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Cooling of solar flare plasmas

โœ Scribed by W. T. Zaumen; L. W. Acton


Publisher
Springer
Year
1974
Tongue
English
Weight
289 KB
Volume
36
Category
Article
ISSN
0038-0938

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๐Ÿ“œ SIMILAR VOLUMES


The cooling of flare produced plasmas in
โœ J. L. Culhane; J. F. Vesecky; K. J. H. Phillips ๐Ÿ“‚ Article ๐Ÿ“… 1970 ๐Ÿ› Springer ๐ŸŒ English โš– 1021 KB

Solar flare X-rays, at energies less than 10 keV, are emitted by hot plasmas located in the corona. Three plasma cooling models are examined in detail. The cooling of the electrons by Coulomb collisions with ions at a lower temperature would require the observed material to occupy very large volumes

Heat flux saturation in hydrodynamic sof
โœ I. J. D. Craig; J. W. Davys ๐Ÿ“‚ Article ๐Ÿ“… 1984 ๐Ÿ› Springer ๐ŸŒ English โš– 699 KB

The role of heat flux limitation in soft X-ray emitting solar flare plasmas is considered. Simple analytic arguments suggest that flux limitation is likely to be important during the explosive heating phase, even for relatively modest coronal energy fluxes (say < 109 erg cm-2 s -1). This conclusion