Discovery of the Earth's Van Allen radiation belts by instruments flown on Explorer 1 in 1958
was the first major discovery of the Space Age. The observation of distinct inner and outer …

In this paper we review recent spacecraft observations of oblique whistler-mode waves in
the Earth's inner magnetosphere as well as the various consequences of the presence of …

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 …

How to properly describe resonant interactions between electrons and quasi‐coherent
chorus waves is still an open question. Previous studies have progressed from modeling …

Prompt recovery of MeV (millions of electron Volts) electron populations in the poststorm
core of the outer terrestrial radiation belt involves local acceleration of a seed population of …

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 …

Whistler mode chorus waves are responsible for electron acceleration in Earth's radiation
belts. It is unclear, however, whether the observed acceleration is still well described by …

We use test particle simulations to model the interaction between radiation belt electrons
and whistler mode chorus waves by focusing on wave amplitude modulations. We quantify …

Many spacecraft fly within or through a natural and variable particle accelerator powered by
the coupling between the magnetosphere and the solar wind: the Earth's radiation belts …

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 …