Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-26T04:27:24.392Z Has data issue: false hasContentIssue false
  • English
  • Français

Nonlinear development of the ion-cyclotron electromagnetic instability

Published online by Cambridge University Press:  13 March 2009

S. Cuperman ,
A. Sternlieb  and
D. J. Williams
S. Cuperman
Affiliation:
Department of Physics and Astronomy, Tel-Aviv University, Ramat Aviv, Israel
A. Sternlieb
Affiliation:
Department of Physics and Astronomy, Tel-Aviv University, Ramat Aviv, Israel
D. J. Williams
Affiliation:
SEL-ERL, NOAA, Boulder, Colorado
Get access Rights & Permissions [Opens in a new window]

Abstract

Cornwall et al. (1970) suggested that if the ring current protons penetrated the plasmapause, intense resonant electromagnetic ion cyclotron turbulence would lead to their rapid precipitation loss. IN this paper we present a computer simulation study of the electromagnetic ion-cyclotron instability in a homogeneous plasma consisting of protons and electrons embedded in a static magnetic field, B0x. The plasma parameters used are and Effects such as sources and losses or space non-uniformities are not considered here. The predictions of the linear theory for the fast build-up of unstable left-hand (proton-like) electromagnetic ion-cyclotron waves are fully confirmed.

Type
Research Article
Information
Journal of Plasma Physics , Volume 16 , Issue 1 , August 1976 , pp. 57 - 72
Copyright
Copyright © Cambridge University Press 1976

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

Cornwall, J. M., Coroniti, F. V. & Thorne, R. M. 1970 J. Geophys. Res. 75, 4899.Google Scholar
Cornwall, J. M. & Schulz, M. 1971 J. Geophys. Res. 76, 7791.Google Scholar
Cuperman, S. & Salu, Y. 1973 Plasma Phys. 15, 107.Google Scholar
Cuperman, S. & Salu, Y., Bernstein, W. & Williams, D. J. 1973 J. Geophys. Res. 78, 7372.Google Scholar
Cuperman, S., Gomberoff, L. & Sternlieb, A. 1975 J. Plasma Phys. 13, 259.Google Scholar
Forslund, D. W., Lindman, E. L., Mitchell, R. W. & Morse, R. L. 1972 Rep. LA-DC-72–721, 1972, Los Alamos Sci. Lab.Google Scholar
Gitomer, S. J. 1971 Phys. Fluids, 14, 1591.Google Scholar
Haber, I., Wagner, C. E., Boris, J. P. & Dawson, J. M. 1970 Proc. Fourth Conf. Numer. Simulation Plasmas, 126.Google Scholar
Hoffman, R. A. 1973 J. Geophys. Res. 78, 4771.Google Scholar
Kennel, C. F. & Petschek, H. E. 1966 J. Geophys. Res. 71, 1–28.Google Scholar
Morse, R. L. & Nielson, C. W. 1971 Phys. Fluids, 14, 830.Google Scholar
Ossakow, S. L., Ott, E. & Haber, I. 1972 Phys. Fluids, 15, 2314.Google Scholar
Scharer, J. 1969 Plasma Phys. 11, 1.Google Scholar
Wandzura, S. & Coroniti, F. V. 1975 Planet. Space Sci. 23, 123.Google Scholar
Williams, D. J., Fritz, T. A. & Konradi, A. 1973 J. Geophys. Res. 78, 4751.Google Scholar