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Kαx-ray emission characterization of 100

✍ Scribed by S. Fourmaux; C. Serbanescu; R. E. Kincaid; A. Krol; J. C. Kieffer


Publisher
Springer
Year
2008
Tongue
English
Weight
494 KB
Volume
94
Category
Article
ISSN
0721-7269

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Kct X-ray line emission from S, Ar, Ca and Fe is calculated for conditions likely to exist in solar flares. We consider both the non-thermal and thermal phases of flares as indicated by X-ray observations. Impulsive non-thermal events seen at the onset of a flare at photon energies > 20 keV generall