Time variations of the hard X-ray spectrum in solar flares are observed by the hard X-ray spectrometer (HXM) aboard the Hinotori satellite. With a new presentation of the dynamic spectrum we have studied the differences between impulsive and gradual hard X-ray bursts. In the impulsive events a "bent
โฆ LIBER โฆ
Computed magnetic field structure of the flares observed by Hinotori hard X-ray telescope
โ Scribed by Takashi Sakurai
- Publisher
- Springer
- Year
- 1983
- Tongue
- English
- Weight
- 306 KB
- Volume
- 86
- Category
- Article
- ISSN
- 0038-0938
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