@article{922406,
      recid = {922406},
      author = {Feng, Xueshang,},
      title = {Magnetohydrodynamic modeling of the solar corona and  heliosphere /},
      pages = {1 online resource :},
      abstract = {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.},
      url = {http://library.usi.edu/record/922406},
      doi = {https://doi.org/10.1007/978-981-13-9081-4,  https://doi.org/10.1007/978-981-13-9},
}