Shock waves standing in the middle- and high-latitude magnetosheath from global MHD simulations-Reference-Cited by-同舟云学术

Shock waves standing in the middle- and high-latitude magnetosheath from global MHD simulations

Published:2011-03 Issue:A3 Volume:116 Page:
ISSN:0148-0227
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res.

Author:

Guo X. C.¹,Wang C.¹,Sun T. R.¹,Hu Y. Q.²

Affiliation:

1. State Key Laboratory of Space Weather, Center for Space Science and Applied Research; Chinese Academy of Sciences; Beijing China

2. CAS Key Laboratory of Basic Plasma Physics, School of Earth and Space Science; University of Science and Technology of China; Hefei China

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1029/2010JA016268/fullpdf

Reference22 articles.

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3. The piecewise parabolic method (PPM) for gas-dynamical simulations;Colella;J. Comput. Phys.,1984

4. A simple Riemann solver and high-order Godunov schemes for hyperbolic systems of conservation laws;Dai;J. Comput. Phys.,1995

5. Stationary slow shocks in the magnetosheath for solar wind conditions with β < 2/γ: Three-dimensional MHD simulations;De Sterck;J. Geophys. Res.,1999

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