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Models of Solar-type Coronae

  • T. W. Hartquist
  • R. Rosner
Part of the Astrophysics and Space Science Library book series (ASSL, volume 143)

Abstract

Simple models for the thermal and ionization structures of ‘closed’ stellar coronal structures (loops) are described, for which the heating rates are specified a priori. We discuss thermal and MHD instabilities of such structures, as well as possible heating mechanisms which have been considered.

Keywords

Current Sheet Flux Tube Coronal Loop Alfven Wave Coronal Heating 
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

© Kluwer Academic Publishers 1988

Authors and Affiliations

  • T. W. Hartquist
    • 1
  • R. Rosner
    • 2
    • 3
  1. 1.Max Planck Institute for Physics and AstrophysicsInstitute for Extraterrestrial PhysicsGarchingGermany
  2. 2.Enrico Fermi Institute and Department of Astronomy and AstrophysicsThe University of ChicagoChicagoUSA
  3. 3.Harvard-Smithsonian Center for AstrophysicsCambridgeUSA

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