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
The solar albedo of hard X-ray flares
โ Scribed by N. Santangelo; H. Horstman; E. Horstman-Moretti
- Publisher
- Springer
- Year
- 1973
- Tongue
- English
- Weight
- 240 KB
- Volume
- 29
- Category
- Article
- ISSN
- 0038-0938
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