Beware that 40m on 21cm is at the Fraunhofer limit for a 2m dish. If your dish is bigger than 2m, you will need to go farther away., to make meaningful measurements of the dish parameters.
The formula for minimum distance is two times dish diameter squared divided by wavelength, for 1/16 wavelength phase error (plus minus 1/32).
Also, if you set your focus with a relatively close source, you will set it too far out. Using the thin lens equation, say your focal length is one meter, and your source is 40m away - that is 40 focal lengths. This wil cause your focal point to be 1/40 focal length farther out, that is 2.5cm.
BTW, when seeking focus, the best way is to go for deep nulls betwen main and first side lobe (remember the Airy disk and diffraction rings).
Deep nulls also tell you that your dish is in good shape - again, think of "star testing" an optical telescope.
Marko Cebokli
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Hi Volker,
There are two things which you might want to consider:
With a 3.8m dish and 21cm wavelength you are still in near field conditions at 40m distance. Due to this, optimizing the dish will not give you correct results. You would need to be at least some 150m away.
Then, using the test transmitter might give you problems: Putting aside the question of legality of transmitting in the radio astronomy band, the additional trouble is that the minicircuits has high harmonics. The first harmonic (2840 MHz) is within the band of air traffic control radar systems.
Cheers
Wolfgang
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