Mixed solar wind originating from coronal regions of different temperatures

Details Mixed solar wind originating from coronal regions of different temperatures Mixed solar wind originating from coronal regions of different temperatures

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nascp.2280.613b&link_type=abstract

In JPL Solar Wind Five p 613-622 (SEE N84-13067 03-92)

Computer Science

1

Ion Charge, Ionization, Solar Corona, Solar Wind, Carbon, Helium Ions, Magnesium, Mass Spectra, Metal Ions, Silicon

Scientific paper

Ionization states of elements in the solar wind have been 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. In this paper, the author investigates features in M/Q-spectra which might appear if the above assumption is violated and compares them with observational evidence.

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