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  • 1
    Publication Date: 2011-08-16
    Description: The effects of the reduction in the thermal conductivity due to heavy ions on electron temperatures in the solar corona and solar wind are examined. Large enhancements of heavy ions in the corona appear to be necessary to give appreciable changes in the thermal gradient of the electrons. These enhancements, if they should occur, may contribute to the understanding of some low values of solar wind temperature measurements at 1 AU.
    Keywords: SPACE RADIATION
    Type: Journal of Geophysical Research; 79; Jan. 1
    Format: text
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