[Laser] a simple test
TWOSIG at aol.com
TWOSIG at aol.com
Fri Apr 28 17:55:02 EDT 2006
The next time you setup your light receiver, here is a simple test that
may give you some insight into how well your system is adjusted.
Point the receiver at a moderate to weak, isolated signal source. It
should be strong enough to be clearly above the noise level, at least 6
dB if you can measure it. The source should be isolated that you can
swing the receiver so that the source is out of the receiver field of
view without picking up another source of similar or greater strength.
Then block off half the aperture of the receiver. A sheet of black
construction paper should work by holding it in front of the lens so
that only half the lens can "see" the source. The signal should drop by
3 dB. Then shift the paper so that the other half of the lens can "see"
the source. It should sound the same, that is 3 dB down from the clear
aperture.
Another way to run the test, that may give clearer results, would be to
cut a hole in the black paper that is half the diameter of the the lens.
The area of the hole is one fourth the area of the lens (assuming that
it is a round lens) so it should result in 6 dB drop in signal. You may
need a stronger source. If you move the paper so that different areas
of the lens are exposed, there should be no change in the signal
strength as the paper moves.
The purpose of the test is to determine if parts of your lens are not
providing light to your detector as effectively as other parts. If
there is an inconsistency, particularly if you find parts of your lens
are "dead", then it is likely that your sensor is not placed at the
proper distance from the lens, and therefore light is spilling past your
sensor. It is also likely that you are more prone to get other noise
sources rather than the source you want.
The situation may not be all bad. If you are getting enough light to be
able to communicate, and if there is not interference from other
sources, it may mean that you have a wider field of view. That in turn,
may make it easier for you to find your desired source. On the other
hand, if you are just a few millimeters off the correct distance from
the lens, you can be losing 20 to 40 dB of signal.
The test is based on a technique, called a Hartman Mask, used by
astronomers, both amateur and professional, to adjust the focus of their
telescopes. I believe that the technique is used more often for
astrophotograph than visual observing. I think of light communication
receivers as single pixel telephoto cameras. There seems to be a lot of
problems that telescope makers (and users) have had and worked on
solving, that can be transferred to light communications.
James
N5GUI
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