haven’t managed to get a good result here yet, I’ll probably need to chemically remove the first layer of the die to get at the interesting bits 😉

Slide
Slide

Once the die has been rinsed in clean water & inspected, it’s mounted on a glass microscope slide with a small spot of Cyanoacrylate glue to make handling easier.

Some dies require some cleaning after decapping, for this I use 99% Isopropanol & 99% Acetone, on the end of a cotton bud. Any residual epoxy flakes or oxide stuck to the die can be relatively easily removed with a fingernail – turns out fingernails are hard enough to remove the contamination, but not hard enough to damage the die features.

Once cleaning is complete, the slide is marked with the die identification, and the photographing can begin.

Microscope Mods

I had bought a cheap eBay USB microscope to get started, as I can’t currently afford a proper metallurgical microscope, but I found the resolution of 640×480 very poor. Some modification was required!

Modified Microscope
Modified Microscope

I’ve removed the original sensor board from the back of the optics assembly & attached a Raspberry Pi camera board. The ring that held the original sensor board has been cut down to a minimum, as the Pi camera PCB is slightly too big to fit inside.
The stock ring of LEDs is run direct from the 3.3v power rail on the camera, through a 4.7Ω resistor, for ~80mA. I also added a 1000µF capacitor across the 3.3v supply to compensate a bit for the long cable – when a frame is captured the power draw of the camera increases & causes a bit of voltage drop.

The stock lens was removed from the Pi camera module by careful use of a razor blade – being too rough here *WILL* damage the sensor die or the gold bond wires, which are very close to the edge of the lens housing, so be gentle!

Mounting Base
Mounting Base

The existing mount for the microscope is pretty poor, so I’ve used a couple of surplus ceramic ring magnets as a better base, this also gives me the option of raising or lowering the base by adding or removing magnets.
To get more length between the Pi & the camera, I bought a 1-meter cable extension kit from Pi-Cables over at eBay, cables this long *definitely* require shielding in my space, which is a pretty aggressive RF environment, or interference appears on the display. Not surprising considering the high data rates the cable carries.
The FFC interface is hot-glued to the back of the microscope mount for stability, for handheld use the FFC is pretty flexible & doesn’t apply any force to the scope.

Die Photography

Since I modified the scope with a Raspberry Pi camera module, everything is done through the Pi itself, and the raspistill command.

Pi LCD
Pi LCD

The command I’m currently using to capture the images is:
raspistill -ex auto -awb auto -mm matrix -br 62 -q 100 -vf -hf -f -t 0 -k -v -o CHIPNAME_%03d.jpg

This command waits between each frame for the ENTER key to be pressed, allowing me to position the scope between shots. Pi control & file transfer is done via SSH, while I use the 7″ touch LCD as a viewfinder.

The direct overhead illumination provided by the stock ring of LEDs isn’t ideal for some die shots, so I’m planning on fitting some off-centre LEDs to improve the resulting images.

Image Processing

Obviously I can’t get an ultra-high resolution image with a single shot, due to the focal length, so I have to take many shots (30-180 per die), and stitch them together into a single image.
For this I use Hugin, an open-source panorama photo stitching package.

Hugin
Hugin

Here’s Hugin with the photos loaded in from the Raspberry Pi. To start with I use Hugin’s built in CPFind to process the images for control points. The trick with getting good control points is making sure the images have a high level of overlap, between 50-80%, this way the software doesn’t get confused & stick the images together incorrectly.

Optimiser
Optimiser

After the control points are generated, which for a large number of high resolution images can take some time, I run the optimiser with only Yaw & Pitch selected for all images.

Optimising
Optimising

If all goes well, the resulting optimisation will get the distance between control points to less than 0.3 pixels.

Panorama Preview
Panorama Preview

After the control points & optimisation is done, the resulting image can be previewed before generation.

Texas Instruments TMS67002
Texas Instruments TMS67002

After all the image processing, the resulting die image should look something like the above, with no noticeable gaps.

