A parametric model for the efficiency of a flare in crosswind
โ Scribed by M.R. Johnson; L.W. Kostiuk
- Book ID
- 104443086
- Publisher
- Elsevier Science
- Year
- 2002
- Tongue
- English
- Weight
- 145 KB
- Volume
- 29
- Category
- Article
- ISSN
- 1540-7489
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
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
The energetics and mass transfer during the X-ray flare of 18:31 GMT on 5 September, 1973 have been studied using the observations in the objective grating mode of the AS&E X-ray spectrographic telescope on Skylab. The flare was a moderately energetic one, Class M1 according to Solrad. In Ha, howeve