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Magnetoacoustic Heating of the Solar Chromosphere

  • S. M. Chitre
  • Joseph M. Davila

Abstract

In the present work we wish to examine the viability of the acoustic waves generated in the solar convection zone propagating radially outward through the overlying atmosphere and getting resonantly absorbed by the magnetic arches of the low-lying chromospheric canopy. We demonstrate that the resultant Poynting and acoustic flux that enters the magnetic canopy in the network regions is adequate to explain the energy losses from the chromospheric layer of the sun.

Keywords

Acoustic Wave Solar Convection Zone Horizontal Magnetic Field Solar Chromosphere Overlie Atmosphere 
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.

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Copyright information

© Springer-Verlag Berlin Heidelberg 1991

Authors and Affiliations

  • S. M. Chitre
    • 1
  • Joseph M. Davila
    • 2
  1. 1.Tata Institute of Fundamental ResearchColaba BombayIndia
  2. 2.NASA Goddard Space Flight CenterGreenbeltUSA

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