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Magnetohydrodynamic Modeling of the Solar Corona and Heliosphere

Record Type:	Language materials, printed : Monograph/item
Title/Author:	Magnetohydrodynamic Modeling of the Solar Corona and Heliosphere/ by Xueshang Feng.
Author:	Feng, Xueshang.
Description:	XIX, 772 p. 199 illus., 141 illus. in color.online resource. :
Contained By:	Springer Nature eBook
Subject:	Solar system. -
Online resource:	https://doi.org/10.1007/978-981-13-9081-4
ISBN:	9789811390814

Magnetohydrodynamic Modeling of the Solar Corona and Heliosphere
Feng, Xueshang.

Magnetohydrodynamic Modeling of the Solar Corona and Heliosphere[electronic resource] /by Xueshang Feng. - 1st ed. 2020. - XIX, 772 p. 199 illus., 141 illus. in color.online resource. - Atmosphere, Earth, Ocean & Space,2524-440X. - Atmosphere, Earth, Ocean & Space,.

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.

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. .

ISBN: 9789811390814

Standard No.: 10.1007/978-981-13-9081-4doiSubjects--Topical Terms:

897437
Solar system.

LC Class. No.: QB500.5-785

Dewey Class. No.: 523.2

Magnetohydrodynamic Modeling of the Solar Corona and Heliosphere
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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. .
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