Dusty plasma in the region of the lunar terminator
- 作者: Popel S.I.1,2, Zelenyi L.M.1,2, Atamaniuk B.3
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隶属关系:
- Space Research Institute
- Moscow Institute of Physics and Technology
- Space Research Center
- 期: 卷 42, 编号 5 (2016)
- 页面: 543-548
- 栏目: Dusty Plasma
- URL: https://journals.rcsi.science/1063-780X/article/view/185790
- DOI: https://doi.org/10.1134/S1063780X16050147
- ID: 185790
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详细
Dusty plasma in the region of the lunar terminator is considered. It is shown that, in this region, a structure resembling a plasma sheath forms near the lunar surface. This sheath creates a potential barrier, due to which electrons over the illuminated part of the Moon are confined by electrostatic forces. The width of the sheath-like structure is on the order of the ion Debye length. In this structure, significant (about several hundred V/m) electric fields arise, which lift charged micron-size dust grains to heights of several tens of centimeters. The suggested effect may be used to explain the glow observed by the Surveyor spacecraft over the lunar terminator.
作者简介
S. Popel
Space Research Institute; Moscow Institute of Physics and Technology
编辑信件的主要联系方式.
Email: popel@iki.rssi.ru
俄罗斯联邦, ul. Profsoyuznaya 84/32, Moscow, 117997; Institutskii per. 9, Dolgoprudnyi, Moscow oblast, 141700
L. Zelenyi
Space Research Institute; Moscow Institute of Physics and Technology
Email: popel@iki.rssi.ru
俄罗斯联邦, ul. Profsoyuznaya 84/32, Moscow, 117997; Institutskii per. 9, Dolgoprudnyi, Moscow oblast, 141700
B. Atamaniuk
Space Research Center
Email: popel@iki.rssi.ru
波兰, ul. Bartycka 18a, Warsaw, 00-716
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