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![]() "Emanuele Colucci" wrote in message ... Thanks to James for the advices and to Jerry and Jim for the news. Jerry: I'd like to know more about your solution, if you agree. ![]() Jim Lux ha scritto: There's a set of articles in IEEE Antennas and Propagation Magazine (not the transactions) a few years back that has all the equations and design rules for all of the various reflector configurations. Where I can find these articles? Best wishes, Emanuele Colucci Hi Emanuele I submit that, if you intend to actually build an antenna for L-Band and are restricting its diameter to 3 meters, you need not consider a cassegrain feed. The reflector at the focus is too small to allow the primary feed to illuminate it with a high percentage of the available source at the rear of the dish. For one example, let the cassegrain reflector be 1/2 meter diameter and be spaced 1meter from the apex of the dish. Wouldnt that suggest that the primary beam, from behind the dish will have a beamwidth of about 30 degrees (at -3dB)?? If the cassegrain reflector is made bigger, that blocks more of the parabolic dish apperature. If the cassegrain reflector is made smaller, that increases the need for a high gain primary feed. It is my contention that, if you want to research Cassegrain antennas, that is a worthy project. If you want to build a functing L-Band telescope with 3 meter dishes, dont include cassegrain feeds in the project. Jerry KD6JDJ |
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