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The draping of heliospheric magnetic fields upstream of coronal mass ejecta

โœ Scribed by Jones, G. H.


Book ID
118663664
Publisher
American Geophysical Union
Year
2002
Tongue
English
Weight
609 KB
Volume
29
Category
Article
ISSN
1944-8007

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โœ E. R. Priest; T. G. Forbes ๐Ÿ“‚ Article ๐Ÿ“… 1990 ๐Ÿ› Springer ๐ŸŒ English โš– 351 KB

Slow photospheric motions can produce flow speeds in the corona which are fast enough to violate quasi-static evolution. Therefore, high-speed flows observed in the corona are not necessarily due to a loss of equilibrium or stability. In this letter we present an example where the flow speed increas