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Astrophysics and Space Science

, Volume 123, Issue 2, pp 403–404 | Cite as

Comments on the heating of solar active regions by magnetic energy dissipation

  • Suresh Chandra
Article
  • 24 Downloads

Abstract

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.

Keywords

Magnetic Field Active Region Energy Dissipation Magnetic Energy Solar Active Region 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Reference

  1. Kumar, M. and Narain, U.: 1985,Solar Phys. 95, 69.Google Scholar

Copyright information

© D. Reidel Publishing Company 1986

Authors and Affiliations

  • Suresh Chandra
    • 1
  1. 1.Department of PhysicsUniversity of GorakhpurIndia

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