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 …

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 …

Test particle codes indicate that electron dynamics due to interactions with low amplitude
incoherent whistler mode‐waves can be adequately described by quasi‐linear theory …

Particle-in-cell methods employ particle representations of unknown fields but also employ
continuum fields for other parts of the problem. Thus projection between particle and …

Long-term simulations of energetic electron fluxes in many space plasma systems require
accounting for two groups of processes with well separated time-scales: a microphysics of …

Resonant interactions with electromagnetic whistler-mode waves are a primary driver of
energetic electron dynamics in the Earth's radiation belts. The most intense waves can …

Abstract The fast Van Allen radiation belt electron dynamics during geomagnetic storms
have not yet been fully explained, in part due to limitations of standard satellite missions in …

Analysis of long timespan heliophysics and space physics data or application of machine
learning algorithms can require access to petabyte-scale and larger data sets and sufficient …

The magnetization| Ωe|/ω e is an important parameter in plasma astrophysics, where Ωe and
ω e are the electron gyro-frequency and electron plasma frequency, respectively. It depends …