The plasmasphere sandwiched between the ionosphere and the outer magnetosphere is
populated by up flow of ionospheric cold (∼ 1 eV) and dense plasma along geomagnetic …

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

A comparison of how well three different electric field models can predict the storm time
plasmapause shape is conducted. The magnetic storm of 17 April 2002 is selected for this …

Transport and acceleration of the 5–50 keV electrons from the plasma sheet to geostationary
orbit were investigated. These electrons constitute the low‐energy part of the seed …

In the diffuse aurora, magnetospheric electrons, initially precipitated from the inner plasma
sheet via wave‐particle interaction processes, degrade in the atmosphere toward lower …

Three ring current models are used to follow the evolution of the proton ring current during
the 2001‐04‐21–25 storm: The ring current model combined with tracing particles …

The storm time inner magnetospheric electric field morphology and dynamics are assessed
by comparing numerical modeling results of the plasmasphere and ring current with many in …

In addition to wave particle scattering in the magnetosphere, atmospheric backscatter of
magnetospheric electrons is an important process that contributes to the formation of the …

The main point of the paper is to investigate how much the modeled ring current depends on
the representations of magnetic and electric fields and boundary conditions used in …

Ninety intense magnetic storms (minimum Dst value of less than− 100 nT) from solar cycle
23 (1996–2005) were simulated using the hot electron and ion drift integrator (HEIDI) model …