用于SMAP的6米网状反射面天线:模拟具有挑战性的地球轨道仪器的射频性能

P. Focardi, P. Brown, Y. Rahmat-Samii
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引用次数: 10

摘要

本文提出了一个完整而精确的SMAP天文台射频模型。在对航天器的所有重要部件进行建模时,都非常小心,以提供有关仪器在各种条件下性能的可靠信息。目前正在进行一项基于航天器和仪器不断发展的射频模型改进工作,以使模型保持最新状态。已经进行了实地研究,也正在考虑机械和热变形。由于没有计划对实际天线的辐射方向图进行测量,因此该射频模型的开发对该任务来说是一个非常重要的里程碑。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A 6-m mesh reflector antenna for SMAP: Modeling the RF performance of a challenging Earth-orbiting instrument
A complete and accurate RF model of the SMAP observatory has been presented in this paper. Extreme care has been used in modeling all the important parts of the spacecraft to provide reliable information about the performance of the instrument under various conditions. An ongoing work of RF model refinement based on the constant development of the spacecraft and instrument is also being carried on to keep the model up to date. Field of view studies have been performed and mechanical and thermal deformations are also being considered. Since radiation pattern measurements of the actual antenna are not planned, the development of this RF model represents a very important milestone for the mission.
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