Magnetohydrodynamic Modeling of the Solar Corona and Heliosphere

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 so...

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Bibliographic Details
Main Author: Feng, Xueshang
Format: eBook
Language:English
Published: Singapore Springer Nature Singapore 2020, 2020
Edition:1st ed. 2020
Series:Atmosphere, Earth, Ocean & Space
Subjects:
Sun
Online Access:
Collection: Springer eBooks 2005- - Collection details see MPG.ReNa
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245 0 0 |a Magnetohydrodynamic Modeling of the Solar Corona and Heliosphere  |h Elektronische Ressource  |c by Xueshang Feng 
250 |a 1st ed. 2020 
260 |a Singapore  |b Springer Nature Singapore  |c 2020, 2020 
300 |a XIX, 772 p. 199 illus., 141 illus. in color  |b online resource 
505 0 |a Current status of MHD simulations for space weather -- Finite Volume Methods -- A Finite Volume MHD Code in Spherical Coordinates for Background solar Wind -- 3D SIP-CESE MHD Model on Triangular Prism Grids -- 3D SIP-CESE MHD Model on Six-component Overset Grid System -- AMR Implementation of 3D SIP-CESE MHD Model on Six-component Overset Grid System -- Data-Driven Modeling of Solar Wind -- Coronal Force-Free Field Extrapolations -- Data-Driven MHD Modeling of Coronal Magnetic Evolutions and Eruptions -- Numerical Study of Coronal Mass Ejections -- Future Avenue 
653 |a Complex Systems 
653 |a Sun 
653 |a Computer simulation 
653 |a Computer Modelling 
653 |a System theory 
653 |a Mathematical physics 
653 |a Solar Physics 
653 |a Theoretical, Mathematical and Computational Physics 
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989 |b Springer  |a Springer eBooks 2005- 
490 0 |a Atmosphere, Earth, Ocean & Space 
856 4 0 |u https://doi.org/10.1007/978-981-13-9081-4?nosfx=y  |x Verlag  |3 Volltext 
082 0 |a 523.7 
520 |a 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.