2011Unpublished venueRequires access

Characterizing reflector-feed interaction for parabolic reflector antennas

Mark A. Apeldoorn

Open publisher page 1 citations

Abstract

Radio telescopes are quite often used for astronomy. Since these telescopes are wideband systems, they encounter standing waves between the reflector and the feed. This interaction has been studied by investigation the radar cross section (RCS) of the feed and the effect the standing waves have on the antenna performance (gain and beamwidth).

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What this paper is about

Radio telescopes are quite often used for astronomy. Since these telescopes are wideband systems, they encounter standing waves between the reflector and the feed. This interaction has been studied by investigation the radar cross section (RCS) of the feed and the effect the standing waves have on the antenna performance (gain and beamwidth).

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Available abstract

Radio telescopes are quite often used for astronomy. Since these telescopes are wideband systems, they encounter standing waves between the reflector and the feed. This interaction has been studied by investigation the radar cross section (RCS) of the feed and the effect the standing waves have on the antenna performance (gain and beamwidth).

Key concepts: Cassegrain antenna, Beamwidth, Parabolic antenna, Offset dish antenna, Fan-beam antenna, Reflector (photography), Parabolic reflector, Feed horn

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