Solar wind fast streams emanating from solar coronal holes cause recurrent, moderate
intensity geomagnetic activity at Earth. Intense magnetic field regions called Corotating …

The Earth's diffuse auroral precipitation provides the major source of energy input into the
nightside upper atmosphere and acts as an essential linkage of the magnetosphere …

Abstract The NASA Radiation Belt Storm Probes (RBSP) mission addresses how
populations of high energy charged particles are created, vary, and evolve in space …

Particle acceleration and loss in the million electron Volt (MeV) energy range (and above) is
the least understood aspect of radiation belt science. In order to measure cleanly and …

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 …

We present a brief review of radiation belt electron losses which are vitally important for
controlling the dynamics of the radiation belts. A historical overview of early observations is …

This paper focuses on the modeling of local acceleration and loss processes in the outer
radiation belt. We begin by reviewing the statistical properties of waves that violate the first …

Electromagnetic ion cyclotron (EMIC) waves which propagate at frequencies below the
proton gyrofrequency can undergo cyclotron resonant interactions with relativistic electrons …

We present analytic expressions for ULF wave‐derived radiation belt radial diffusion
coefficients, as a function of L and Kp, which can easily be incorporated into global radiation …