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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Analysis and observation of spacecraft plume/ionosphere interactions during maneuvers of the space shuttle
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Analysis and observation of spacecraft plume/ionosphere interactions during maneuvers of the space shuttle

机译:航天飞机演习过程中航天器羽流/电离层相互作用的分析与观察

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This work employs in situ measurement data and constructive simulations to examine the underlying physical mechanisms that drive spacecraft plume interactions with the space environment in low-Earth orbit. The study centers on observations of the enhanced flux of plasma generated during a maneuver of Space Shuttle Endeavour as part of the Sensor Test for Orion Relative Navigation Risk Mitigation experiment in May 2011. The Canary electrostatic analyzer (ESA) instrument mounted on the portside truss of the International Space Station indicated an elevated ion current during the shuttle maneuver. The apparent source of enhanced ion current is a result of interaction of the spacecraft thruster plume with the rarefied ambient ionosphere, which generates regions of relatively high density plasma through charge exchange between the neutral plume and ambient ions. To reconstruct this event, unsteady simulation data were generated using a combined direct simulation Monte Carlo/particle-in-cell methodology, which employed detailed charge exchange cross-section data and a magnetic field model. The simulation provides local plasma characteristics at the ESA sensor location, and a sensor model is subsequently used to transform the local properties into a prediction of measured ion current. The predicted and observed total currents are presented as a function of time over a 30 s period of pulsed thruster firings. A strong correlation is observed in the temporal characteristics of the simulated and measured total current, and good agreement is also achieved in the total current predicted by the model. These results support conclusions that (1) the enhanced flux of plasma observed by the ESA instrument is associated with Space Shuttle thruster firings and (2) the simulation model captures the essential features of the plume interactions based on the observation data.
机译:这项工作采用了原位测量数据和建设性模拟,以检查驱动航天器羽流与低地球轨道中的空间环境的潜在物理机制。该研究中心关于在航天飞机努力运转期间产生的等离子体增强通量的研究中心,作为2011年5月的猎户座相对导航风险缓解实验的传感器测试的一部分。金丝雀静电分析仪(ESA)仪器安装在Portside Truss上国际空间站在穿梭机动期间表示离子电流升高。增强离子电流的表观源是航天器推进器羽状与稀污染的环境电离层相互作用的结果,其通过中性羽流和环境离子之间的电荷交换产生相对高密度等离子体的区域。为了重建该事件,使用组合的直接仿真蒙特卡罗/粒子电池方法产生不稳定的模拟数据,该方法采用详细的电荷交换横截面数据和磁场模型。该模拟在ESA传感器位置提供局部等离子体特性,随后使用传感器模型将本地特性转换为测量离子电流的预测。预测和观察到的总电流被呈现为30秒的脉冲推进器烧制的时间函数。在模拟和测量的总电流的时间特征中观察到强烈的相关性,并且在模型预测的总电流中也实现了良好的一致性。这些结果支持结论:(1)ESA仪器观察到的等离子体的增强通量与航天飞机推动和(2)仿真模型基于观察数据捕获羽流相互作用的基本特征。

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