Model of the energization of outer-zone electrons by whistler-mode chorus during the October 9, 1990 geomagnetic storm

Author:

Summers D.1,Ma C.2,Meredith N. P.3,Horne R. B.4,Thorne R. M.5,Heynderickx D.6,Anderson R. R.7

Affiliation:

1. Department of Mathematics and Statistics; Memorial University of Newfoundland; St. John's Newfoundland Canada

2. Department of Computer Science; University of Calgary; Calgary Alberta Canada

3. Mullard Space Science Laboratory; University College London; Holmbury St. Mary, Dorking, Surrey UK

4. British Antarctic Survey; Natural Environment Research Council; Cambridge UK

5. Department of Atmospheric Sciences; University of California; Los Angeles California USA

6. Belgian Institute for Space Aeronomy; Brussels Belgium

7. Department of Physics and Astronomy; University of Iowa; Iowa City Iowa USA

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Reference21 articles.

1. CRRES plasma wave experiments;Anderson;J. Spacecr. Rockets,1992

2. Recurrent geomagnetic storms and relativistic electron enhancements in the outer magnetosphere: ISTP coordinated measurements;Baker;J. Geophys. Res.,1997

3. Radial diffusion analysis of outer radiation belt electrons during the October 9, 1990, magnetic storm;Brautigam;J. Geophys. Res.,2000

4. Relativistic electron dynamics in the inner magnetosphere-a review;Friedel;J. Atmo. Solar Terr. Phys.,2002

5. Horne , R. B. Rationale and requirements for a European space weather programme Proceedings of ESA Workshop 2002

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