A three-dimensional, multispecies, comprehensive MHD model of the solar wind interaction with the planet Venus
作者： N. Terada , H. Shinagawa , T. Tanaka , K. Murawski , K. Terada
DOI: 10.1029/2008JA013937
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摘要: [1] We present our newly developed numerical model of the solar wind interaction with planet Venus. The solves three-dimensional, 10-ion-species magnetohydrodynamic (MHD) equations using a total variation diminishing monotonic upstream scheme for conservation laws, which is implemented on an unstructured grid system. These describe dynamics both and planetary ionosphere. An excellent performance verified by comparing results existing observational data. In particular, profiles magnetic field, number densities, velocity, transterminator flux ionospheric plasma are shown to reproduce findings. A main goal this paper its general structures ionosphere
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