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  • Xueshang Feng
    978-981-13-9081-4
    2020
    Edition 1
    • Provides a brief review of existing magnetohydrodynamic (MHD) models in studying solar corona and the helioshpere
    • Covers all the topics necessary to develop a robust MHD code based on the finite volume method (FVM)
    • Presents applications of the 3D Solar-InterPlanetary space-time Conservation Element and Solution Element (SIP-CESE) MHD model
    • Compares the modeled results with different observations

    €260

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