𝔖 Bobbio Scriptorium
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Heat transfer in solar flares

✍ Scribed by B. V. Somov


Publisher
Springer
Year
1978
Tongue
English
Weight
327 KB
Volume
60
Category
Article
ISSN
0038-0938

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✦ Synopsis


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.


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