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

Loss mechanisms responsible for the sudden depletions of the outer electron radiation belt
are examined based on observations and radial diffusion modeling, with L*‐derived …

We analyze wave and particle data from the CRRES satellite to determine the variability of
plasmaspheric hiss (0.1< f< 2 kHz) with respect to substorm activity as measured by AE …

We perform a comprehensive analysis to evaluate hiss‐induced scattering effect on the pitch
angle evolution and associated decay processes of relativistic electrons. The results show …

Relativistic electrons in the outer radiation belt are subjected to pitch angle and energy
diffusion by chorus, electromagnetic ion cyclotron (EMIC), and hiss waves. Using quasi …

The fluxes of energetic particles in the radiation belts are found to be strongly controlled by
the solar wind conditions. In order to understand and predict the radiation particle intensities …

Energetic electrons (E> 100 keV) in the Earth's radiation belts undergo Doppler‐shifted
cyclotron resonant interactions with a variety of whistler mode waves leading to pitch angle …

Much current research in magnetospheric physics is directed toward understanding the
dramatic variations in relativistic (> 1 MeV) electron fluxes that can take place in the Earth's …

We compute quasilinear diffusion rates due to pitch angle scattering by various mechanisms
in the Earth's electron radiation belts. The calculated theoretical lifetimes are compared with …

We study the effect of electromagnetic ion cyclotron (EMIC) wave scattering on radiation belt
electrons during the large geomagnetic storm of 21 October 2001 with minimum Dst=− 187 …