Three-Dimensional Magnetohydrodynamic Simulation of a Global Solar Corona Using a Temperature Distribution Map Obtained from SOHO EIT Measurements
Authors:
- Keiji HayashiKeiji Hayashi
- Elena BenevolenskayaEBElena Benevolenskaya
- Todd HoeksemaTodd Hoeksema
- Yang LiuYLYang Liu
- Xue Pu ZhaoXZXue Pu Zhao
- 20 December 2005
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 636 (2) , L165-L168
Abstract
No abstract availableThis publication has 7 references indexed in Scilit:
- Magnetohydrodynamic Simulations of the Solar Corona and Solar Wind Using a Boundary Treatment to Limit Solar Wind Mass FluxThe Astrophysical Journal Supplement Series, 2005
- CHIANTI—An Atomic Database for Emission Lines. VI. Proton Rates and Other ImprovementsThe Astrophysical Journal Supplement Series, 2003
- Two‐Temperature Coronal Models fromSOHO/EIT ObservationsThe Astrophysical Journal, 1999
- CHIANTI - an atomic database for emission linesAstronomy and Astrophysics Supplement Series, 1997
- Solar activity and the coronaSolar Physics, 1996
- Numerical tests of a modified full implicit continuous eulerian (fice) scheme with projected normal characteristic boundary conditions for mhd flowsComputer Methods in Applied Mechanics and Engineering, 1987
- A model of interplanetary and coronal magnetic fieldsSolar Physics, 1969