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 …

Magnetohydrodynamic (MHD) oscillatory processes in different plasma systems, such as the
corona of the Sun and the Earth's magnetosphere, show interesting similarities and …

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

Learning from successful applications of methods originating in statistical mechanics,
complex systems science, or information theory in one scientific field (eg, atmospheric …

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 …

We present results from global, three‐dimensional magnetohydrodynamic (MHD)
simulations of the solar wind/magnetosphere interaction. These MHD simulations are used …

Structures in the solar wind result from two basic mechanisms: structures injected or
imposed directly by the Sun, and structures formed through processing en route as the solar …

The solar wind‐magnetosphere system is nonlinear. The solar wind drivers of
geosynchronous electrons with energy range of 1.8–3.5 MeV are investigated using mutual …

The source of the slow solar wind has challenged scientists for years. Periodic density
structures (PDSs), observed regularly in the solar wind at 1 AU, can be used to address this …

The magnetopause is the key region in space for the transfer of solar wind mass,
momentum, and energy into the magnetosphere. During the last decade, our understanding …