Physical processes of formation and features of the plasma-dust exosphere of the Moon

被引:3
作者
Zelenyi, L. M. [1 ]
Zakharov, A., V [1 ]
Popel, S., I [1 ,2 ]
Kuznetsov, I. A. [1 ]
Rosenfeld, E., V [3 ]
机构
[1] Russian Acad Sci, Space Res Inst, Ul Profsoyuznaya 84-32, Moscow 117997, Russia
[2] HSE Univ, Ul Myasnitskaya 20, Moscow 101000, Russia
[3] Russian Acad Sci, Mikheev Inst Met Phys, Ural Branch, Ul S Kovalevskoi 18, Ekaterinburg 620108, Russia
关键词
Moon; plasma; lunar dust; solar wind; micrometeoroids; regolith; exosphere; LUNAR-SURFACE; SOLAR-WIND; PHOTOELECTRON SHEATH; TERMINATOR REGION; ILLUMINATED PART; MAGNETIC-FIELDS; TRANSPORT; LEVITATION; PARTICLES; SODIUM;
D O I
10.3367/UFNe.2023.09.039567
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We review studies of physical processes associated with the impact of external factors in outer space flows of micrometeoroids and solar radiation on the lunar regolith. Under the influence of these factors, regolith microparticles can detach from the surface and levitate. Near-surface plasma and levitating dust particles form a plasma-dust exosphere of the Moon. Under anthropogenic effects on the lunar environment, charged levitating microparticles can have an extremely negative impact on the engineering systems of lunar landers and on the activity and health of astronauts on the Moon. Based on information gained by automated and manned lunar missions and in laboratory experiments, we discuss modern ideas about physical processes occurring near the Moon's surface. Unsolved problems associated with the plasma-dust exosphere of the Moon are considered, and the principal strategies for their solution are outlined.
引用
收藏
页码:533 / 560
页数:28
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