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000922406 019__ $$a1117303840$$a1117706210
000922406 020__ $$a9789811390814$$q(electronic book)
000922406 020__ $$a9811390819$$q(electronic book)
000922406 020__ $$z9789811390807
000922406 0247_ $$a10.1007/978-981-13-9081-4$$2doi
000922406 0247_ $$a10.1007/978-981-13-9
000922406 035__ $$aSP(OCoLC)on1114331883
000922406 035__ $$aSP(OCoLC)1114331883$$z(OCoLC)1117303840$$z(OCoLC)1117706210
000922406 040__ $$aGW5XE$$beng$$erda$$epn$$cGW5XE$$dLQU$$dUKMGB$$dOCLCF
000922406 049__ $$aISEA
000922406 050_4 $$aQB529$$b.F46 2020eb
000922406 08204 $$a523.7/5$$223
000922406 1001_ $$aFeng, Xueshang,$$eauthor.
000922406 24510 $$aMagnetohydrodynamic modeling of the solar corona and heliosphere /$$cXueshang Feng.
000922406 264_1 $$aSingapore :$$bSpringer,$$c[2020]
000922406 264_4 $$c©2020
000922406 300__ $$a1 online resource :$$billustrations.
000922406 336__ $$atext$$btxt$$2rdacontent
000922406 337__ $$acomputer$$bc$$2rdamedia
000922406 338__ $$aonline resource$$bcr$$2rdacarrier
000922406 4901_ $$aAtmosphere, earth, ocean & space,$$x2524-440X
000922406 504__ $$aIncludes bibliographical references.
000922406 5050_ $$aCurrent 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.
000922406 506__ $$aAccess limited to authorized users.
000922406 520__ $$aThe 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.
000922406 588__ $$aOnline resource; title from PDF title page (SpringerLink, viewed August 29, 2019).
000922406 650_0 $$aMagnetohydrodynamics.
000922406 650_0 $$aHeliosphere (Astrophysics)
000922406 650_0 $$aSpace environment.
000922406 651_0 $$aSun$$xCorona.
000922406 830_0 $$aAtmosphere, earth, ocean & space.
000922406 852__ $$bebk
000922406 85640 $$3SpringerLink$$uhttps://univsouthin.idm.oclc.org/login?url=http://link.springer.com/10.1007/978-981-13-9081-4$$zOnline Access$$91397441.1
000922406 909CO $$ooai:library.usi.edu:922406$$pGLOBAL_SET
000922406 980__ $$aEBOOK
000922406 980__ $$aBIB
000922406 982__ $$aEbook
000922406 983__ $$aOnline
000922406 994__ $$a92$$bISE