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Rigol DS1054Z DC Power Supply – Linear Post Regulation

Finally, here’s the last part of the Rigol 12v DC Power Supply project, the linear post regulation section to remove some of the ripple.

I have made a couple of layout adjustments since the last post about this part of the project – a little more filtering on the DC outputs. As usual the Eagle project files are at the bottom of the post for those who might find them useful.

Updated PCB
Updated PCB
Updated Schematic
Updated Schematic

 

Completed PCB
Completed PCB

Here’s the completed PCB, partially installed in the back of the scope. The missing regulator is the 5v one, since I already have a source of clean 5v from my original attempt at the supply, it’s not a problem not using a linear after the switcher. The filtering is the same on all channels, input from the switchers is on the right, outputs to the scope on the left.

PCB Bottom
PCB Bottom

Here’s the bottom of the PCB, with the common mode input chokes. The design of this board has allowed me to remove a couple of the switching modules as well, as I can use a single bipolar supply to run both sets of bipolar regulators on this board. This should help remove some of the noise also.

The ripple level has now dropped to lower than it was originally on the mains supply! Current draw at 13.8v DC is about 1.75A.

Scope Ripple
Scope Ripple

[download id=”5589″]

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GY561 Power Calibration

Unfortunately the manual for the eBay GY561 Frequency & RF Power Meter is very badly translated, but I think I have figured out the calibration procedure, so here it goes 🙂

Initial Screen
Initial Screen

On removing the front cover, which is just clipped on, there are 4 buttons. The only button that is usually available is the one on the far right, the power button.

I will term these buttons A, B, C, D, starting from the left side.

To get into the initial calibration screen, in the above image, hold button A while the power button (D) is pressed. Release the power button (D), then release button A.
The meter will show the screen above, where the frequency to calibrate can be chosen. This goes in 5MHz steps, 0-500MHz, using the B button to go down in frequency, and the C button to go up.

Once you’ve selected the frequency you wish to calibrate against, press button A, and the following screen will appear:

Frequency Calibration Screen
Frequency Calibration Screen

On this screen, the actual calibration can be done.
The number in the bottom left signifies the power level setting, from 1-5. The centre number is the calibration setting in Watts. The D in the bottom corner signifies that the setting is at the factory default.
Button C will cycle through the power level settings, for 2W, 5W, 10W 20W, 40W. This allows calibration at different power levels per frequency.
Once you have the frequency to calibrate, and you’ve selected the power level to calibrate at, connect a known RF power source to the input of the unit.
At this point, key the transmitter, and press button A. The display will change to the following:

Calibration Stage 2
Calibration Stage 2

When on this screen, you can set the power level of your RF source. Use the A key for +0.1W, the B key for +1W, and the C key for +10W.
Once you’ve keyed in the power of your source, press button D to save the setting. The “S” in the bottom corner will change to a “C”, to indicate a user calibration has been entered:

Calibration Complete
Calibration Complete

If you make a mistake with entering the power level, press the “C” key to cycle up to 60W, once at this level, another press of the button will reset the reading to zero. You can then enter the power level again.

If you wish to revert a user-entered setting to the factory default, press button B on the page above. The “D” will reappear in the bottom corner to indicate the setting has been restored.

At this point you can either press button C to calibrate at another power level for this frequency, or press button D to go back to the frequency selection.
Press button D again when at the frequency selection page to turn the unit off. The unit will then power up normally next time the power button (D) is pressed.

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Solderless N-Type Connector Fitting

I thought I’d detail the process I use to fit an N-Type connector to a coax cable, as I don’t usually solder these connectors.

Backnut & Seal
Backnut & Seal

Before stripping, fit the backnut, washer & rubber seal onto the cable.

Stripped Coax
Stripped Coax

The cable is first stripped back to reveal the shield. This cable has a foil tape as well as the usual copper braid.

Shield Connection
Shield Connection

Once the inner core has been revealed, the shield washer is fitted. This has a knife edge on the inner diameter, to fit between the outer sheath & the shield, this makes the electrical connection.

