基于导电轨迹的空间碎片原位检测评估新方法

Sebastian Fexer
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摘要

为了能够探测亚毫米范围内的微流星体和小型空间碎片,航天器上的原位探测器是首选工具。不幸的是,直到今天,只有几个项目被送到了太空。然而,了解MMSD的数量对于保持参考模型的最新状态和对碎片数量及其沿特定轨道分布等因素的更多了解是很重要的。这对当前和未来太空飞行任务的安全至关重要。目前的原位探测系统主要依赖于使用不同方法的冲击识别和表征。其中之一是在这种事件中特殊探测区域的穿孔。这些区域由具有导电迹线的一个或多个层组成。这些线路中的任何中断都可以通过某种电气连续性测试方法或电阻的测定来识别。这也伴随着一些缺点,比如沿一行进行多事件识别很困难,甚至是不可能的。提出的概念依赖于反射方法。例如,在这样做的过程中,脉冲沿着一条定义明确的传输线发送,这是探测区域的一部分。任何特征线阻抗的改变,例如,由于撞击,将产生反射回发电机。它们的评估可以提供扰动的位置和复杂阻抗。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A novel evaluation method for in situ space debris detection based on conductive traces
To enable the detection of micrometeoroids and small-sized space debris (MMSD) in the sub-mm range, in situ detectors aboard a spacecraft are the tool of choice. Unfortunately, only a few projects have been sent to space until today. However, knowledge of the MMSD population is important to keep the reference models up-to-date and gain more insights into factors like the amount of debris and its distribution along certain orbits. This will be crucial for the safety of current and future spaceflight missions. Present-day in situ detection systems mostly rely on impact recognition and characterization using different methods. One of them is the perforation of a special detection area during such an event. These areas consist of one or more layers provided with conductive traces. Any interruption of one of these lines can be recognized using some kind of electrical continuity testing method or the determination of the resistance. This goes along with some drawbacks, like the difficult or even impossible multi-event recognition along one line. The proposed concept relies on a reflectometric approach. In doing so, for example, pulses are being sent along a well-defined transmission line, which is a part of the detection area. Any alteration in the characteristic line impedance, for instance, due to an impact, will generate reflections back into the generator. Their evaluation can provide the location as well as the complex impedance of the perturbation.
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