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Shock Drift Electron Acceleration and Pitch Angle Scattering

Published online by Cambridge University Press:  13 May 2016

M. Vandas*
Affiliation:
Astronomical Institute, Academy of Sciences, Boční II 1401, 141 31 Praha 4, Czech Republic

Abstract

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Spacecraft measurements of energetic electrons in the vicinity of the Earth's bow shock and interplanetary shocks are analyzed and compared with theoretical calculations. It is concluded that shock drift acceleration of electrons is very modified by an additional process, probably by strong pitch angle scattering. Calculations including this effect are presented.

Type
Session VI: The Solar Wind and Heliosphere
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Anderson, K. 1981, JGR, 86, 4445.Google Scholar
Anderson, K., Lin, R., Martel, F., Lin, C., Parks, G., & Rème, H. 1979, GRL, 6, 401.Google Scholar
Gosling, J., Thomsen, M., Bame, S., & Russell, C. 1989, JGR, 94, 10,011.Google Scholar
Kocharov, L., Kovaltsov, G. A., & Torsti, J. 1999, ApJ, 519, 422.Google Scholar
Krauss-Varban, D., & Wu, C. 1989, JGR, 94, 15,367.Google Scholar
Leroy, M., & Mangeney, A. 1984, Ann. Geophys., 2, 449.Google Scholar
Vandas, M. 1989a, Bull. Astron. Inst. Czech., 40, 175.Google Scholar
Vandas, M. 1989b, Bull. Astron. Inst. Czech., 40, 189.Google Scholar
Vandas, M. 1995, JGR, 100, 23,499.Google Scholar
Wu, C. 1984, JGR, 89, 8857.Google Scholar