83 citations · 892 across the 63 of their papers we have counts for
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Temporal Scales of Electron Precipitation Driven by Whistler-Mode Waves
Xiao-Jia Zhang, Vassilis Angelopoulos, Anton Artemyev +4
Electron resonant scattering by whistler-mode waves is one of the most important mechanisms responsible for electron precipitation to the Earth's atmosphere. We investigate tempora…
Intense whistler-mode waves at foreshock transients: characteristics and regimes of wave-particle resonant interaction
Xiaofei Shi, Terry Liu, Anton Artemyev +3
Thermalization and heating of plasma flows at shocks result in unstable charged-particle distributions which generate a wide range of electromagnetic waves. These waves, in turn, c…
Tens to hundreds of keV electron precipitation driven by kinetic Alfvén waves during an electron injection
Y. Shen, A. V. Artemyev, X. -J. Zhang +9
Electron injections are critical processes associated with magnetospheric substorms, which deposit significant electron energy into the ionosphere. Although wave scattering of 1…
Nonresonant scattering of relativistic electrons by electromagnetic ion cyclotron waves in Earth's radiation belts
Xin An, Anton Artemyev, Vassilis Angelopoulos +3
Electromagnetic ion cyclotron waves are expected to pitch-angle scatter and cause atmospheric precipitation of relativistic ( MeV) electrons under typical conditions in Earth'…
Thin current sheet formation: comparison between Earth's magnetotail and coronal streamers
Anton Artemyev, Victor Reville, Ivan Zimovets +4
Magnetic field line reconnection is a universal plasma process responsible for the magnetic field topology change and magnetic field energy dissipation into charged particle heatin…
Relativistic electron precipitation by EMIC waves: importance of nonlinear resonant effects
Veronika S. Grach, Anton V. Artemyev, Andrei G. Demekhov +7
Relativistic electron losses in Earth's radiation belts are usually attributed to electron resonant scattering by electromagnetic waves. One of the most important wave mode for suc…
Configuration of magnetotail current sheet prior to magnetic reconnection onset
Xin An, Anton Artemyev, Vassilis Angelopoulos +3
The magnetotail current sheet configuration determines magnetic reconnection properties that control the substorm onset, one of the most energetic phenomena in the Earth's magnetos…
Fast inverse transform sampling of non-Gaussian distribution functions in space plasmas
Xin An, Anton Artemyev, Vassilis Angelopoulos +3
Non-Gaussian distributions are commonly observed in collisionless space plasmas. Generating samples from non-Gaussian distributions is critical for the initialization of particle-i…
Suppression of reconnection in polarized, thin magnetotail current sheets: 2D simulations and implications
Xin An, Anton Artemyev, Vassilis Angelopoulos +3
Many in-situ spacecraft observations have demonstrated that magnetic reconnection in the Earth's magnetotail is largely controlled by the pre-reconnection current sheet configurati…