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Coronal magnetic field evolution under reconnective relaxation

✍ Scribed by G. E. Vekstein; E. R. Priest; R. Wolfson


Book ID
104935297
Publisher
Springer Netherlands
Year
1994
Tongue
English
Weight
257 KB
Volume
70
Category
Article
ISSN
0038-6308

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The evolution of coronal magnetic fields
✍ E. R. Priest; T. G. Forbes πŸ“‚ Article πŸ“… 1990 πŸ› Springer 🌐 English βš– 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