PPT-SH31C-08: The Photospheric Poynting Flux and Coronal Heatin
Author : natalia-silvester | Published Date : 2016-06-17
Some models of coronal heating suppose that convective motions at the photosphere shuffle the footpoints of coronal magnetic fields and thereby inject sufficient
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SH31C-08: The Photospheric Poynting Flux and Coronal Heatin: Transcript
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