Environmental Challenges to OASIS’s Primary Reflector

J. Arenberg, Micahaela N. Villareal, G. Harpole, D. McGregor, Ariane Walker-Horne, J. Pohner, Kevin Moore, Alex Clithero, Lauren Halvonik Harris, A. Palisoc
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引用次数: 2

Abstract

This paper discusses pressure control for the OASIS primary antenna element, A1. This discussion is centered around the evaluation of pressure changes and what might drive them. A1 is created from thin polyimide film and from its orbital position near Sun-Earth L1, is subject to many environmental effects, the solar wind, radiation pressure, charging and micrometeoroids. This paper begins by describing the architecture of the pressure control system. We show that the solar wind and radiation pressure are too small to impact A1’s performance. We also discuss the need to connect the A1 to system ground for solid technical and programmatic reasons. A large section discusses the micrometeoroid environment and how recent mission data shows that the flux faced by OASIS is likely larger by factor of ~3 than might be expected from naive application of the traditional models.
OASIS主反射器面临的环境挑战
本文讨论了OASIS主天线单元A1的压力控制。这个讨论的中心是对压力变化的评估以及可能驱动它们的因素。A1是由薄聚酰亚胺薄膜制成的,它的轨道位置靠近太阳-地球L1,受到许多环境影响,太阳风,辐射压力,充电和微流星体。本文首先介绍了压力控制系统的结构。我们表明,太阳风和辐射压力太小,不会影响A1的性能。我们还讨论了将A1连接到系统接地的必要性,这是出于坚实的技术和编程原因。有很大一部分讨论了微流星体环境,以及最近的任务数据如何显示OASIS面临的通量可能比传统模型的天真应用所预期的要大3倍。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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