A new magnetodynamic model for loop flares is proposed to explain the following observational facts obtained from space during the last solar activity maximum: (i) Blueshifted lines of CaxIx and Fe xxv appear in some cases a minute or so before the initiation of impulsive bursts and relax into the u
โฆ LIBER โฆ
Heating and reconnection of the emerging magnetic flux-tubes and the role of the interchange instability
โ Scribed by Yutaka Uchida; Takashi Sakurai
- Publisher
- Springer
- Year
- 1977
- Tongue
- English
- Weight
- 855 KB
- Volume
- 51
- Category
- Article
- ISSN
- 0038-0938
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