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Empirical versus exact numerical quasilinear analysis of electromagnetic instabilities driven by temperature anisotropy

Published online by Cambridge University Press:  29 September 2011

PETER H. YOON
Affiliation:
School of Space Research, Kyung Hee University, Yongin-Si, Gyeonggi-Do, 446-701, South Korea ([email protected]) Institute for Physical Science and Technology, University of Maryland, College Park, MD 20742, USA
JUNG JOON SEOUGH
Affiliation:
School of Space Research, Kyung Hee University, Yongin-Si, Gyeonggi-Do, 446-701, South Korea ([email protected])
KHAN HYUK KIM
Affiliation:
School of Space Research, Kyung Hee University, Yongin-Si, Gyeonggi-Do, 446-701, South Korea ([email protected])
DONG HUN LEE
Affiliation:
School of Space Research, Kyung Hee University, Yongin-Si, Gyeonggi-Do, 446-701, South Korea ([email protected])

Abstract

In the present paper, quasilinear development of anisotropy-driven electromagnetic instabilities is computed on the basis of recently formulated empirical wave dispersion relation and compared against exact numerical calculation based upon transcendental plasma dispersion function and exact numerical roots. Upon comparison with the exact method it is demonstrated that the empirical model provides reasonable results. The present findings may be relevant to space physical application, as the present paper provides a useful short-cut research method for self-consistent analysis of temporal development of anisotropy-driven instabilities.

Type
Papers
Copyright
Copyright © Cambridge University Press 2011

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