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Energy Transfer to and Through Ionospheric Electrons

  • N. P. Carleton
Conference paper
  • 156 Downloads
Part of the Astrophysics and Space Science Library book series (ASSL, volume 10)

Abstract

Energy can be transferred through the ionospheric electrons in essentially three ways :
  1. (1)

    the degradation of fast electrons (photoelectrons or precipitated particles),

     
  2. (2)

    the flow of electric currents,

     
  3. (3)

    thermal conduction.

     

I wish to deal here with two problems, one in each of the first two categories.

Keywords

Fast Electron Maxwellian Distribution Hall Current Collision Term Excitation Rate 
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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References

  1. Dalgarno, A., McElroy, M. B. and Moffett, R. J.: 1963, Planet. Space Sci. 11, 463–484.ADSCrossRefGoogle Scholar
  2. Dalgarno, A., McElroy, M. B. and Walker, J. C.: 1967, Planet. Space Sci. 15, 331–345.ADSCrossRefGoogle Scholar
  3. Hoegy, W. F., Fournier, J. P., and Fontheim, E. G.: 1965, J. Geophys. Res. 70, 5464–5468.ADSCrossRefGoogle Scholar
  4. Rishbeth, H., Megill, L. R. and Cahn, J. H.: 1965, Ann. Géophys. 21, 235–244.Google Scholar

Copyright information

© D. Reidel Publishing Company, Dordrecht, Holland 1968

Authors and Affiliations

  • N. P. Carleton
    • 1
  1. 1.Smithsonian Astrophysical Observatory and Harvard UniversityUSA

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