Hostname: page-component-7b7567c8c-7pwfn Total loading time: 0 Render date: 2026-11-15T07:16:33.837Z Has data issue: false hasContentIssue false

Parametric excitation of electromagnetic waves in a magnetized plasma

Published online by Cambridge University Press:  04 April 2001

A. K. YUKHIMUK
Affiliation:
Main Astronomical Observatory of the National Academy of Sciences of Ukraine, Kyiv-22, 252650, Ukraine
V. A. YUKHIMUK
Affiliation:
Los Alamos National Laboratory, Los Alamos, NM87545, USA
O. K. SIRENKO
Affiliation:
Main Astronomical Observatory of the National Academy of Sciences of Ukraine, Kyiv-22, 252650, Ukraine
Yu. M. VOITENKO
Affiliation:
Main Astronomical Observatory of the National Academy of Sciences of Ukraine, Kyiv-22, 252650, Ukraine
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the 'Save PDF' action button.

The parametric interaction of an upper-hybrid pump wave with kinetic Alfvén and electromagnetic waves that propagate in parallel and perpendicular directions to the ambient magnetic field is investigated on the basis of two-fluid magnetohydrodynamics. A nonlinear dispersion relation describing three-wave interaction and instability growth rates are found. The theoretical results are used for the interpretation of satellite observations in the magnetospheric plasma. It is shown that as a result of the decay of an upper-hybrid wave, electromagnetic waves propagating in both parallel and perpendicular directions to the ambient magnetic field are generated. The instability growth rate is much higher in the case of left-polarized electromagnetic wave generation than in the case of ordinary electromagnetic wave generation. The nonlinear parametric processes studied here could also take place during powerful bursts on the Sun, and in the magnetosphere of Jupiter.

Information

Type
Research Article
Copyright
1999 Cambridge University Press