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Chromospheric and Coronal Heating Mechanisms
Published online by Cambridge University Press: 19 July 2016
Extract
Stellar chromospheres lose energy, predominantly, via radiation and coronae via conduction, radiation and stellar wind flows. To prevent these hot layers from rapidly cooling down to photopsheric temperature some source of heating must be present.
- Type
- III. Stellar Plasmas
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- Copyright © Kluwer 1990