Inner Insulation
Inner Insulation

With the shield washer fitted, the inner insulation can be cut back, it should be just about level with the final washer when you’re done, this allows the connector to fit together properly.

Center Core Trimmed
Center Core Trimmed

Trim the center conductor to about double the length required, to allow it to be folded over, as shown. This allows the copper to spring back against the center pin of the connector when it’s fitted, to allow a good connection.

Final Washer
Final Washer

Here the final washer is fitted over the shield washer. The center insulation should be at the same level to allow the center pin to fit properly.

Center Terminal
Center Terminal

Finally, the center pin is pushed over the inner conductor of the cable, with it’s insulating spacer. Soldering these usually results in the plastic melting and a ruined connector.

Finished Plug
Finished Plug

Finished plug. Make sure the backnut is tightened fully home, without twisting the connector body itself. After I’m done with the termination, I use self-amalgamating tape to form a strain relief on the cable. This prevents it from breaking at the point where it enters the backnut.

I’ve been terminating these connectors this way for a long time & have not had any issues with SWR or bad connections, dispite the fact that I don’t solder them. This also has the advantage that fewer tools are required for the job & the connectors can easily be reused should the cable wear out.

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Roving Networks RN-52 Bluetooth Audio

I’ve been doing some tinkering with the RN-52 Bluetooth Audio module from Roving Networks, in prep for building a portable wireless speaker system, & thought I’d share my designs.

Initially I was having some issues with RF noise on the audio output from the RN-52, as I was only using the outputs single-ended. The module didn’t like this treatment, with all the RF whine coming straight out of the speakers.

To fix this issue I have used a pair of jellybean LM386 audio power amplifiers, running in differential input mode. This solves the high-pitched whine when the audio is enabled, & also allows the module to directly drive a set of 32Ω headphones at a reasonable level.

In Eagle I have designed a simple board, routing only the audio output, serial TTL & command mode pins out, along with the supporting power supply circuitry to operate from 12v DC.

RN-52 Breadboard
RN-52 Breadboard

Above is the current incarnation of the circuit on the breadboard. The RN-52 is on the left, audio power stage in the centre & headphone output on the right.

RN-52 Breakout
RN-52 Breakout

The bluetooth module on a breakout board. I was cheap in this case & etched my own board. I’m not paying Sparkfun, (as much as I like them), an extra ~£10 for a small PCB with the pins broken out. Much cheaper to spend 15 minutes with the laser printer & the iron, & do a toner transfer PCB.
As this board is single sided, I added a ground plane on the underside with copper foil, to help with the RF issues. Breadboards really aren’t all that good at rejecting noise induced when there’s a 2.4GHz transceiver mounted on them.

LM386 Amplifier
LM386 Amplifier

The LM386 audio power stage. The differential inputs from the module are capacitively coupled with 1µF electrolytics. This setup remarkably reduced the noise on the output. I left these at their default gain of 20, as I’ll be connecting another high power amplifier stage to drive large speakers.

RN-52 Eagle Layout
RN-52 Eagle Layout

Here’s the circuit laid out in Eagle, ready for PCB.

RN-52 Eagle PCB
RN-52 Eagle PCB

And here’s the PCB layout. Only one link required for the +5v line from the TTL serial port.

As always, the Eagle PCB & Schematic layout files are available at the bottom of the article.

*Update 29-01-15*
Rerouted a few things:

  • Moved the audio power stage to the +12v rail to improve sound response. – As the LM386 has a max input voltage of 12v (absolute maximum 15v), a regulated supply is recommended. The LM386-N4 variant has a higher voltage range, up to 18v. This should be suitable for an unregulated supply.
  • Removed 1µF coupling capacitors to reduce distortion & amplifier hiss. The capacitors appeared to cause some instability on the amplifier, causing random distortion. Removing them has cured this. No signal hiss has also been reduced to a very low level.
  • Reversed input polarity on input of one of the amplifiers – this appears to produce better audio.
  • Added PWR.EN header to allow connection of power button. Saves hassle of cycling power to the board when the RN-52 goes into sleep mode.

