A prediction model for the global distribution of whistler chorus wave amplitude developed separately for two latitudinal zones
Author:
Affiliation:
1. Department of Astronomy and Space Science; Chungbuk National University; Cheongju South Korea
2. Korea Astronomy and Space Science Institute; Daejeon South Korea
3. Department of Atmospheric and Oceanic Sciences; UCLA; Los Angeles California USA
Funder
NSL of the National Research Foundation of Korea
“Planetary system research for space exploration” project
KASI
NASA
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Geophysics
Link
http://onlinelibrary.wiley.com/wol1/doi/10.1002/2014JA020900/fullpdf
Reference108 articles.
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2. Statistics of whistler-mode waves in the outer radiation belt: Cluster STAFF-SA measurements;Agapitov;J. Geophys. Res. Space Physics,2013
3. Quasi-linear pitch angle diffusion coefficients: Retaining high harmonics;Albert;J. Geophys. Res.,1994
4. The THEMIS mission;Angelopoulos;Space Sci. Rev.,2008
5. Statistical study of chorus wave distributions in the inner magnetosphere using Ae and solar wind parameters;Aryan;J. Geophys. Res. Space Physics,2014
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