๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Hard X-ray imaging of a solar gradual hard X-ray burst on April 1, 1981

โœ Scribed by T. Takakura; K. Ohki; T. Sakurai; J. L. Wang; J. Y. Xuan; S. C. Li; R. Y. Zhao

Publisher
Springer
Year
1984
Tongue
English
Weight
969 KB
Volume
94
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

Note on solar hard X-ray bursts
Note on solar hard X-ray bursts
โœ C. Jager ๐Ÿ“‚ Article ๐Ÿ“… 1967 ๐Ÿ› Springer ๐ŸŒ English โš– 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

Hard X-ray images of impulsive bursts
Hard X-ray images of impulsive bursts
โœ T. Takakura; K. Ohki; S. Tsuneta; N. Nitta ๐Ÿ“‚ Article ๐Ÿ“… 1983 ๐Ÿ› Springer ๐ŸŒ English โš– 544 KB

A morphological study is made for the hard X-ray images (25-50 keV) of nine impulsive bursts observed by Hinotori. Most of them revealed single sources, either extended or compact, during the whole duration of the bursts. The sources of all of four spike bursts in the present sample are compact. Aft