The five THEMIS spacecraft and a dedicated ground-based observatory array will pinpoint
when and where substorms occur, thereby providing the observations needed to identify the …

One of the definitions of space weather describes it as the time-varying space environment
that may be hazardous to technological systems in space and/or on the ground and/or …

Gyroresonant wave‐particle interactions with very low frequency whistler mode chorus
waves can accelerate subrelativistic seed electrons (hundreds of keV) to relativistic energies …

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 …

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 …

Empirical models for the plasma densities in the inner magnetosphere, including
plasmasphere and polar magnetosphere, have been in the past derived from in situ …

We present the nowcast model for low‐energy (< 200 keV) electrons in the inner
magnetosphere, which is the version of the Inner Magnetosphere Particle Transport and …

In the present work, we determine how three well documented models of the
magnetospheric electric field, and two different mechanisms proposed for the formation of …

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 …

Numerous simulations were conducted in order to quantify the influence of nightside
conductance morphology and intensity on the storm‐time ring current and plasmasphere …