57 citations · 214 across the 12 of their papers we have counts for
13 papers
Properties of Intense Electromagnetic Ion Cyclotron Waves: Implications for Quasi-linear, Nonlinear, and Nonresonant Wave-Particle Interactions
Xiaofei Shi, Anton Artemyev, Xiao-Jia Zhang +3
Resonant interactions between relativistic electrons and electromagnetic ion cyclotron (EMIC) waves provide an effective loss mechanism for this important electron population in th…
Beam-driven ECH waves: A parametric study
Xu Zhang, Vassilis Angelopoulos, Anton V. Artemyev +1
Electron cyclotron harmonic (ECH) waves play a significant role in driving the diffuse aurora, which constitutes more than 75% of the particle energy input into the ionosphere. ECH…
Nonlinear Landau resonant interaction between kinetic Alfvén waves and thermal electrons: Excitation of time domain structures
Xin An, Jacob Bortnik, Xiaojia Zhang
Phase space holes, double layers and other solitary electric field structures, referred to as time domain structures (TDSs), often occur around dipolarization fronts in the Earth's…
Accretion of Gas Giants Constrained by the Tidal Barrier
Ya-Ping Li, Yi-Xian Chen, Douglas N. C. Lin +1
After protoplanets have acquired sufficient mass to open partial gaps in their natal protostellar disks, residual gas continues to diffuse onto horseshoe streamlines under effect o…
Long-term dynamics driven by resonant wave-particle interactions: from Hamiltonian resonance theory to phase space mapping
Anton V. Artemyev, Anatoly I. Neishtadt, Alexei. A. Vasiliev +3
In this study we consider the Hamiltonian approach for the construction of a map for a system with nonlinear resonant interaction, including phase trapping and phase bunching effec…
Retention of Long-Period Gas Giant Planets: Type II Migration Revisited
Yi-Xian Chen, Xiaojia Zhang, Ya-Ping Li +2
During their formation, emerging protoplanets tidally interact with their natal disks. Proto-gas-giant planets, with Hills radius larger than the disk thickness, open gaps and quen…