The dynamics of hard X-ray producing electron beams in solar flares can be strongly affected by the occurrence of a reverse current. The parameter diagram for a beam can be divided into three regimes, one of which is the usual thick target case, the two others being due to two different possible con
✦ LIBER ✦
Relative Timing and Spectra of Solar Flare Hard X-ray Sources
✍ Scribed by Säm Krucker; R.P. Lin
- Book ID
- 110420435
- Publisher
- Springer
- Year
- 2002
- Tongue
- English
- Weight
- 601 KB
- Volume
- 210
- Category
- Article
- ISSN
- 0038-0938
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