Effects of x-ray hardness on fluorogram informativeness
โ Scribed by G. A. Chuiko; V. M. Tsvetkov
- Publisher
- Springer US
- Year
- 1982
- Tongue
- English
- Weight
- 195 KB
- Volume
- 16
- Category
- Article
- ISSN
- 0006-3398
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
A number of solar X-ray events above 10 keV and 20 keV were compiled in order to test for evidence of anisotropic emission. The results are not definite, although the two samples show apparently different behaviours. Among the mechanism of X-ray emission from solar bursts and of related phenomena,
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