Hαemission line profiles of solar flares with turbulent velocity fields
✍ Scribed by M. D. Ding; C. Fang
- Publisher
- Springer
- Year
- 1993
- Tongue
- English
- Weight
- 851 KB
- Volume
- 147
- Category
- Article
- ISSN
- 0038-0938
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📜 SIMILAR VOLUMES
We observed in He the impulsive phase of a 1N/M2.0 limb flare on September 8, 1988 with high temporal resolution. With an imaging spectrograph line profiles have been acquired every 2.3 s. The temporal evolution in the blue and red wing has been correlated with hard X-ray data from HXRB S. It is sho
During 1967During -1970 , the greatness of ~ 90 large flares (Ha importance > 2) was influenced by the orientation of the large-scale (~ 100000 km) magnetic field structure over the flare site. Although the average X-ray and optical emissions are only slightly larger for flares with their overlying