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Detailed Reference Information |
Mann, I.R. (1998). An MHD model for driven high m field line resonances. Geophysical Research Letters 25: doi: 10.1029/98GL51092. issn: 0094-8276. |
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Radar observations of field line resonances (FLRs) show two categories of waves with large or small azimuthal wavenumbers (m). Low m resonances are relatively well understood theoretically, however high m waves appear to be continually driven and display characteristics which can only be understood by considering the effects of the driver. We discuss an heuristic model driving term suggested by [Southwood, 1974>, and recently adopted by [Fenrich and Samson, 1997> in an attempt to explain their observations. We show how their model introduces non-causal (unphysical) features which are not good approximations to reality. We offer a possible alternative heuristic MHD model which can better explain the observational features of high m FLRs. The new model formulation may generate modal solutions with the observed equatorwards phase motion, growth in time, and radially oscillatory characteristics. ¿ 1998 American Geophysical Union |
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Abstract |
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Keywords
Ionosphere, Ionosphere/magnetosphere interactions, Magnetospheric Physics, MHD waves and instabilities, Ionosphere, Wave propagation |
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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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