Interstellar helium distribution in the heliosphere and interaction with the solar wind

Details Interstellar helium distribution in the heliosphere and interaction with the solar wind Interstellar helium distribution in the heliosphere and interaction with the solar wind

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980artsa..15...39g&link_type=abstract

(International Seminar of Magnetosphere, Ionosphere and Interplanetary Space, 2nd, Warsaw, Poland, June 21-23, 1979.) Artificial

Physics

Helium, Interstellar Gas, Neutral Gases, Plasma Interactions, Solar Wind, Space Plasmas, Distribution, Tables (Data)

Scientific paper

Heliospheric distribution of neutral He of galactic origin was calculated on a hot model for interstellar temperatures of 10,000 K, 15,000 K and interstellar velocities of 10 km/sec and 20 km/sec. The interaction of the resulting helium cone in the downwind region with the single-fluid distant solar wind is discussed. The relative increase of solar wind temperature due to friction with neutral He depends primarily on the interstellar temperature and not the interstellar velocity and is of the order of 10 - 30% at 10 AU, depending on the case.

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