Advertisement

Springer Nature is making SARS-CoV-2 and COVID-19 research free. View research | View latest news | Sign up for updates

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

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.

This is a preview of subscription content, log in to check access.

Reference

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

Download references

Author information

Rights and permissions

Reprints and Permissions

About this article

Cite this article

Chandra, S. Comments on the heating of solar active regions by magnetic energy dissipation. Astrophys Space Sci 123, 403–404 (1986). https://doi.org/10.1007/BF00653960

Download citation

Keywords

  • Magnetic Field
  • Active Region
  • Energy Dissipation
  • Magnetic Energy
  • Solar Active Region