Abstract The Electric and Magnetic Field Instrument and Integrated Science (EMFISIS)
investigation on the NASA Radiation Belt Storm Probes (now named the Van Allen Probes) …

Earth's radiation belt electrons exhibit pronounced dynamic variability in response to solar
activity and resultant changes in the solar wind. The nonadiabatic variability of radiation belt …

The flux of energetic electrons in the Earth's outer radiation belt can vary by several orders of
magnitude over time scales less than a day, in response to changes in properties of the …

The global distribution of chorus wave amplitudes and their wave normal angles is
investigated using high‐resolution wave spectra and waveform data from THEMIS for lower …

Van Allen radiation belts consist of relativistic electrons trapped by Earth's magnetic field.
Trapped electrons often drift azimuthally around Earth and display a butterfly pitch angle …

A statistical survey of plasma densities and electron distributions (0.5–100 keV) is performed
using data obtained from the Time History of Events and Macroscale Interactions During …

Whistler mode chorus waves in the outer Van Allen belt can have consequences for
acceleration of relativistic electrons through wave‐particle interactions. New multicomponent …

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

We perform test particle simulations of energetic electrons interacting with whistler mode
chorus emissions. We compute trajectories of a large number of electrons forming a delta …

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 …