Reflectarray RF Modeling and Optimization for the VenSAR Mission
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http://dataverse.jpl.nasa.gov/citation?persistentId=doi:10.48577/jpl.X16V9D
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This paper describes the RF modeling and optimization of the reflectarray antenna for the Venus Synthetic Aperture Radar (VenSAR) instrument. VenSAR is a dual-polarized radar operating at S-band (3.2 GHz). The antenna will be employed to perform scientific studies of the surface of Venus. The reflectarray is illuminated by a feed, which is composed of two horns to generate dual polarization (horizontal and vertical). The reflectarray was optimized for beamwidth, side-lobe level, and directivity using the QUPES tool of TICRA. The RF model includes the impact of the spacecraft deck on which the reflectarray antenna is mounted. A comparison is made of the reflectarray performance including a preliminary representation of the top deck to the ideal case (no scattering from the deck).
本文描述了用于金星合成孔径雷达(VenSAR)仪器的反射阵列天线的射频建模与优化。VenSAR是一款工作于S波段(3.2 GHz)的双极化雷达,该天线将用于开展金星表面的科学研究。反射阵列由一个馈源照射,该馈源包含两个喇叭以产生双极化(水平与垂直)。反射阵列通过TICRA公司的QUPES工具针对波束宽度、旁瓣电平及方向性进行了优化。射频模型包含了反射阵列天线所安装的航天器甲板的影响。本文对包含顶部甲板初步模型的反射阵列性能与理想情况(无甲板散射)进行了对比。
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Root
创建时间:
2025-04-20



