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arXiv · 1101.5682

Measurements of Antenna Surface for Millimeter-Wave Space Radio Telescope

Kazuhisa Kamegai·Masato Tsuboi·Akihiro Doi·Eiichi Sato
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Abstract

In the construction of a space radio telescope, it is essential to use materials with a low noise factor and high mechanical robustness for the antenna surface. We present the results of measurements of the reflection performance of two candidates for antenna surface materials for use in a radio telescope installed in a new millimeter-wave astronomical satellite, ASTRO-G. To estimate the amount of degradation caused by fluctuations in the thermal environment in the projected orbit of the satellite, a thermal cycle test was carried out for two candidates, namely, copper foil carbon fiber reinforced plastic (CFRP) and aluminum-coated CFRP. At certain points during the thermal cycle test, the reflection loss of the surfaces was measured precisely by using a radiometer in the 41-45 GHz band. In both candidates, cracks appeared on the surface after the thermal cycle test, where the number density of the cracks increased as the thermal cycle progressed. The reflection loss also increased in proportion to the number density of the cracks. Nevertheless, the loss of the copper foil surface met the requirements of ASTRO-G at the end of the equivalent life, whereas that of the aluminum-coated surface exceeded the maximal value in the requirement even before the end of the cycle.

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Kazuhisa Kamegai, Masato Tsuboi, Akihiro Doi, Eiichi Sato. 2011-01-29. Measurements of Antenna Surface for Millimeter-Wave Space Radio Telescope. https://doi.org/10.1093/pasj%2F63.3.475

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