Impacts of fast meteoroids and a plasma–dust cloud over the lunar surface


如何引用文章

全文:

开放存取 开放存取
受限制的访问 ##reader.subscriptionAccessGranted##
受限制的访问 订阅存取

详细

The possibility of the formation of a plasma–dust cloud in the exosphere of the Moon owing to impacts of meteoroids on the lunar surface is discussed. Attention is focused on dust particles at large altitudes of ~10–100 km at which measurements were performed within the NASA LADEE mission. It has been shown that a melted material ejected from the lunar surface owing to the impacts of meteoroids plays an important role in the formation of the plasma–dust cloud. Drops of the melted material acquire velocities in the range between the first and second cosmic velocities for the Moon and can undergo finite motion around it. Rising over the lunar surface, liquid drops are solidified and acquire electric charges, in particular, owing to their interaction with electrons and ions of the solar wind, as well as with solar radiation. It has been shown that the number density of dust particles in the plasma–dust cloud present in the exosphere of the Moon is ≲10−8 cm−3, which is in agreement with the LADEE measurements.

作者简介

S. Popel

Space Research Institute; Moscow Institute of Physics and Technology (State University); National Research University Higher School of Economics

编辑信件的主要联系方式.
Email: popel@iki.rssi.ru
俄罗斯联邦, Moscow, 117997; Dolgoprudnyi, Moscow region, 141700; Moscow, 101000

A. Golub’

Space Research Institute

Email: popel@iki.rssi.ru
俄罗斯联邦, Moscow, 117997

L. Zelenyi

Space Research Institute; Moscow Institute of Physics and Technology (State University); National Research University Higher School of Economics

Email: popel@iki.rssi.ru
俄罗斯联邦, Moscow, 117997; Dolgoprudnyi, Moscow region, 141700; Moscow, 101000

M. Horányi

University of Colorado Boulder

Email: popel@iki.rssi.ru
美国, Boulder, CO, 80303

补充文件

附件文件
动作
1. JATS XML

版权所有 © Pleiades Publishing, Inc., 2017