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Auroral Heating

  • Alv Egeland
Part of the Space Science Library book series (ASSL, volume 51)

Abstract

Today we can explain and predict fairly accurately several of the regular, global-scale variations in the upper atmosphere, while existing models fail to reproduce rapid structural changes which occur more or less continuously in the high latitude ionosphere. Particularly in the auroral E region, there is a wide gap between our present theoretical understanding of the physics and the experimental data.

Keywords

Solar Wind Joule Heating Hall Conductivity Auroral Electrojet Geomagnetic Field Line 
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

© D. Reidel Publishing Company, Dordrecht, Holland 1975

Authors and Affiliations

  • Alv Egeland
    • 1
  1. 1.The Norwegian Institute of Cosmic PhysicsBlindern, Oslo 3Norway

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