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Mixed solar wind originating from coronal regions of different temperaturesIonization 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.
Document ID
19840005046
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Bochsler, P.
(Bern Univ. Bern, Switzerland)
Date Acquired
August 12, 2013
Publication Date
November 1, 1983
Publication Information
Publication: JPL Solar Wind Five
Subject Category
Solar Physics
Accession Number
84N13114
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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