Owing to the ever-present solar wind, our vast solar system is full of plasmas. The turbulent
solar wind, together with sporadic solar eruptions, introduces various space plasma …

Storm time electron radiation belt dynamics have been widely investigated for many years.
Here we present a rarely reported nonstorm time event of electron radiation belt evolution …

It has been suggested that the equilibrium structure of the slot region, which separates the
inner and outer radiation belts, forms as the result of a balance between inward radial …

Precipitation of energetic electrons to the atmosphere is both a loss mechanism for radiation
belt particles and a means by which the geospace environment influences the Earth's …

Resonant pitch angle scattering by plasmaspheric hiss has long been considered to be
responsible for the energetic electron loss in the slot region, but the detailed quantitative …

Wave‐particle interaction which occurs in the radiation belts is generally determined by
variations in wave normal angles. Using the Gaussian wave normal angle () distribution, we …

The most significant unknown regarding relativistic electrons in Earth's outer Van Allen
radiation belt is the relative contribution of loss, transport, and acceleration processes within …

An unusual event of deep injections of> 30 keV electrons from the radiation belt to low L
shells (L< 1.2) in the midnight–dawn sector was found from NOAA/POES observations …