Plasma wake simulations and object charging in a shadowed lunar crater during a solar storm
Plasma wake simulations and object charging in a shadowed lunar crater during a solar storm
复制标题
太阳风暴期间阴影月球陨石坑中的等离子体尾流模拟和物体充电
DOI:
10.1029/2012je004094
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发表时间:
2012
影响因子:
--
通讯作者:
T. Stubbs
中科院分区:
文献类型:
--
作者:
M. Zimmerman;T. Jackson;W. Farrell;T. Stubbs
[1] Within a permanently shadowed lunar crater the horizontal flow of solar wind is obstructed by upstream topography, forming a plasma wake that electrostatically diverts ions toward the crater floor and generates a surface potential that can reach kilovolts. In the present work kinetic plasma simulations are employed to investigate the morphology of a lunar crater wake during passage of a solar storm. Results are cast in terms of leading dimensionless ratios including the ion Mach number, ratio of crater depth to plasma Debye length, peak secondary electron yield, and electron temperature versus electron impact energy at peak secondary yield. This small set of ratios allows generalization to a much wider range of scenarios. The kinetic simulation results are fed forward into an equivalent-circuit model of a roving astronaut. In very low-plasma-current environments triboelectric charging of the astronaut suit becomes effectively perpetual, representing a critical engineering concern for roving within shadowed lunar regions. Finally, simulated ion fluxes are used to explore sputtering and implantation processes within an idealized crater. It is suggested that the physics of plasma miniwakes formed in the vicinity of permanently shadowed topography may play a critical role in modulating the enigmatic spatial distribution of volatiles at the lunar poles.