This investigation shows that statistically there are significant time delays between Ha and hard X-ray (HXR) emissions during solar flares; most impulsive flares produce HXR emissions up to ~ 1 min before and up to 2 min after the onset of Hc~ emission. HXR emissions are also found to be peaked up
Relationship between impulsive and post-eruptive processes in solar X-ray flares
โ Scribed by M. A. Livshits; O. G. Badalyan
- Book ID
- 110140666
- Publisher
- Springer
- Year
- 2004
- Tongue
- English
- Weight
- 446 KB
- Volume
- 48
- Category
- Article
- ISSN
- 1063-7729
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