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
The orientation of pre-transient coronal magnetic fields
โ Scribed by Gerard Trottet; R. M. MacQueen
- Publisher
- Springer
- Year
- 1980
- Tongue
- English
- Weight
- 636 KB
- Volume
- 68
- Category
- Article
- ISSN
- 0038-0938
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