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On application of asymmetric Kan-like exact equilibria to the Earth magnetotail modeling 10-15 RE at high levels of magnetospheric activity. The essential model parameters (current sheet

Two-Dimensional Model of the Global Ionospheric ConductorTo numerically simulate large-scale electric fields in the magnetosphere and ionosphere

Features of the Electromagnetic and Plasma Disturbances Induced at the Altitudes of the Earth’s Outer Ionosphere by Modification of the Ionospheric F 2 Region Using High-Power Radio Waves Radiated by the SURA Heating Facility on the ionosphere–magnetosphere coupling and propagation of radio waves of various frequency ranges are demonstrated

Evidence for the radiation-pressure dominated accretion disk in bursting pulsar GRO J1744-28 using timing analysis-II X-ray bursts, allowing studies of the interaction of the accretion disk with the magnetosphere

Large-Scale Disturbances Features Induced in the Ionosphere by Powerful Decameter Radiation during Moderate Magnetic Storms are found. The role of magnetic activity in the Earth–atmosphere–ionosphere–magnetosphere system, which

Dynamics of Solitons of the Generalized Nonlinear Schrödinger Equation in an Inhomogeneous and Nonstationary Medium: Evolution and Interaction and magnetospheric plasma and in many other areas of physics.

European Space Agency SMILE and Czech participation© 2020 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim SMILE (Solar wind Magnetosphere Ionosphere Link

ИЗМЕНЧИВОСТЬ УСЛОВИЙ РАСПРОСТРАНЕНИЯ КВ РАДИОВОЛН НА ТРАССАХ ВОСТОЧНОЙ СИБИРИ В ИЮНЕ 2015 Г.. The contribution of solar cosmic rays, the amplifications of the magnetospheric convection and the thermospheric

Aperiodic optical variability of intermediate polars-cataclysmic variables with truncated accretion disks at the boundary of the white dwarfs' magnetospheres. We propose that the properties of the optical power spectra

Dynamics of Solitons of the Generalized Nonlinear Schrödinger Equation in an Inhomogeneous and Nonstationary Medium: Evolution and Interaction and magnetospheric plasma and in many other areas of physics.

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