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New SPIS Capabilities to Simulate Dust Electrostatic Charging, Transport, and Contamination of Lunar Probes

机译:新的SPIS功能可模拟尘埃静电充电,传输和污染月球探测器

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摘要

The spacecraft–plasma interaction simulator has been improved to allow for the simulation of lunar and asteroid dust emission, transport, deposition, and interaction with a spacecraft on or close to the lunar surface. The physics of dust charging and of the forces that they are subject to has been carefully implemented in the code. It is both a tool to address the risks faced by lunar probes on the surface and a tool to study the dust transport physics. We hereby present the details of the physics that has been implemented in the code as well as the interface improvements that allow for a user-friendly insertion of the lunar topology and of the lander in the simulation domain. A realistic case is presented that highlights the capabilities of the code as well as some general results about the interaction between a probe and a dusty environment.
机译:改进了航天器-等离子体相互作用模拟器,可以模拟月球和小行星尘埃的发射,传输,沉积以及与月球表面或接近月球的航天器的相互作用。规范中已认真实现了粉尘充电的物理原理以及粉尘承受的力。它既是解决表面探月仪面临的风险的工具,也是研究粉尘传输物理学的工具。在此,我们将介绍代码中已实现的物理原理以及接口改进,这些接口改进可在模拟域中方便地插入月球拓扑和着陆器。提出了一个现实的案例,该案例突出了代码的功能以及有关探针和多尘环境之间相互作用的一些常规结果。

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