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  • 1
    Publication Date: 2011-08-17
    Description: Observations of the average oxygen ionization equilibrium as a function of speed of the solar wind are presented. At low solar wind speeds they indicate a coronal temperature at the freezing-in point of (1.6 + or - 0.2) x 10 to the 6th K. At speeds above 450 km/sec the apparent temperature starts to rise rapidly. This rise is tentatively interpreted in terms of a lack of thermodynamic equilibrium in the source region.
    Keywords: SOLAR PHYSICS
    Type: Geophysical Research Letters; 7; Aug. 198
    Format: text
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