A mechanism to produce a dawn-dusk component of plasma flow during magnetic reconnection in the magnetotail

Author:

Hawkins J. G.,Lee L. C.,Yan M.,Lin Y.,Perkins F. W.,Yamada M.

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

Reference11 articles.

1. Characteristics of high-speed ion flows in the plasma sheet;Baumjohann;J. Geophys. Res.,1990

2. On the structure of resistive MHD intermediate shocks;Hau;J. Geophys. Res.,1989

3. Statistical characteristics of plasma flow in the magnetotail;Hayakawa;J. Geophys. Res.,1982

4. Landau, L. D., , E. M., Lifshitz, , Electrodynamics of Continuous Media, Pergamon, Elmsford, N.Y., 1960,

5. Structure of the dayside reconnection layer in resistive MHD and hybrid models;Lin;J. Geophys. Res.,1993

Cited by 4 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Recent Experiments on Magnetic Reconnection in Laboratory Plasmas;Geophysical Monograph Series;2013-03-20

2. Magnetic reconnection;Reviews of Modern Physics;2010-03-05

3. Review of controlled laboratory experiments on physics of magnetic reconnection;Journal of Geophysical Research: Space Physics;1999-07-01

4. Study of driven magnetic reconnection in a laboratory plasma;Physics of Plasmas;1997-05

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