Minor constituents in the solar wind originating from plasma-dust interactions

Details Minor constituents in the solar wind originating from plasma-dust interactions Minor constituents in the solar wind originating from plasma-dust interactions

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nascp.2280.643r&link_type=abstract

In JPL Solar Wind Five p 643-645 (SEE N84-13067 03-92)

Physics

Interplanetary Dust, Ions, Plasma Interactions, Solar Wind, Zodiacal Dust, Atoms, Carbon, Helium, Hydrogen, Ion Charge, Ionization, Mass Spectroscopy, Molecules, Silicon

Scientific paper

Atoms, 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.

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