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JOURNAL OF GEOPHYSICAL RESEARCH,
VOL. 109,
A11301,
doi:10.1029/2004JA010636,
2004
Collisional shear instability in the equatorial F region ionosphere
D. L. Hysell
Department of Earth and Atmospheric Science, Cornell University, Ithaca, New York, USA
E. Kudeki
Department of Electrical and Computer Engineering, University of Illinois, Urbana, Illinois, USA
Abstract
A collisional shear instability in a magnetized plasma is described and evaluated. The instability is related to electrostatic
Kelvin Helmholtz but operates in inhomogeneous plasmas in the collisional regime. Boundary value analysis predicts that the
linear growth rate for the instability could be comparable to that of the collisional interchange instability in the equatorial
F region ionosphere under ideal conditions. An initial value simulation of a nonlinear model of the instability run under realistic
conditions produces growing waves with a relatively long growth time (50 min) and with an initial wavelength of about 30 km.
The simulation results are consistent with recent radar observations showing large-scale plasma waves in the bottomside equatorial
ionosphere at sunset prior to the onset of spread F conditions. The role of shear instability in preconditioning the F region for interchange instabilities to occur after sunset is discussed.
Received 17
June
2004;
accepted 27
August
2004;
published 3
November
2004.
Keywords: coherent scatter radar;
ionospheric irregularities;
shear;
equatorial spread F;
plasma instability;
equatorial ionosphere.
Index Terms: 2471 Ionosphere: Plasma waves and instabilities; 2415 Ionosphere: Equatorial ionosphere; 2439 Ionosphere: Ionospheric irregularities; 6929 Radio Science: Ionospheric physics (2409).
Subscriber Access to Full Article (Nonsubscribers may purchase for $9.00, Includes print PDF, file size: 3647457 bytes)
Citation: Hysell, D. L., and E. Kudeki
(2004),
Collisional shear instability in the equatorial F region ionosphere,
J. Geophys. Res.,
109,
A11301,
doi:10.1029/2004JA010636.
Copyright 2004 by the American Geophysical Union.
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