Interpretation of Solar Wind Composition Measurements from Ulysses

Details Interpretation of Solar Wind Composition Measurements from Ulysses Interpretation of Solar Wind Composition Measurements from Ulysses

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999stin...9914461e&link_type=abstract

Technical Report, Smithsonian Astrophysical Observatory Cambridge, MA United States

Astronomy and Astrophysics

Astrophysics

Solar Corona, Solar Wind, In Situ Measurement, Ion Charge, Ions, Electron Density (Concentration), Solar Wind Velocity, Interplanetary Space, Ulysses Mission, Charged Particles, Flow Velocity

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. This information is, however, not easy to extract from the in situ observations. The goal of the proposal was to determine solar wind models and coronal observations that are necessary tools for the interpretation of charge state observations. It has been shown that the interpretation of the in situ ion fractions are heavily dependent on the assumptions about conditions in the inner corona.

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