One of the most important issues in space physics is to identify the dominant processes that
transfer energy from the solar wind to energetic particle populations in Earth's inner …

Energetic particle fluxes in the outer zone radiation belts can vary over orders of magnitude
on a variety of timescales. Power at ULF frequencies, on the order of a few millihertz, have …

Strong interplanetary shock interactions with the Earth's magnetosphere have great impacts
on energetic particle dynamics in the magnetosphere. An interplanetary shock on 7 …

In this paper, we focus on the modeling of radial transport in the Earth's outer radiation belt.
A historical overview of the first observations of the radiation belts is presented, followed by …

The interaction between interplanetary shocks and the Earth's magnetosphere manifests in
many important space physics phenomena including particle acceleration. We investigated …

When a solar wind dynamic pressure impulse impinges on the magnetophere, ultra‐low‐
frequency (ULF) waves can be excited in the magnetosphere and the solar wind energy can …

A study was undertaken to estimate the radial diffusion timescale, τLL, for relativistic
electrons (2–6 MeV) to diffuse into the slot region due to drift‐resonance with Pc5 ULF …

Relativistic electron fluxes in the outer radiation belt exhibit highly variable complex
behavior. Previous studies have established a strong correlation of electron fluxes and the …

Solar wind dynamic pressure pulse is one of the sources of ultra‐low frequency (ULF)
waves. Based on 1‐second resolution magnetic field observations from SuperMAG from …

As one type of driver of magnetospheric Alfvén waves, foreshock transients have received
less attention than, for example, the Kelvin‐Helmholtz instability, discrete and broadband …