Journal
JOURNAL OF PLASMA PHYSICS
Volume 79, Issue -, Pages 1071-1074Publisher
CAMBRIDGE UNIV PRESS
DOI: 10.1017/S0022377813001001
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Funding
- Alexander von Humboldt Foundation
- Presidium of the Russian Academy of Sciences [22]
- Russian Foundation for Basic Research [12-02-00270-a]
- International Space Science Institute
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Waves in a dusty plasma over the lunar dayside are considered. It is shown that the relative motion of the solar wind with respect to the photoelectrons over the lunar surface leads to the excitation of high-frequency oscillations with frequencies in the range of Langmuir and electromagnetic waves. The dust acoustic wave excitation is possible in the vicinity of the lunar terminator.
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