The determination of the location of the region of origin of hard X-rays is important in evaluating the importance of 10-100 keV electrons in solar flares arm in understanding flare particle acceleration. At present only limb-occulted events are available to give some information on the height of X-
The inter-relationship of hard X-ray and EUV bursts during solar flares
โ Scribed by A. Gordon Emslie; John C. Brown; Richard F. Donnelly
- Publisher
- Springer
- Year
- 1978
- Tongue
- English
- Weight
- 708 KB
- Volume
- 57
- Category
- Article
- ISSN
- 0038-0938
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