欧几里德准备。第二十九篇。航天器中的水冰，第一部分：冰的形成和污染物的物理学
摘要：空间飞行中的分子污染是一个众所周知的问题。水是最常见的污染物，会改变低温光学系统的许多性质。如果冰太多，那么欧几里得的校准要求和科学目标将无法实现。欧几里得必须进行热污染去除，这是一个漫长且危险的过程。我们需要了解冰冻光学元件对数据的影响以及何时需要进行去污染。这对于建立适当的校准和调查计划至关重要，然而，在天体物理空间调查的背景下进行全面分析尚未完成。 在本文中，我们研究了其他存在有良好记录挥发出气的航天器，并回顾了薄冰膜的形成。我们预计欧几里得将出现无定形和晶体冰的混合。它们的表面形貌取决于基底水和水-水界面之间竞争的能量需求，并且很难通过当前的理论来预测。我们用扫描隧道显微镜和原子力显微镜图像来说明这一点。 工业工具存在用于估计污染物，我们必须了解它们的不确定性。我们发现扩散和升华系数的知识误差很大，限制了这些工具的准确性。我们开发了一个水运输模型来计算欧几里得的污染率，并与工业估计达成了一致。在太空模拟器中对欧几里得的飞行硬件进行的测试并没有发现污染信号；我们的飞行校准观测将更加敏感。 我们必须了解光学元件上冰的数量与其对欧几里得数据的影响之间的联系。关于这种联系的研究很少，可能是因为其他航天器可以轻松进行去污染，从而降低了对更深入理解的需求。在我们的第二篇论文中，我们量化了冰冻光学元件对光谱光度数据的各种影响。
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Marconi, 00185 Roma, Italy, (118) Centro de Astrof''isica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal, (119) Zentrum f"ur Astronomie, Universit"at Heidelberg, Philosophenweg 12, 69120 Heidelberg, Germany, (120) Dipartimento di Fisica - Sezione di Astronomia, Universit''a di Trieste, Via Tiepolo 11, 34131 Trieste, Italy, (121) Department of Mathematics and Physics E. De Giorgi, University of Salento, Via per Arnesano, CP-I93, 73100, Lecce, Italy, (122) INAF-Sezione di Lecce, c/o Dipartimento Matematica e Fisica, Via per Arnesano, 73100, Lecce, Italy, (123) INFN, Sezione di Lecce, Via per Arnesano, CP-193, 73100, Lecce, Italy, (124) Institute for Computational Science, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland, (125) Universit''e St Joseph, Faculty of Sciences, Beirut, Lebanon, (126) Department of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, NJ 08544, USA)
论文ID：2305.10107
分类：Instrumentation and Methods for Astrophysics
分类简称：astro-ph.IM
提交时间：2023-07-19