The evolution of coronal loops in response to slow photospheric twisting motions is investigated using a variety of methods. Firstly, by solving the time-dependent equations it is shown that the field essentially evolves through a sequence of 2-D equilibria with no evidence of rapid dynamic evolutio
Modeling of dynamic evolution of coronal loops
โ Scribed by T. V. Stepanova; A. G. Kosovichev
- Publisher
- Springer Netherlands
- Year
- 1994
- Tongue
- English
- Weight
- 249 KB
- Volume
- 70
- Category
- Article
- ISSN
- 0038-6308
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๐ SIMILAR VOLUMES
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