Improved PCB & Schematic layouts.

RN-52-SCH-v3.6
RN-52-SCH-v3.6
RN-52-PCB-v3.6
RN-52-PCB-v3.6

[download id=”5579″]

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AD9850 DDS VFO PCB & Schematic Layout

I recently came across a design for an Arduino controlled AD9850 DDS module, created by AD7C, so I figured I would release my Eagle CAD design for the PCB here.

It is a mainly single-sided layout, only a few links on the top side are needed so this is easy to etch with the toner transfer method.

My version uses an Arduino Pro Mini, as the modular format is much easier to work with than a bare ATMega 328.

RF output is via a SMA connector & has a built in amplifier to compensate for the low level generated by the DDS Module.

DDS VFO
DDS VFO

Version 2 Update: Added reverse polarity protection, added power indicator LED, beefed up tracks around the DC Jack.
[download id=”5571″]

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LM386 Stereo Audio Amplifier

The quickest project from inception to working PCB yet:

From inception to a working PCB took only 4 hours!

LM386 Amplifier
LM386 Amplifier

This is a miniature stereo audio amplifier, 0.5W per channel, that can be run from any voltage between 4-12v DC.

As usual, all the Eagle project files are available for download below & kits/bare PCBs will be available for sale for those that cannot etch boards.

In Operation
In Operation

Here is the circuit driving a pair of 3W 8Ω speakers from a line level audio source. The gain of this circuit is set at 50 with the components specified.

 

Schematic
Schematic

As can be seen from the schematic, this is a pair of single LM386 ICs for each channel.

Gain can be set by altering R3 & R4

[download id=”5566″]

Buy Kits Here £9.50:
[wp_cart_button name=”LM386 Stereo Audio Amplifier Kit” price=”9.50″]

Buy bare PCBs here £5:
[wp_cart_button name=”LM386 Stereo Audio Amplifier PCB” price=”5″]

PCBs are etched on FR4 laminate with 8oz copper with top component silkscreen.

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DIY Valve Amplifier – Part 1 – Amplifier Section

Components
Components

Here are a few details of a valve amplifier I am building, using the valve related parts from a 1960’s reel to reel tape recorder.

This amplifier is based on an a Mullard ECL82 triode/pentode valve, with an EM84 magic eye tube for level indication.

Beginnings Of The Amplifier
Beginnings Of The Amplifier

Here the first components are being soldered to the tags on the valve holder, there are so few components that a PCB is not required, everything can be rats-nested onto the valve holders.

Progress
Progress

Progressing with the amplifier section componentry, all resistors are either 1/2W or 2W.

Valve Sockets Fitted
Valve Sockets Fitted

Here the valve holders have been fitted, along with the output transformer, DC smoothing capacitor & the filament wiring, into the top of the plastic housing. At this point all the components that complete the amplifier section are soldered to the bottom of the right hand valve holder.

Wiring
Wiring

Starting the wiring between the valves & the power supply components. The volume control pot is fitted between the valve holders.

Valves Test Fit
Valves Test Fit

The valves here are test fitted into their sockets, the aluminium can at the back is a triple 32uF 250v electrolytic capacitor for smoothing the B+ rail.

Amplifier Section First Test
Amplifier Section First Test

First test of the amplifier, with the speaker from the 1960’s tape recorder from which the valves came from. the 200v DC B+ supply & the 6.3v AC filament supply is derived from the mains transformer in the background.

Magic Eye Tube Added
Magic Eye Tube Added

Here the magic eye tube has been fitted & is getting it’s initial tuning to the amplifier section. This requires selecting combinations of anode & grid resistors to set the gap between the bars while at no signal & picking a coupling RC network to give the desired response curve.

Final Test
Final Test

Here both valves are fitted & the unit is sitting on it’s case for final audio testing. the cathodes of the ECL82 can be clearly seen glowing dull red here.

 

In the final section, I will build a SMPS power supply into the unit to allow it to be powered from a single 12v DC power supply.