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Magnetohydrodynamic modeling of the ...

Feng, Xueshang.

Magnetohydrodynamic modeling of the solar corona and heliosphere

Record Type:	Electronic resources : Monograph/item
Title/Author:	Magnetohydrodynamic modeling of the solar corona and heliosphereby Xueshang Feng.
Author:	Feng, Xueshang.
Published:	Singapore :Springer Singapore :2020.
Description:	xix, 772 p. :ill. (some col.), digital ;24 cm.
Contained By:	Springer eBooks
Subject:	Magnetohydrodynamics.
Subject:	SunCorona.
Online resource:	https://doi.org/10.1007/978-981-13-9081-4
ISBN:	9789811390814$q(electronic bk.)

Magnetohydrodynamic modeling of the solar corona and heliosphere
Feng, Xueshang.

Magnetohydrodynamic modeling of the solar corona and heliosphere[electronic resource] /by Xueshang Feng. - Singapore :Springer Singapore :2020. - xix, 772 p. :ill. (some col.), digital ;24 cm. - 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$q(electronic bk.)

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

207822
Magnetohydrodynamics.
Subjects--Geographical Terms:

451681
Sun
--Corona.

LC Class. No.: QB529 / .F46 2020

Dewey Class. No.: 523.75

Magnetohydrodynamic modeling of the solar corona and heliosphere
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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.
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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