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Solar and Stellar Magnetic Fields and Atmospheric Structures: Theory

  • E. N. Parker

Abstract

This presentation reviews selected ideas on the origin of the magnetic field of the Sun, the dynamical behavior of the azimuthal field in the convective zone, the fibril state of the field at the photosphere, the formation of sunspots, prominences, the spontaneous formation of current sheets in the bipolar field above the surface of the Sun, coronal heating, and flares.

Keywords

Current Sheet Solar Phys Solar Flare Convective Zone Tangential Discontinuity 
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 1989

Authors and Affiliations

  • E. N. Parker
    • 1
  1. 1.Enrico Fermi Institute, Depts. Physics and AstronomyUniversity of ChicagoChicagoUSA

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