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Saturn ionosphere: theoretical interpretation

Nature volume 292, pages 682–683 (1981)Cite this article

Abstract

Voyager 1 high latitude and Pioneer 11 equatorial ionospheric structure indicate a solar EUV-controlled ionosphere with a possible molecular ion in the topside. Vibrationally excited H2 in the high latitudes may be an important loss mechanism. Dynamical effects are expected to be important for determining the peak density and its location.

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Authors and Affiliations

  1. Department of Atmospheric and Oceanic Science, Space Physics Research Laboratory, The University of Michigan, Ann Arbor, Michigan, 48109, USA

    S. K. Atreya

  2. Marshall Space Flight Center, Huntsville, Alabama, 35812, USA

    J. H. Waite Jr

Authors
  1. S. K. Atreya
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  2. J. H. Waite Jr
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Atreya, S., Waite, J. Saturn ionosphere: theoretical interpretation. Nature 292, 682–683 (1981). https://doi.org/10.1038/292682a0

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