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         Title:  Modeling of the Jovian magnetosphere 
        Author(s):  E.S. Belenkaya (Oral)
         ABSTRACT 
        A paraboloid model of the Jovian magnetosphere is presented. The
        magnetopause is approximated by a paraboloid of revolution.
        Magnetospheric magnetic field consists of a planet dipole field, a
        magnetodisc field, a magnetotail current sheet field and a partially
        penetrating interplanetary magnetic field. All magnetospheric magnetic
        fields are screened by the magnetopause currents. The purpose of this
        paper is to discuss a possibility to compare the Jovian magnetospheric
        electric fields and plasma motions caused by the unipolar inductor and
        the solar wind MHD generator. this is one of the approaches to the
        fundumental question regarding the nature of the global plasma
        convection and corotation in the  Jupiter's magnetosphere.
        
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