Plasma diagnostics and the heating of the solar corona
Firstly, we present reviews of the background atomic, magnetohydrodynamic, and solar, physics involved in the analysis of the problem. We proceed to produce a time dependent code to calculate the Ionisation state distribution of Iron and of Argon, using some of the recent data for Ionisation coeffic...
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University of Cambridge
2006
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.598268 |