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- W2000643075 abstract "The effect of the azimuthal angle ψ of the wave vector k on the propagation characteristics of the superluminous L–O mode waves (together with a case of the R-X mode) during different geomagnetic activities using a three-dimensional (3D) ray-tracing method is investigated. This work is primarily an extension of our previous two-dimensional study in which the wave azimuthal angle was not considered. We present numerical simulations for this mode which is generated in the source cavity along a 70° night geomagnetic field line at the specific altitude of 1.5RE (where RE is the Earth's radius). It is found that, as in the two-dimensional case, the trajectory of L–O mode starting in the source meridian plane (or the wave azimuthal angle ψ = 180°) can reach the lowest latitude; whereas it basically stays at relatively higher latitudes starting off the source meridian plane (or ψ ≠ 180°). The results reveal that under appropriate conditions, the superluminous L–O mode waves may exist in the radiation belts of the Earth, but this remains to be supplemented by observational data." @default.
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- W2000643075 date "2008-10-01" @default.
- W2000643075 modified "2023-09-24" @default.
- W2000643075 title "Propagation of Superluminous L–O Mode Waves During Geomagnetic Activities" @default.
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- W2000643075 doi "https://doi.org/10.1088/1009-0630/10/5/05" @default.
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