Statistical properties of tail plasma sheet electrons above 40 keV-Reference-Cited by-同舟云学术

Statistical properties of tail plasma sheet electrons above 40 keV

Published:2008-03 Issue:A3 Volume:113 Page:n/a-n/a
ISSN:0148-0227
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res.

Author:

Åsnes A.¹²,Friedel R. W. H.¹,Lavraud B.¹,Reeves G. D.¹,Taylor M. G. G. T.²,Daly P.³

Affiliation:

1. Los Alamos National Laboratory; Los Alamos New Mexico USA

2. ESTEC; Noordwijk Netherlands

3. Max-Planck Institute for Solar System Research; Katlenburg-Lindau Germany

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

Reference51 articles.

1. Energetic electron fluxes in the tail of the geomagnetic field;Anderson;J. Geophys. Res.,1965

2. Anderson , K. A. 1965 Radial dependence of energetic electron fluxes in the tail of the Earth's magnetic field 14

3. Energetic electron fluxes in and beyond the Earth's outer magnetosphere;Anderson;J. Geophys. Res.,1965

4. Bursty bulk flows in the inner central plasma sheet;Angelopoulos;J. Geophys. Res.,1992

5. Observations of energetic eletrons (>200 kev) in the Earth's magnetotail: Plasma sheet and fireball observations;Baker;J. Geophys. Res.,1977

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