Radial and Meridional Trends in Solar Wind Thermal Electron Temperature and Anisotropy: ULYSSES

Details Radial and Meridional Trends in Solar Wind Thermal Electron Temperature and Anisotropy: ULYSSES Radial and Meridional Trends in Solar Wind Thermal Electron Temperature and Anisotropy: ULYSSES

Apr 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ssrv...72..109p&link_type=abstract

Space Science Reviews, Volume 72, Issue 1-2, pp. 109-112

Physics

18

Scientific paper

Ulysses plasma measurement from 1.15 to 5.31 AU and from S6.4° to S48.3° solar latitude are used to assess the trends in the solar wind thermal electron temperature and anisotropy. Improved spacecraft potential corrections and data products have been incorporated. The radial temperature gradient is steeper than in previous determinations, but flatter than adiabatic. When normalized to 1 AU, temperature decrease with increasing latitude. Little change in the average thermal anisotropy has been seen during the mission.

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