Geomagnetic activity and local time dependence of the distribution of ultra low-frequency wave power in azimuthal wavenumbers, <i>m</i>

The azimuthal wavenumber <i>m</i> of ultra low-frequency (ULF) waves in the magnetosphere is a required parameter in the calculations of the diffusion rates of energetic electrons and protons in the magnetosphere, as electrons and protons of drift frequency <i>ω</i><sub...

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Bibliographic Details
Main Authors: T. E. Sarris, X. Li
Format: Article
Language:English
Published: Copernicus Publications 2017-05-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/35/629/2017/angeo-35-629-2017.pdf