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 …

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 …

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 …

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 …

Gyroresonant wave particle interactions with whistler mode chorus play a fundamental role
in the dynamics of the Earth's radiation belts and inner magnetosphere, affecting both 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 …

We present statistical characteristics of electron microburst precipitation using high time‐
resolution measurements from the low‐altitude Electron Losses and Fields InvestigatioN …

Using the statistical wave power spectral profiles obtained from CRRES wave data within
the 0000–0600 MLT sector under different levels of geomagnetic activity and a modeled …

We extend our database of whistler mode chorus, based on data from seven satellites, by
including∼ 3 years of data from Radiation Belt Storm Probes (RBSP)‐A and RBSP‐B and …