Super-Alfvénic propagation of reconnection signatures and Poynting flux during substorms

Tens to hundreds of keV electron precipitation driven by kinetic Alfvén waves during an electron injection

Electron injections are critical processes associated with magnetospheric substorms, which deposit significant electron energy into the ionosphere. Although wave scattering of $<$10 keV electrons during injections has been well studied, the link between magnetotail electron injections and energetic ($\geq$100 keV) electron precipitation remains elusive. Using conjugate observations between the ELFIN and Magnetospheric Multiscale (MMS) missions, we present evidence of tens to hundreds of keV electron precipitation to the ionosphere potentially driven by kinetic Alfvén waves (KAWs) associated wi…

发现由核心局部化阿尔维恩离子温度梯度不稳定性引起的密度限制破坏在托卡马克等离子体中

Discovery of Density Limit Disruption Induced by Core-localized Alfv${é}$nic Ion Temperature Gradient Instabilities in a Tokamak Plasma

研究发现核心局部化阿尔维恩离子温度梯度不稳定性引发等离子体密度限制破坏，为未来聚变反应堆提供关键理解。

Large amplitude electromagnetic solitons in a fully relativistic magnetized electron-positron-pair plasma

Nonlinear propagation of purely stationary large amplitude electromagnetic (EM) solitary waves in a magnetized electron-positron (EP) plasma is studied using a fully relativistic two-fluid hydrodynamic model which accounts for physical regimes of both weakly relativistic $(P\ll nmc^2)$ and ultrarelativistic $(P\gg nmc^2)$ random thermal energies. Here, $P$ is the thermal pressure, $n$ the number density and $m$ the mass of a particle, and $c$ is the speed of light in vacuum. Previous theory in the literature [Phys. Plasmas \textbf{11}, 3078 (2004)] is advanced and generalized by the relativist…

The Origin of Underdense Plasma Downflows Associated with Magnetic Reconnection in Solar Flares

Magnetic reconnection is a universal process that powers explosive energy release events such as solar flares, geomagnetic substorms, and some astrophysical jets. A characteristic feature of magnetic reconnection is the production of fast reconnection outflow jets near the plasma Alfvén speeds. In eruptive solar flares, dark, finger-shaped plasma downflows moving toward the flare arcade have been commonly regarded as the principal observational evidence for such reconnection-driven outflows. However, they often show a speed much slower than that expected in reconnection theories, challenging t…