The role of heat flux limitation in soft X-ray emitting solar flare plasmas is considered. Simple analytic arguments suggest that flux limitation is likely to be important during the explosive heating phase, even for relatively modest coronal energy fluxes (say < 109 erg cm-2 s -1). This conclusion
Effects of soft x-ray flux on the lower solar atmosphere in flares
โ Scribed by J. C. Henoux; Y. Nakagawa
- Publisher
- Springer
- Year
- 1977
- Tongue
- English
- Weight
- 99 KB
- Volume
- 53
- Category
- Article
- ISSN
- 0038-0938
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