The dynamics of relativistic electrons in the inner magnetosphere around the time of
geomagnetic disturbances have received considerable attention in recent years. In addition …

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 …

Strong enhancements of outer Van Allen belt electrons have been shown to have a clear
dependence on solar wind speed and on the duration of southward interplanetary magnetic …

Outer zone radiation belt electrons can undergo gyroresonant interaction with various
magnetospheric wave modes including whistler‐mode chorus outside the plasmasphere …

Electron acceleration inside the Earth's magnetosphere is required to explain increases in
the∼ MeV radiation belt electron flux during magnetically disturbed periods. Recent studies …

The response of outer radiation belt relativistic electrons to the October 9, 1990, magnetic
storm is analyzed in detail using a radial diffusion model and data from the Combined …

The classic view is that Dst and SYM‐H time series differ mainly due to the dissimilarity in
the method to determine the base values. Dst and SYM‐H are both indices designed to …

The outer zone radiation belt consists of energetic electrons drifting in closed orbits
encircling the Earth between∼ 3 and 7 RE. Electron fluxes in the outer belt show a strong …

The flux of relativistic electrons in the Earth's radiation belts is highly variable and can
change by orders of magnitude on timescales of a few hours. Understanding the drivers for …

Satellites can be damaged by high energy charged particles in the Earth's radiation belts
and during solar energetic particle (SEP) events. Here we review the growing reliance on …