Properties of Minor Ions in the Solar Wind and Implications for the Background Solar Wind Plasma

Details Properties of Minor Ions in the Solar Wind and Implications for the Background Solar Wind Plasma Properties of Minor Ions in the Solar Wind and Implications for the Background Solar Wind Plasma

Nov 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001stin...0210113e&link_type=abstract

Technical Report, Smithsonian Astrophysical Observatory Cambridge, MA United States

Astronomy and Astrophysics

Astrophysics

Solar Wind, Plasma Interactions, Ion Charge, Ions, Interplanetary Space, Charged Particles, Coronas

Scientific paper

Ion charge states measured in situ in interplanetary space carry information on the properties of the solar wind plasma in the inner corona where these ion charge states are formed. The goal of the proposed research was to determine solar wind models and coronal observations that are necessary tools for the interpretation of the ion charge state observations made in situ in the solar wind.

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