Energy filter effect for solar wind particle entry to the plasma sheet via flank regions during southward interplanetary magnetic field

Author:

Zhou X.-Z.12,Pu Z. Y.23,Zong Q.-G.1,Xie L.2

Affiliation:

1. Center for Atmospheric Research; University of Massachusetts; Lowell Massachusetts USA

2. Institute of Space Physics and Applied Technology; Peking University; Beijing China

3. Center for Space Science and Applied Research; Chinese Academy of Sciences; Beijing 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

Reference27 articles.

1. Some properties of magnetospheric neutral surfaces;Alfvén;J. Geophys. Res.,1968

2. Trapping conditions for energetic particles incident on a tangential discontinuity surface;Baumjohann;Planet. Space Sci.,1987

3. Average plasma properties in the central plasma sheet;Baumjohann;J. Geophys. Res.,1989

4. The superdense plasma sheet: Plasmaspheric origin, solar wind origin, or ionospheric origin?;Borovsky;J. Geophys. Res.,1997

5. The adiabatic flow model of a neutral sheet;Cowley;Cosm. Electrodyn.,1971

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