Abstract

Scrimp horns and stacked Fabry-Perot (FP) cavity antennas with small radiating apertures (≤ 2.5λ <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">0</sub> ) are very attractive antenna solutions for global Earth illumination or primary feeds of focal arrays. Several antennas of each type have been optimized for different radiating sizes, and their radiation characteristics are compared in terms of aperture efficiency and pattern quality. It is shown that scrimp horns provide excellent aperture efficiencies over large bandwidths, but are limited to applications requiring aperture sizes smaller than 2λ <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">0</sub> . It is also demonstrated that the stacked FP cavity antennas are very promising for aperture sizes varying between 1.5λ <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">0</sub> and 2.5λ <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">0</sub> , and show comparable performances to scrimp horns for aperture size lower than 2λ <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">0</sub> ; they also exhibit higher aperture efficiencies for apertures larger than 2λ <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">0</sub> while keeping the antenna height fixed at λ <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">0</sub> in contrast to scrimp horns with height increases naturally with the aperture size.

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