MHD simulations of oppositely propagating Alfvén waves in the magnetosheath and solar wind-Reference-Cited by-同舟云学术

MHD simulations of oppositely propagating Alfvén waves in the magnetosheath and solar wind

Published:1998-06-01 Issue:11 Volume:25 Page:1821-1824
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

Cable S.,Lin Y.

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

http://www.agu.org/journals/gl/v025/i011/98GL01397/98GL01397.pdf

Reference8 articles.

1. Three-dimensional MHD simulations of the interaction between Venus and the solar wind;Cable;J. of Geophys. Res.,1995

2. A detached shock calculation by second-order finite differences;Lapidus;J. Comput. Phys.,1967

3. Generation of dynamic pressure pulses downstream of the bow shock by variations in the interplanetary magnetic field orientation;Lin;J. of Geophys. Res.,1996

4. Simulation of pressure pulses in the bow shock and magnetosheath driven by variations in interplanetary magnetic field direction;Lin;J. Geophys. Res.,1996

5. Nonlinear interaction of discontinuities in the solar wind and the origin of slow shocks;Neubauer;J. Geophys. Res.,1976

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