Anisotropy and polarization of solar X-ray bursts
β 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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π SIMILAR VOLUMES
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
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