Physics
Scientist
Institute of Computational Modelling, Russian Academy of Sciences, 660036 Krasnoyarsk 36, Russia
Institute of Computational Modeling of Russian Academy of Sciences, Krasnoyarsk, Russia
A slow mode transition region adjoining the front boundary of a magnetic cloud as a relic of a convected solar wind feature: Observations and MHD simulation
Electric potential difference due to MHD slow shocks propagating along the Io flux tube
Propagation of nonlinear slow waves produced by pressure pulses along the Io flux tube
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