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Energy Transfer to and Through Ionospheric Electrons

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Part of the book series: Astrophysics and Space Science Library ((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.

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References

  • Dalgarno, A., McElroy, M. B. and Moffett, R. J.: 1963, Planet. Space Sci. 11, 463–484.

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  • Hoegy, W. F., Fournier, J. P., and Fontheim, E. G.: 1965, J. Geophys. Res. 70, 5464–5468.

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  • Rishbeth, H., Megill, L. R. and Cahn, J. H.: 1965, Ann. Géophys. 21, 235–244.

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© 1968 D. Reidel Publishing Company, Dordrecht, Holland

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Carleton, N.P. (1968). Energy Transfer to and Through Ionospheric Electrons. In: Carovillano, R.L., McClay, J.F., Radoski, H.R. (eds) Physics of the Magnetosphere. Astrophysics and Space Science Library, vol 10. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3467-8_18

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  • DOI: https://doi.org/10.1007/978-94-010-3467-8_18

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-3469-2

  • Online ISBN: 978-94-010-3467-8

  • eBook Packages: Springer Book Archive

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