Radiative cooling and heat conduction determine the temperature structure of flare plasmas along magnetic field. It is shown that both in the case of slow heating and of impulsive heating, temperatures are distributed in such a way that classical collisional heat conduction is valid.
โฆ LIBER โฆ
Heat transfer in solar-bioclimatic houses
โ Scribed by E. Bilgen; P. Vasseur
- Publisher
- Elsevier Science
- Year
- 1994
- Tongue
- English
- Weight
- 390 KB
- Volume
- 5
- Category
- Article
- ISSN
- 0960-1481
No coin nor oath required. For personal study only.
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