[Moon-net] [Mw] CIRCULAR / LINEAR POL ON 10 GHz EME
Robert McGwier
rwmcgwier at comcast.net
Mon Oct 2 22:48:27 CDT 2006
(Why am I getting involved with this? Sigh. )
Jerry:
This dish at Bochum is pretty large.
http://www.amsat.org/amsat/archive/amsat-bb/200406/msg00232.html
It is 20 meters. In general, the beamwidth of an aperture that is X
wavelengths in size is about 1/X radians or about 57/X degrees.
Let's call the beamwidth of 1.22/X radians = 70/X degrees. The 1.22
number is often called the "Airy Criterion" (since this makes it larger).
So, depending on the illumination, the 20 meter dish at a wavelength of
3 cm, the quantity X is about 690 wavelengths wavelengths. Therefore
the beam will be about
(Airy criterion = 1.22)/(691 wavelengths) = .00183 radians = 0.1
degrees.
which is less than 20% of the (typically used) 0.5 degree moon. Paul's
feed (in use at Bochum) will be assumed to be spectacular and we will
take this number. I suspect that reflections aimed at the "dark seas"
which make up a large portion of the moon's visible face would scatter
less and if the dish happened to be aimed at these smoother areas, I
would expect demonstrably less scattering.
SO, I do not find this graph conclusive. More experiments with smaller
antennas showing a similar effect would be more suggestive.
Bob
N4HY
Jerry Kleker wrote:
> PLEASE RAINER, LOOK AT THIS PICTURE!
>
> http://groups.msn.com/W7QX/10ghzemepolarizationtests.msnw?action=ShowPhoto&PhotoID=72
> <http://groups.msn.com/W7QX/10ghzemepolarizationtests.msnw?action=ShowPhoto&PhotoID=72>
>
> IF 10 DB IS MARGINAL TO YOU.........
>
> 73,
>
> Jerry W7QX
--
AMSAT VP Engineering. Member: ARRL, AMSAT-DL, TAPR, Packrats,
NJQRP/AMQRP, QRP ARCI, QCWA, FRC. ARRL SDR Wrk Grp Chairman
"You see, wire telegraph is a kind of a very, very long cat.
You pull his tail in New York and his head is meowing in Los
Angeles. Do you understand this? And radio operates exactly
the same way: you send signals here, they receive them there.
The only difference is that there is no cat." - Einstein
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