Three-dimensional steady compressible perturbations in the magnetohydrodynamic solar wind-Reference-Cited by-同舟云学术

Three-dimensional steady compressible perturbations in the magnetohydrodynamic solar wind

Published:1993 Issue:A7 Volume:98 Page:11501
ISSN:0148-0227
Container-title:Journal of Geophysical Research
language:en
Short-container-title:J. Geophys. Res.

Author:

Lou Yu-Qing

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://www.agu.org/journals/ja/v098/iA07/93JA00633/93JA00633.pdf

Reference82 articles.

1. Solar wind acceleration caused by the gradient of Alfvén wave pressure;Alazraki;Astron. Astrophys. J.,1971

2. Alfvén waves in stellar winds;Barkhudarov;Sol. Phys.,1991

3. Hydromagnetic waves and turbulence in the solar wind;Barnes,1979

4. Alfvénic wave pressures and the solar wind;Belcher;Astrophys. J.,1971

5. Large-amplitude Alfvén waves in the interplanetary medium: Mariner 5;Belcher;J. Geophys. Res.,1969

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