๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Common features in the development of powerful long-duration solar X-ray flares

โœ 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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๐Ÿ“œ SIMILAR VOLUMES


Development of flare morphology in X-ray
โœ C. Jager ๐Ÿ“‚ Article ๐Ÿ“… 1983 ๐Ÿ› Springer ๐ŸŒ English โš– 580 KB

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

On the production of hard X-rays in sola
โœ G. M. Simnett; M. G. Haines ๐Ÿ“‚ Article ๐Ÿ“… 1990 ๐Ÿ› Springer ๐ŸŒ English โš– 613 KB

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