Earth's radiation belt electrons exhibit pronounced dynamic variability in response to solar
activity and resultant changes in the solar wind. The nonadiabatic variability of radiation belt …

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 …

Local acceleration is required to explain electron flux increases in the outer Van Allen
radiation belt during magnetic storms. Here we show that fast magnetosonic waves …

Coupling between the Rice Convection Model and Ring Current–Atmospheric Interactions
Model codes is used to simulate the dynamical evolution of ring current ion phase space …

Fast magnetosonic waves can lead to the local acceleration of electrons from∼ 10 keV up to
a few MeV on a timescale of 1–2 d and may play an important role in radiation belt …

We investigate the importance of electron scattering by magnetosonic waves in the Earth's
inner magnetosphere. A statistical survey of the magnetosonic wave amplitude and wave …

Recent analysis using quasilinear theory (QLT) has shown that magnetosonic (MS) waves
are able to accelerate electrons to relativistic energies on fast time scales (∼ 1 day) …

Recent observations show that the decay rate of relativistic electrons measured at low
altitudes in the slot region at L= 2 is an order of magnitude shorter than theoretical estimates …

We report a representative concurrent event of four wave modes at L≈ 5.0, including
electrostatic electron cyclotron harmonic (ECH) waves, exohiss, magnetosonic (MS) waves …

A Polar magnetosonic wave (MSW) study was conducted using 1 year of 1996–1997 data
(during solar minimum). Waves at and inside the plasmasphere were detected at all local …