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) …

The past decade transformed our observational understanding of energetic particle
processes in near‐Earth space. An unprecedented suite of observational systems was in …

Recent analysis of satellite data obtained during the 9 October 2012 geomagnetic storm
identified the development of peaks in electron phase space density, which are compelling …

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 …

Earth's diffuse aurora occurs over a broad latitude range and is primarily caused by the
precipitation of low-energy (0.1–30-keV) electrons originating in the central plasma sheet …

To improve our understanding of the role of electromagnetic ion cyclotron (EMIC) waves in
radiation belt electron dynamics, we perform a comprehensive analysis of EMIC wave …

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 …

Pulsating aurora, a spectacular emission that appears as blinking of the upper atmosphere
in the polar regions, is known to be excited by modulated, downward-streaming electrons …

Local acceleration driven by whistler‐mode chorus waves is fundamentally important for
accelerating seed electron populations to highly relativistic energies in the outer radiation …

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 …