ИСТИНА

To use the universal approach to modelling of the planetary magnetosphere we analyzed the global current systems which control magnetic field inside the magnetosphere. Usually these current systems included the magnetopause and tail currents but for rotate dominated magnetospheres of the Jupiter and Saturn we are needed to add the equatorial disk current. The magnetospheric structure can be fixed by a small number of the parameters. These parameters are determined by the planetary dipole, by the planetary rotation, by the solar wind pressure, by the mass loading of the satellite plasma, and by the interplanetary magnetic field