A Red Light Source For Optical Testing

Light sources for astronomical testing do not have to be expensive. The light source needs to replicate a star. Stars are extremely large but since they are an extremely long way away, they appear as a very small light source. To replicate them in a workshop all you really need is an extremely small light source.

Happily for us, a small light source capable of testing down below PV 1/10λ Wavefront accuracy can be made extremely cheaply from a standard red LED laser pointer that can be bought for a couple of pounds.

Example types are in the photographs below:- If you can't find one for less than £3, - you are not looking hard enough!

 

Section Through Red Laser Pointer

If you were to section one of these laser pointers, you would see the basic arrangement in the drawing adjacent.

The laser unit is powered by three small cells connected in series to give a maximum voltage of about 4V.

There is a simple push button switch that must be held in to turn the laser on. The source that generates the light is a very small Red LED Laser Diode.

This produces a spherical Wavefront that is collimated to a parallel "Laser" beam by a small lens.

The position of the lens is adjusted by a screw thread and spring to set the exiting beam completely parallel. (In some pointers, the threads are subsequently locked with superglue before despatch.)

 

Basic Laser Module With 6mm Removed

Once you have found one of these in the shops or on the internet, it can be converted to a light source simply by removing or unscrewing the front lens. This gives access to the expanding spherical Wavefront from the tiny Laser diode. This leaves you with a nearly perfect light source for optical testing of astronomical mirrors.

If the laser is a type supplied with the lens screw threads locked with superglue, then saw off 4-6mm from the front of the unit with a small hacksaw. This is usually sufficient to release the front lens. The picture adjacent is an example of one of these types with 6mm removed from the front.

Clothes Peg Holds Button In

To operate the push button needs to be held in. Probably the simplest way to do this is with something like a clothes peg. There is no reason the peg cannot also perhaps double up as part of the arrangement for holding the light source?

The internal batteries have sufficient life for occasional use. They are a common type so are easy to find in the shops and cheap to buy.

Be aware when changing batteries that inside the tube there is a thin cellophane sleeve that stops the metal cases of the batteries shorting out on the inside of the metal tube. If this sleeve gets displaced or slips out, the pointer will not work and the cells will soon run flat. This sleeve slipping out seems to be the major cause of failure of these cheap units.

If the cellophane sleeve does get damaged, - then all is not lost! - Try one turn of sello-tape round a pack of three batteries together, and push the pack carefully back into the tube.

LED Module Out Of Tube

Oldham Optical uses red light sources similar to these Red LED laser Diode modules to test mirrors.

In our case we require regular and continuous use so using the internal batteries would not be very sensible, We would have to change them too often. We have specially made mains power supplies in the workshop to power the lasers. These supplies give a variable DC Voltage adjustable between 2-3.5 Volts to give variable light levels.

So if a considerable amount of testing is being considered then the laser pointer needs to be taken apart to allow wires to be inserted into the pointer to allow external batteries or a mains power supply to be used. This also allows a potentiometer to vary the light level.

Being able to vary the light level is a good bonus. While a bright light is useful for setting up, a very dim light can be better for accurate testing.)

Once the first 4-6mm is cut off to release the lens, the module can be taken apart as follows:-

The LED module is a push fit into the front of the tube. Pressure on the collar can be released with a short longitudinal saw-cut from the front of the tube back about 8mm maximum, as seen in the upper part of the photo adjacent. This will usually allow the module to fall out, - or if not it can be gently pushed out from the back using a screwdriver or similar tool. The module removed is in the lower part of the photo adjacent.

 

External Battery Unit

Although Oldham Optical uses mains power supplies in the workshop, we often give demonstrations of astronomical mirror testing at various gatherings away from the workshop. For these rather than take a mains supply that needs somewhere to plug it in, we take a simple external battery unit as depicted adjacent.

This one contains a battery holder for three AA cells together with a 500 Ohm potentiometer to vary the light intensity and a pair of terminals. The circuit of the unit is adjacent.

We suggest a power supply of this type will have more than sufficient capacity for any amount of testing contemplated by an amateur mirror maker and it saves the expense of a mains powered unit. 

LED Module Wired Up

A small flexible 2 core cable like "Bell-Wire" is used to wire the module. The negative wire is soldered to one of the switch contacts, - but beyond the switch mechanism itself, - so it no longer needs to be pressed to operate the LED. The laser does not like a lot of heat, - so its a quick dab on with the soldering iron. Preferably use the switch terminal away from the one with the printed circuit board track leading to the laser diode.

