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 present a three‐dimensional code (storm‐time evolution of electron radiation belt,
STEERB) for the storm‐time evolution of electron radiation belt following the preceding work …

The adiabatic transport process is introduced into our recently developed three‐dimensional
physics‐based electron radiation belt model (STEERB, Storm‐Time Evolution of Electron …

Abstract Van Allen Probes have detected nonlinear electrostatic spikes around injection
fronts in the outer radiation belt. These spikes include electron holes (EH), double layers …

During the period 19–22 November 2007, the near‐equatorial satellites THEMIS D (ThD)
and E (ThE) traversed the Earth's morningside magnetosphere once per day and for nearly …

Auroral brightening driven by interplanetary shocks on Earth's closed magnetic field lines is
commonly attributed to the 0.1–10 keV electron precipitations by electron cyclotron harmonic …

The electromagnetic ion cyclotron (EMIC) wave has long been suggested to be responsible
for the rapid loss of radiation belt relativistic electrons. The test‐particle simulations are …

We perform a comprehensive analysis of resonant scattering of diffuse auroral electrons by
oblique nightside chorus emissions present along a field line with an equatorial crossing of …

Using the statistical CRRES measurements of the electric field intensities of lower band
chorus (LBC) and upper band chorus (UBC) around L= 6 under geomagnetically moderate …

The precipitation of high‐energy magnetospheric electrons (E∼ 600 eV–10 KeV) in the
diffuse aurora contributes significant energy flux into the Earth's ionosphere. To fully …