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The book covers intimately all the topics necessary for the
development of a robust magnetohydrodynamic (MHD) code within the
framework of the cell-centered finite volume method (FVM) and its
applications in space weather study. First, it presents a brief
review of existing MHD models in studying solar corona and the
heliosphere. Then it introduces the cell-centered FVM in
three-dimensional computational domain. Finally, the book presents
some applications of FVM to the MHD codes on spherical coordinates
in various research fields of space weather, focusing on the
development of the 3D Solar-InterPlanetary space-time Conservation
Element and Solution Element (SIP-CESE) MHD model and its
applications to space weather studies in various aspects. The book
is written for senior undergraduates, graduate students, lecturers,
engineers and researchers in solar-terrestrial physics, space
weather theory, modeling, and prediction, computational fluid
dynamics, and MHD simulations. It helps readers to fully understand
and implement a robust and versatile MHD code based on the
cell-centered FVM.
The book covers intimately all the topics necessary for the
development of a robust magnetohydrodynamic (MHD) code within the
framework of the cell-centered finite volume method (FVM) and its
applications in space weather study. First, it presents a brief
review of existing MHD models in studying solar corona and the
heliosphere. Then it introduces the cell-centered FVM in
three-dimensional computational domain. Finally, the book presents
some applications of FVM to the MHD codes on spherical coordinates
in various research fields of space weather, focusing on the
development of the 3D Solar-InterPlanetary space-time Conservation
Element and Solution Element (SIP-CESE) MHD model and its
applications to space weather studies in various aspects. The book
is written for senior undergraduates, graduate students, lecturers,
engineers and researchers in solar-terrestrial physics, space
weather theory, modeling, and prediction, computational fluid
dynamics, and MHD simulations. It helps readers to fully understand
and implement a robust and versatile MHD code based on the
cell-centered FVM.
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