Comments on the heating of solar active regions by magnetic energy dissipation
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The method of Kumar and Narain (1985) to calculate the twisting velocity of magnetic field appears to be erroneous. Hence, their conclusion about Tucker's proposal for the heating of active regions by magnetic energy dissipation may not be correct.
KeywordsMagnetic Field Active Region Energy Dissipation Magnetic Energy Solar Active Region
- Kumar, M. and Narain, U.: 1985,Solar Phys. 95, 69.Google Scholar
© D. Reidel Publishing Company 1986