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
A new approximation of relaxed energies for harmonic maps and the Faddeev model
β Scribed by Mariano Giaquinta; Min-Chun Hong; Hao Yin
- Publisher
- Springer
- Year
- 2010
- Tongue
- English
- Weight
- 291 KB
- Volume
- 41
- Category
- Article
- ISSN
- 0944-2669
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