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    Transition from a supersonic to a subsonic solar wind (1972)
    In:  CASI
    Details
    Publication Date: 2016-06-07
    Description: The transition from a supersonic to a subsonic corona was investigated by increasing the density N sub O at the base of the corona while keeping the temperature T sub O constant. For the initial values of N sub O and T sub O, the solution of the inviscid solar wind equations is of the Parker type. As N sub O is increased, Parker type supersonic solutions cease to exist. No subsonic solutions exist.
    Keywords: SPACE RADIATION
    Type: NASA. Ames Res. Center Solar Wind; p 232-235
    Format: application/pdf
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