Common features in the development of powerful long-duration solar X-ray flares
โ Scribed by M. A. Livshits; O. G. Badalyan; A. V. Belov
- Book ID
- 110131815
- Publisher
- Springer
- Year
- 2002
- Tongue
- English
- Weight
- 362 KB
- Volume
- 46
- Category
- Article
- ISSN
- 1063-7729
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We define the ~p~iUs phgL6s of a flare as its first phase, characterized by: X-ray bursts of short (seconds to tens of seconds) duration, a patchy X-ray morphology, and injection of energy. It lasts some five to ten minutes. The g~d~cg~ or ~s phase starts virtually at the same time as the impulsive
The problem of producing the hard X-ray burst at the onset of solar flares may be thought of in terms of the problem of producing the non-thermal electrons which emit the X-rays via bremsstrahlung. Electron acceleration to relativistic energies without similar ion acceleration is difficult to achiev