We present statistical characteristics of electron microburst precipitation using high time‐
resolution measurements from the low‐altitude Electron Losses and Fields InvestigatioN …

The significant role of nonlinear wave–particle interactions in the macrodynamics and
microdynamics of the Earth's outer radiation belt has long been recognised. Electron …

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 …

Short and intense lower‐band chorus wave packets are ubiquitous in the Earth's outer
radiation belt. In this article, we perform various Vlasov hybrid simulations, with one or two …

Electron resonant scattering by whistler‐mode waves is one of the most important
mechanisms responsible for electron precipitation to the Earth's atmosphere. The temporal …

During magnetospheric storms, radiation belt electrons are produced and then removed by
collisions with the lower atmosphere on varying timescales. An efficient loss process is …

Electron fluxes in Earth's radiation belts are significantly affected by their resonant
interaction with whistler‐mode waves. This wave‐particle interaction often occurs via first …

Resonant interactions of energetic electrons with electromagnetic whistler‐mode waves
(whistlers) contribute significantly to the dynamics of electron fluxes in Earth's outer radiation …

The whistler‐mode chorus emission, a major driver of radiation belt electron energization
and precipitation, exhibits significant amplitude modulations on millisecond timescales …

Electromagnetic ion cyclotron (EMIC) waves can scatter radiation belt electrons with
energies of a few hundred keV and higher. To accurately predict this scattering and the …