Concurrent users
Unlimited
Authorized users
Authorized users
Document Delivery Supplied
Can lend chapters, not whole ebooks
Title
Magnetohydrodynamic modeling of the solar corona and heliosphere / Xueshang Feng.
ISBN
9789811390814 (electronic book)
9811390819 (electronic book)
9789811390807
Published
Singapore : Springer, [2020]
Copyright
©2020
Language
English
Description
1 online resource : illustrations.
Item Number
10.1007/978-981-13-9081-4 doi
10.1007/978-981-13-9
Call Number
QB529 .F46 2020eb
Dewey Decimal Classification
523.7/5
Summary
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.
Bibliography, etc. Note
Includes bibliographical references.
Access Note
Access limited to authorized users.
Source of Description
Online resource; title from PDF title page (SpringerLink, viewed August 29, 2019).
Series
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.
