Longitudinal distribution of the hard X-ray bursts on the Sun
โ Scribed by V. K. Verma; M. C. Pande
- Publisher
- Springer
- Year
- 1985
- Tongue
- English
- Weight
- 232 KB
- Volume
- 99
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
The analysis of 315 hard X-ray bursts (HXR) producing solar flares observed by Hinotori satellite shows that the HXR bursts occur most prominently at 110 ~ 140~ 290 ~ and 320 ~ longitude, respectively. These longitudes are not only prolific in producing flares in number but also in producing flares with large photon counts.
๐ SIMILAR VOLUMES
The primary scientific objectives of the Hard X-Ray Burst Spectrometer (HXRBS) to be flown on the Solar Maximum Mission are as follows: (1) To determine the nature of the mechanisms which accelerate electrons to 20-100 keV in the first stage of a solar flare and to > 1 MeV in the second stage of man
The height distribution of hard X-ray bremsstrahlung is predicted for dissipative thermal models, involving rapid heating of many small (tearing mode) islands near the top of a magnetic arch. Emission at low energies (e) originates mainly at high altitudes in the heated kernels themselves while high