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Minor constituents in the solar wind originating from plasma-dust interactionsAtoms, molecules, and atomic and molecular ions generated by solar wind interactions with dust grains of the zodiacal cloud are discussed. The main processes leading to the generation of these particles are described and relevant methods of observation are examined.
Document ID
19840005048
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Ripken, H. W.
(Bonn Univ.)
Date Acquired
August 12, 2013
Publication Date
November 1, 1983
Publication Information
Publication: JPL Solar Wind Five
Subject Category
Solar Physics
Accession Number
84N13116
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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