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Cristiana Dumitrache Submitted: 2007-12-15 15:04
Coronal streamers are very interesting, long lived, features of solar corona. They are linked to prominences, CMEs and also to slow solar wind. The have different shape and behavior.
We present a numerical simulation of a coronal streamer computed on five solar radii. Vertical motions in the streamer, both ascending and descending, are revealed during the streamer evolution, as well as eddy flows.
Authors: C.Dumitrache
Projects: None
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Publication Status: AIP Conference Proceedings 934, 129-138, 2007
Last Modified: 2007-12-15 22:02
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