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Detailed Reference Information |
Hamza, A.M. (1999). Perkins instability revisited. Journal of Geophysical Research 104: doi: 10.1029/1999JA900307. issn: 0148-0227. |
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A thorough review of the Perkins instability is presented in this paper. We introduce two new elements to the earlier model presented by Perkins [1973>, namely, the neutral wind velocity and gradients in the background field line integrated density and Pedersen conductivity, respectively. We derive the eigenfrequencies and growth rates for a new instability and recover the limiting cases discussed by Perkins [1973> and Miller [1997>. The presence of gradients in the background density and Pedersen conductivity reveals a new branch in the dispersion relation and can possibly enhance the Perkins instability growth rate. The need for horizontal gradients, as was pointed out by Basu et al. [1981>, is essential for the generation of small-scale and kilometer-scale irregularities. The Perkins instability is shown to be enhanced by both the presence of a neutral wind and the background density and Pedersen conductivity. ¿ 1999 American Geophysical Union |
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Abstract |
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Keywords
Ionosphere, Ionosphere/atmosphere interactions, Ionosphere, Plasma waves and instabilities, Ionosphere, Midlatitude ionosphere, Ionosphere, Ionospheric irregularities, Interplanetary Physics, Ejecta, driver gases, and magnetic clouds, Interplanetary Physics, Interplanetary magnetic fields, Space Plasma Physics, Numerical simulation studies |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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