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Return current losses in pulse beam heating of the solar atmosphere

✍ Scribed by Marian Karlický; Jean-Claude Hénoux


Publisher
Elsevier Science
Year
1993
Tongue
English
Weight
290 KB
Volume
13
Category
Article
ISSN
0273-1177

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An elementary analysis based on Amp6re's Law is given to separate the general magnetic field above the photosphere into two parts B = BI + B\*. The field B1 is a potential field due to electric currents below the photosphere. The field B\* is produced by electric currents above the photosphere combi