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2014

Estimates of the power per mode number of broadband ULF waves at geosynchronous orbit

In studies of radial diffusion processes in the magnetosphere it is well known that ultralow frequency (ULF) waves of frequency mωd can resonantly interact with particles of drift frequency ωd, where m is the waves\textquoteright azimuthal mode number. Due to difficulties in estimating m, an oversimplifying assumption is often made in simulations, namely that all ULF wave power is located at a single mode number. In this paper a technique is presented for extracting information on the distribution of ULF power in a range o ...

Sarris, T.;

YEAR: 2014     DOI: 10.1002/2013JA019238

Magnetosphere; mode number; radial diffusion; Radiation belts; ULF waves; ultralow frequency



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