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Gang Qin

Researcher at Harbin Institute of Technology

Publications -  95
Citations -  2829

Gang Qin is an academic researcher from Harbin Institute of Technology. The author has contributed to research in topics: Diffusion (business) & Solar energetic particles. The author has an hindex of 25, co-authored 95 publications receiving 2560 citations. Previous affiliations of Gang Qin include Florida Institute of Technology & University of Delaware.

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Nonlinear collisionless perpendicular diffusion of charged particles

TL;DR: In this article, a nonlinear theory of the perpendicular diffusion of charged particles is presented, including the influence of parallel scattering and dynamical turbulence, and the theory shows encouraging agreement with numerical simulations.
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Perpendicular Transport of Charged Particles in Composite Model Turbulence: Recovery of Diffusion

TL;DR: In this article, Qin, Matthaeus, and Bieber demonstrate that parallel scattering suppresses perpendicular diffusion to a sub-diffusive level when the turbulence lacks transverse structure, and a second regime of diffusive transport can be established.
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Subdiffusive transport of charged particles perpendicular to the large scale magnetic field

TL;DR: In this article, the authors examined the transport of charged particles across the mean magnetic field due to broad band, powerlaw-distributed magnetic fluctuations by direct computation of a large number of charged test particle trajectories.
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Nonlinear Parallel and Perpendicular Diffusion of Charged Cosmic Rays in Weak Turbulence

TL;DR: In this article, a nonlinear guiding center theory for parallel and perpendicular diffusion of cosmic rays is proposed, which is based on a coupled system of nonlinear Fokker-Planck coefficients.
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Propagation of solar energetic particles in three-dimensional interplanetary magnetic fields

TL;DR: In this article, a model calculation of solar energetic particle propagation in a three-dimensional interplanetary magnetic field is presented, which includes essentially all the particle transport mechanisms: streaming along magnetic field lines, convection with the solar wind, pitch-angle diffusion, focusing by the inhomogeneous interplanarial magnetic field, perpendicular diffusion, and pitch angle dependent adiabatic cooling by the expanding solar wind.