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Lunar nightside electron fluxesStudies of particle fluxes at the lunar surface with the Apollo 14 ALSEP/CPLEE particle spectrometer during lunar night periods have shown three distinct types of electron flux events. One of these is shown to originate at the earth's bow shock, but the remaining two are shown to arise most likely as a result of local solar wind-lunar interactions. The flux events had mean electron energies of a few hundred electron volts and total fluxes of 10 to the 5th to 10 to the 7th electrons/sq cm-sec. These fluxes are a possible source of the large negative lunar surface potentials observed by other ALSEP instruments
Document ID
19780062873
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Reasoner, D. L.
Date Acquired
August 9, 2013
Publication Date
January 1, 1975
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 17, 1975
End Date: March 21, 1975
Accession Number
78A46782
Funding Number(s)
CONTRACT_GRANT: NSG-07025
CONTRACT_GRANT: NAS9-5884
Distribution Limits
Public
Copyright
Other

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