Electron resonant interaction with whistler mode waves is traditionally considered as one of
the main drivers of radiation belt dynamics. The two main theoretical concepts available for …

Electron losses from the outer radiation belt are typically attributed to resonant electron
scattering by whistler‐mode waves. Although the quasi‐linear diffusive regime of such …

Wave‐particle resonant interaction is a key process controlling energetic electron flux
dynamics in the Earth's radiation belts. All existing radiation belt codes are Fokker‐Planck …

Energetic electron precipitation into Earth's atmosphere is an important process for radiation
belt dynamics and magnetosphere‐ionosphere coupling. The most intense form of such …

The impact of randomly distributed field‐aligned density irregularities on whistler‐mode
wave propagation is investigated using full‐wave simulations and multipoint spacecraft …

We derive weak turbulence and quasilinear models for relativistic charged particle dynamics
in pitch-angle and energy space, due to interactions with electromagnetic waves …

Radiation belt codes evolve electron dynamics due to resonant wave‐particle interactions. It
is not known how to best incorporate electron dynamics in the case of a wave power …

In the Earth's radiation belts, an upper limit on the electron flux is expected to be imposed by
the Kennel‐Petschek mechanism, through the generation of exponentially more intense …

The electron resonant interaction with whistler‐mode waves is characterized by transport in
pitch angle–energy space. We calculate electron diffusion and advection coefficients (a …

Electron resonant interactions with electromagnetic whistler-mode waves play an important
role in electron flux dynamics in various space plasma systems: planetary radiation belts …