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2014 |

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 ... YEAR: 2014 DOI: 10.1002/2013JA019238 Magnetosphere; mode number; radial diffusion; Radiation belts; ULF waves; ultralow frequency |

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