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Detailed Reference Information |
Draganov, A.B., Inan, U.S., Sonwalkar, V.S. and Bell, T.F. (1992). Magnetospherically reflected whistlers as a source of plasmaspheric hiss. Geophysical Research Letters 19: doi: 10.1029/91GL03167. issn: 0094-8276. |
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Ray-tracing simulations and estimates of whistler wave damping show that magnetospherically reflected whistlers can persist for ~102 s in a low frequency band ( f~1 kHz). The combined contribution from whistler rays produced by a single lightning flash but entering the magnetosphere at different points form a continuous hiss-like signal, as observed at a fixed point. Estimates indicate that the total whistler wave energy input into the magnetosphere from lightning discharges may maintain experimentally observed levels of magnetospheric hiss. ¿ American Geophysical Union 1992 |
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Abstract |
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Keywords
Magnetospheric Physics, Plasma waves and instabilities, Magnetospheric Physics, Plasmasphere, Meteorology and Atmospheric Dynamics, Lightning, Ionosphere, Wave-particle interactions |
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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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