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• W1968299635 abstract "The global configuration and topology of the terrestrial magnetosphere for typical IMF conditions is simulated with a new 3D MHD model using adaptive mesh refinement (AMR). The paper briefly describes the main elements of the solution method and presents a steady-state solution for nominal Parker-spiral IMF conditions. The simulated magnetic field topology in the magnetotail is in excellent agreement with the recent empirical model derived from four years of IMP 8 observations (Kaymaz and Siscoe, 1998)." @default.
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• W1968299635 date "2000-01-01" @default.
• W1968299635 modified "2023-10-15" @default.
• W1968299635 title "Magnetospheric configuration for Parker-spiral IMF conditions: Results of a 3D AMR MHD simulation" @default.
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• W1968299635 doi "https://doi.org/10.1016/s0273-1177(99)01040-6" @default.
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