Highlights Analytical representation of the ionospheric electric field distribution continuously evolving with the solar wind parameters. Effects of the convection electric field as a driver of high-latitude ionospheric structure are modeled. Main large-scale irregularities are reproduced.

    Abstract The numerical model predicts the 3-D distribution of electron density over the high-latitude F region ionosphere in the altitudes between 130 and 600km. The distinctive feature of the model is an analytical representation of the electric potential distribution over the high-latitude ionospheric shell which continuously evolving with the solar wind parameters, season and universal time. In this approach the convection electric field is directly related to the field-aligned currents of magnetospheric origin which are controlled by the solar wind. The time-dependent ion continuity and momentum equations are solved as a function of altitude within a convecting and corotating plasma flux tube. Modeling results show that the polar ionosphere F region responds strongly to the change in the IMF polarity and the solar zenith angle. Large-scale ionospheric irregularities are reproduced in details.


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    Titel :

    Numerical modeling of the polar F region ionosphere taking into account the solar wind conditions


    Beteiligte:
    Uvarov, V.M. (Autor:in) / Lukianova, R.Yu. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 56 , 11 ; 2563-2574


    Erscheinungsdatum :

    2015-10-01


    Format / Umfang :

    12 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch





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