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    Mixed solar wind originating from coronal regions of different temperatures (1983)
    In:  CASI
    Details
    Publication Date: 2016-06-07
    Description: Ionization states of elements in the solar wind are often used to determine thermal gradients in the lower corona. This method is based on the assumption, that in the beginning, solar wind material has a homogeneous temperature determining the original charge state of elements. Features in M/Q-spectra which might appear if the above assumption is violated are investigated and compared with observational evidence.
    Keywords: SOLAR PHYSICS
    Type: JPL Solar Wind Five; p 613-622
    Format: application/pdf
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