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Minor Ions in the solar Wind

Published online by Cambridge University Press:  25 April 2016

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It has been recently recognized that the presence of ions heavier than hydrogen determines to a large extent the dynamics of the expanding solar corona. In the following I shall give a brief account of the most recent results related to minor ions (i.e. He and ions heavier than helium).

Type
Research Article
Copyright
Copyright © Kluwer 1988 

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