Energetic electrons, 50 keV to 6 MeV, at geosynchronous orbit: Their responses to solar wind variations-Reference-Cited by-同舟云学术

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Energetic electrons, 50 keV to 6 MeV, at geosynchronous orbit: Their responses to solar wind variations

Published:2005-04 Issue:4 Volume:3 Page:n/a-n/a
ISSN:1542-7390
Container-title:Space Weather
language:en
Short-container-title:Space Weather

Author:

Li Xinlin¹,Baker D. N.¹,Temerin M.²,Reeves G.³,Friedel R.³,Shen C.⁴

Affiliation:

1. Laboratory for Atmospheric and Space Physics; University of Colorado; Boulder Colorado USA

2. Space Sciences Laboratory; University of California; Berkeley California USA

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

4. Laboratory for Space Weather; Chinese Academy of Sciences; Beijing China

Publisher

American Geophysical Union (AGU)

Subject

Atmospheric Science

Reference34 articles.

1. Nonlinear interaction of outer zone electrons with VLF waves;Albert;Geophys. Res. Lett.,2002

2. Highly relativistic electrons in the Earth's outer magnetosphere: 1. Lifetimes and temporal history 1979-1984;Baker;J. Geophys. Res.,1986

3. Linear prediction filter analysis of relativistic electron properties at 6.6 RE;Baker;J. Geophys. Res.,1990

4. A strong CME-related magnetic cloud interaction with the Earth's magnetosphere: ISTP observation of rapid relativistic electron acceleration on May 15, 1997;Baker;Geophys. Res. Lett.,1998

5. Strong electron acceleration in the Earth's magnetosphere;Baker;Adv. Space Res.,1998

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