Modeling of the planetary structure of the ionosphere and the protonosphere coupling

descriptionPublicationkeyboard_double_arrow_right Article , Part of book or chapter of book 01 Jan 1988 English Publisher:Springer Science and Business Media LLCJournal:pure and applied geophysics, volume 127, pages 335-352 (issn: 0033-4553, eissn: 1420-9136,

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Authors: Yu. S. Saenko; N. S. Natsvalyan; N. Yu. Tepenitsyna;

doi: 10.1007/bf00879816 , 10.1007/978-3-0348-6532-6_7

Modeling of the planetary structure of the ionosphere and the protonosphere coupling

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Abstract

A planetary model of the ionosphere and the protonosphere coupling is described. The system of three-dimensional nonstationary modeling equations of continuity and motion for the ions O+ and H+ is presented. Some numerical results of model calculations are compared with the experimental data. The important role of electromagnetic drifts in the formation of large-scale morphological peculiarities of the ionosphere and the protonosphere coupling is shown.

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