Abstract
In radio astronomy applications, antennas having the highest aperture efficiencies are requested. In order to meet this request, a reector shaping program for dual reector antennas has been developed. The design procedure is based on the geometrical optics where differential equations have been formulated to dene the ray trace of the antenna system. Recently, the fourth generation programming language MATLAB has become well known for its numerical computing environment and very useful three-dimensiona data visualization functions. The authors wished to make a dual reector shaping program by a ray tracing method in MATLAB. In this paper, details of the program are explained, and antenna ray tracing results are shown visually by three-dimensiona viewgraphs. The numerical results are compared with the theoretical ones to conrm the correctness of the developed shaping program for a Cassegrain dual reector antenna system. For uniform aperture distribution therst side lobe level is numerically obtained as {17.59 dB, which can be further reduced through shaping to {24.67 dB and {30.65 dB for parabolic and squared parabolic, respectively.
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