Effects of shock parameters on upstream energetic electron burst events

Author:

Yuan Xingqiu12,Cairns Iver H.1,Trichtchenko Larisa2,Rankin Robert3

Affiliation:

1. School of Physics; University of Sydney; Sydney, New South Wales Australia

2. Geomagnetic Laboratory, Natural Resource Canada; Ottawa, Ontario Canada

3. Department of Physics; University of Alberta; Edmonton, Alberta Canada

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

Reference40 articles.

1. Energetic electrons of terrestrial origin behind bow shock and upstream in solar wind;Anderson;J. Geophys. Res.,1969

2. Measurements of bow shock particles far upstream from the Earth;Anderson;J. Geophys. Res.,1981

3. Thin sheets of energetic electrons upstream from the Earth's bow shock;Anderson;Geophys. Res. Lett.,1979

4. Simulation of electron acceleration at collisionless shocks: The effects of surface fluctuations;Burgess;Astrophys. J.,2006

5. The electron distribution function upstream from the Earth's bow shock;Cairns;J. Geophys. Res.,1987

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