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
โฆ LIBER โฆ
Cooling of solar flare plasmas
โ 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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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