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Anisotropy and polarization of solar X-ray bursts

✍ Scribed by J. C. Henoux


Publisher
Springer
Year
1975
Tongue
English
Weight
641 KB
Volume
42
Category
Article
ISSN
0038-0938

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πŸ“œ SIMILAR VOLUMES


Note on solar hard X-ray bursts
✍ C. Jager πŸ“‚ Article πŸ“… 1967 πŸ› Springer 🌐 English βš– 193 KB

Observationally solar X bursts fall into three different categories: soft X bursts (E ,< I 0 keV), deka-keV bursts (10-150 keV), and very hard X bursts or deci-MeV bursts (200-1000 keV). The first kind is quasi-thermal, the last kind is non-thermal. The real existence of the third kind of burst look

Theory of deka-keV solar X-ray bursts
✍ R. Snijders πŸ“‚ Article πŸ“… 1968 πŸ› Springer 🌐 English βš– 573 KB

In this paper an attempt has been made to investigate theoretically the time-profile of an X-ray burst observed at photon energies well below 0.5 MeV. Following DE JAGER (1967) this type of X-bursts is called deka-keV X-ray bursts. The energy distribution of fast electrons which emit the hard X-ray