Effect of the solar wind on the formation of a photoinduced dusty plasma layer near the surface of the Moon
Effect of the solar wind on the formation of a photoinduced dusty plasma layer near the surface of the Moon
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DOI：
10.1134/s0021364013240144
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发表时间：
2014-02-01
期刊：
影响因子：
1.3
通讯作者：
Fortov, V. E.
中科院分区：
文献类型：
--
作者：
Lisin, E. A.;Tarakanov, V. P.;Fortov, V. E.
在紫外线辐射以及快速和慢速太阳风的作用下，月球表面被照射部分附近形成的尘埃等离子体层已被数值模拟。数值计算（包括传送到地球的月球风化层样本的光发射特性）已与已知理论模型中的估计值进行了比较。研究表明，太阳风粒子通量对表面光电子层的形成起着重要作用。分析了月球表面等离子体层尘埃粒子的带电和稳定悬浮条件。
A dusty plasma layer formed near the illuminated part of the surface of the Moon under the action of ultraviolet radiation, as well as fast and slow solar wind, has been numerically simulated. The numerical calculations including the photoemission properties of lunar regolith samples delivered to the Earth have been compared to estimates within known theoretical models. It has been shown that the flux of solar wind particles plays an important role in the formation of the surface photoelectron layer. The conditions of the charging and stable levitation of dust particles in the surface plasma layer of the Moon have been analyzed.