A new model is presented for the distribution of solar (and stellar) flare energies. Flares are assumed to result from energy release in multiple reconnecting current sheets (RCSs) in the solar corona. The model takes into account both the dynamical evolution of separate RCSs and their interaction b
β¦ LIBER β¦
A Reconnection Model for the Distribution of Flare Energies
β Scribed by I.J.D. Craig
- Book ID
- 110304542
- Publisher
- Springer
- Year
- 2001
- Tongue
- English
- Weight
- 62 KB
- Volume
- 202
- Category
- Article
- ISSN
- 0038-0938
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