In the picture above, the spring that connects the front battery to the module can be seen poking out of the tube. This can be cut off if it gets in the way.

Do not attempt to solder the positive contact. Depending on what type of module you have got, the collar of the module is made either from low melting point metal or is just plastic covered with conductive metallic paint. Instead arrange the positive wire length so when the module is pressed back into the tube, the wire is trapped between the module collar and the tube. The right length can be seen in the photograph above.

The module will easily press back into the tube using a vice. The positive wire should first have the individual cores spread out slightly so they are not bunched up so will make good contact with the tube and collar.

The tube can be shortened as required with a hack saw to clear the longitudinal saw-cut that was originally made to release the module.

Completed LED module and External Battery PSU

To complete the unit, push some tissue paper down the tube from the back round the wire. Seal it in with a few drops of Uhu or similar glue. But make sure the glue does not run forward as far as the LED module.

The paper and glue are to provide support to the wire, so it, (and the soldered connection to the diode module), is less likely to break off when used.

Fit appropriate plugs or connectors to the other ends of the wires to connect to your power supply. Make sure its easy to tell positive and negative apart as connecting up the wrong way round will probably destroy the LED.

Otherwise you will have to find another laser pointer and start all over again.

The unit is now finished and you are ready to start testing mirrors.

 

Why Green Laser Pointers are no Good!

Green Laser Pointer

Green Laser Pointer Head DrawingThe present generation of green laser pointers do not develop their light directly from a small point on a laser diode. They are "true Lasers".

The main method used to produce green light is to first shine infra red light at 880nm, (produced from a infra-red diode), into a material that absorbs it but re-emits a signal at 1064nm.

This is then fed into a different material adjacent that absorbs the 1064nm signal and re-emits at double the frequency to give green light at 532nm.

The cavity where this occurs has mirrors at each end with only a single small hole in the mirror surface at one end. The result is that green light is emitted from the head through the hole in the mirror surface as a very narrow intense parallel beam. In this form it is no use for testing astronomical mirrors.

This is a pity, - because green would be about the best possible match we can get for the main optical sensors we use for testing in our workshop. (The human eye is most sensitive to yellow-green light!)

Green ones are extremely good for pointing out stars at star parties. In this respect they beat the red ones easily.

And we do understand that work is continuing to produce a true green laser diode. When they do, - these will be better for optical testing.

Why Blue Laser Pointers are no Good!

Blue Laser Diode DrawingBlue Laser DiodeBlue laser diodes are the most recent type to be introduced to the market. They are being produced principally for Blu-ray recorders. They are expensive compared to Red or Green types, but they are potentially better than red light units for optical testing. The light frequency being blue is higher and - much more importantly for optical testing, - The blue light is produced from an even smaller area than in the red units.

The present blue units are extremely powerful, and blue light is known to damage the eye more easily than red or green, so if these are being considered for optical testing, then the power supply circuit to run them needs to be produced specifically with optical testing in mind and be limited to very low current.

Blue diode modules and power supplies to drive them are available on the internet but be aware the usual power supplies are sized to drive the blue modules up to full power. They must be altered or restricted to an extremely low current before you should consider using a blue module for astronomical testing. With a module we tried, only 1mA was needed to develop sufficient light for testing.

Section Through Blue Laser Diode ModuleBut there is a problem with the units we have seen at present. They also produce a lot of stray white light. As we presently understand the process, white light is first generated by a LED and illuminates another material which is what generates the blue light. In doing so the white light illuminates the interior of the module, reflecting off various internal parts and fixtures and then finds the exit window.

So there is a lot of stray white light and it appears to come from the full area of the window. The effect for optical testing is the stray white light from a large area tends to swamp out the blue light. Nulls become more difficult to identify. The result is that optical testing with the present blue modules has no advantage over red units. 

Its surprising the stray white light is not an issue for reading and burning Blu-ray disks. It's certainly a bit of a killer for optical testing.

If in future a blue light unit was to be produced without as much stray white light, - it would become a contender for testing astronomical optics.

But whether the shorter wavelength from a future blue laser diode would test better than a future Green laser diode with its better eye sensitivity? - We have no idea. 

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