Hostname: page-component-5c6d5d7d68-wtssw Total loading time: 0 Render date: 2024-08-24T12:38:33.288Z Has data issue: false hasContentIssue false

The mean electromotive force generated by random Alfvén waves in a collisionless non-uniform plasma

Published online by Cambridge University Press:  13 March 2009

Hiromitsu Hamabata
Affiliation:
Department of Physics, Faculty of Science, Osaka City University, Osaka, Japan
Tomikazu Namikawa
Affiliation:
Department of Physics, Faculty of Science, Osaka City University, Osaka, Japan
Yasusi Hosoya
Affiliation:
Department of Physics, Faculty of Science, Osaka City University, Osaka, Japan

Abstract

The mean electromotive force produced by random hydromagnetic waves in a collisionless plasma is investigated taking into account non-uniformities in the mean magnetic field, fluid velocity and plasma density. It is shown that the mean electromotive force associated with gradients in mean quantities and the helicity spectrum function of the random velocity field exists and has a component parallel to the mean magnetic field which is associated with field-aligned gradients in mean quantities and density gradients parallel to the mean flow. The results are discussed in the context of the field-aligned currents in the earth's magnetosphere.

Type
Research Article
Copyright
Copyright © Cambridge University Press 1982

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

REFERENCES

Boström, R. A. 1964 J. Geophys. Res. 69, 4983.CrossRefGoogle Scholar
Boström, R. A. 1968 Ann. Geophys. 24, 681.Google Scholar
Boström, R. A. 1975 Physics of the hot plasma in the magnetosphere (ed. Hultqvist, B. and Stenflo, L.), p. 341. Plenum.CrossRefGoogle Scholar
Iijima, T. & Potemra, T. A. 1978 J. Geophys. Res. 83, 599.CrossRefGoogle Scholar
Krause, F. & Rädler, K.-H. 1981 Mean field magnetohydrodynamics and dynamo theory. Pergamon.Google Scholar
Moffatt, H. K. 1978 Magnetic field generation in electrically conducting fluids. Cambridge University Press.Google Scholar
Namikawa, T. 1980 Highlights of the Japanese IMS program, p. 430. Institute of Space and Aeronautical Sciences, University of Tokyo.Google Scholar
Namikawa, T., Hosoya, Y. & Hamabata, H. 1981 Proceedings of 1980 ISAS Symposium on Magneto-ionosphere, p. 77. University of Tokyo.Google Scholar
Namikawa, T. & Hamabata, H. 1982 a J. Plasma Phys. 27, 415.CrossRefGoogle Scholar
Namikawa, T. & Hamabata, H. 1982 b J. Plasma Phys. 28, 293.CrossRefGoogle Scholar
Parker, E. N. 1979 Cosmical magnetic fields. Oxford University Press.Google Scholar
Roberts, P. H. & Stix, M. 1971 The turbulent dynamo: a translation of a series of papers by F. Krause, K.-H. Rädler & M. Steenbeck. NCAR, Boulder, Colorado Tech. Note, 1A–60.Google Scholar
Rostoker, G. & Boström, R. 1974 Report TRITA-EPP-74–25. Royal Institute of Technology, Stockholm.Google Scholar
Steenbeck, M., Krause, F. & Rädler, K.-H. 1966 Z. Naturf. 21a, 369.CrossRefGoogle Scholar
Wälder, M., Deinzer, W. & Stix, M. 1980 J. Fluid Mech. 96, 207.CrossRefGoogle Scholar