欧盟冲击管用于高度研究的VUV到IR发射光谱和干涉测试诊断
Ricardo Grosso Ferreira1, Bernardo Brotas Carvalho1, Luís Lemos Alves1
1Instituto de Plasmas e Fusão Nuclear, Instituto Superior Técnico, Universidade de Lisboa, 1049-001 Lisbon, Portugal.
Sensors (Basel, Switzerland)
|July 14, 2023
概括
欧洲冲击管高度研究设施使用先进的诊断技术进行航天器进入模拟. 它可以为未来的欧洲太空探索任务进行关键的高速流量测量.
科学领域:
- 太空飞船工程 太空飞船工程
- 血物理学的等离子体物理学
- 空气动力学 航空动力学
背景情况:
- 欧洲航天局支持用于太空探索的先进研究设施.
- 高热流对于模拟行星进入条件至关重要.
- 以前的设施缺乏全面的诊断能力,无法进行详细的分析.
研究的目的:
- 详细介绍欧洲高度研究冲击管的设计和规格.
- 概述了行星进入模拟中的高速流量测量的要求.
- 讨论先进诊断系统的技术选择.
主要方法:
- 开发一个最先进的冲击管设施.
- 集成光学光谱学 (VUV到MIR) 覆盖120-5000nm.
- 微波干涉测量的实施用于测量高达1.5 × 10^20 m^-3.的电子密度.
主要成果:
- 该设施配备了先进的诊断系统,用于全面描述流量.
- 光谱学和微波干扰测量提供了关于等离子体条件的详细数据.
- 该设计成功地满足了对高速流量测量的严格要求.
结论:
- 欧洲高度研究冲击管是欧洲太空探索的关键资产.
- 该设施的诊断能够进行精确的测量,这对于任务的成功至关重要.
- 这项研究支持未来行星任务的技术开发.
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