"Numerical modeling of magnetohydrodynamic activity in the
Swarthmore spheromak experiment",
V. S. Lukin, G. Qin, W. H. Matthaeus and M. R. Brown,
Phys. Plasmas,Volume 8, Number 5, 1600-1606, 2001.
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"Energetic particles and Magnetohydrodynamic Activity in the
Swarthmore spheromak experiment",
G. Qin, V. S. Lukin,C.D. Cothran, M. R. Brown and W. H. Matthaeus,
Phys. Plasmas,Volume 8, Number 11, 4816-4826, 2001.
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"Subdiffusive transport of charged particles perpendicular to
the large scale magnetic field",
G. Qin, W. H. Matthaeus and J. W. Bieber,
Geophys. Res. Lett., 29(4), 1048, doi:10.1029/2001GL014035, 2002.
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"Energetic particles from three-dimensional magnetic
reconnection events in the Swarthmore Spheromak Experiment",
M.R. Brown, C.D. Cothran, M. Landreman, D. Schlossberg, W.H. Matthaeus,
G. Qin, V.S. Lukin, and T. Gray,
Phys. Plasmas, Volume 9, Number 5, Part 2, 2077-2084,
2002.
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"Perpendicular transport of charged particles in composite
model turbulence: recovery of diffusion", G. Qin, W.H. Matthaeus
and J.W. Bieber, Astrophys. J., 578(2), L117-L120, 2002.
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"Transport in random magnetic fields: diffusion,
subdiffusion and nonlinear second diffusion", G. Qin, W.H. Matthaeus,
and J.W. Bieber, SOLAR WIND TEN: Proceedings of the Tenth
International Solar Wind Conference. AIP Conference Proceedings,
Volume 679, pp. 664-667, 2003
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"Nonlinear collisionless perpendicular diffusion of charged
particles", W.H. Matthaeus, G. Qin, J.W. Bieber and G.P. Zank,
Astrophys. J., 590(1), L53-L56, 2003.
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"Nonlinear Guiding Center Theory of Perpendicular Diffusion:
General Properties and Comparison with Oberservation",
J. W. Bieber, W. H. Matthaeus, A. Shalchi and G. Qin,
Geophys. Res. Lett., 31, 10, L10805, 2004
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"Interplanetary transport mechanisms of solar energetic
particles",
G. Qin, M. Zhang, J.R. Dwyer and H.K. Rassoul,
Astrophys. J., 609(2), 1076-1081, 2004,
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"Nonlinear Parallel and Perpendicular Diffusion of Charged
Cosmic Rays in Weak Turbulence"
A. Shalchi, J.W. Bieber, W.H. Matthaeus and G. Qin,
Astrophys. J., 616(1), 617-629, 2004,
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"The Model Dependence of Solar Energetic Particle Mean Free Paths
Under Weak Scattering",
G. Qin, M. Zhang, J.R. Dwyer, H.K. Rassoul G.M. Mason,
Astrophys. J., 627(1), 562-566, 2005
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"Parallel diffusion of charged particles in strong 2D turbulence",
G. Qin, W.H. Matthaeus, J.W. Bieber, Astrophys. J., 640(1),
L103-L106,
2006
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"The effect of adiabatic cooling on the fitted parallel mean free
path of solar energetic particles",
G. Qin, M. Zhang, J.R. Dwyer, J. Geophys. Res.,
111, A08101, 2006, doi:10.1029/2005JA011512
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"Ulysses observations of Jovian relativistic electrons in the
interplanetary space near Jupiter: Determination of perpendicular
particle transport coefficients and their energy dependence",
M. Zhang, G. Qin, H. Rassoul, B. McKibben, C. Lopate and B. Heber,
Planet. Space Sci., 55, Issues 1-2, 12-20, January, 2007
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"Nonlinear Parallel Diffusion of Charged Particles: Extension to the
Nonlinear Guiding Center Theory", G. Qin, Astrophys. J., 656(1),217-221,
2007
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Effect of flux tubes in solar wind on the diffusion of energetic
particles, G. Qin, and G. Li, Astrophys. J., 682, L129, 2008
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Propagation of Solar Energetic Particles in 3-dimensional
Interplanetary Magnetic Fields, M. Zhang, G. Qin and H. Rassoul,
Astrophys. J., 692, 109, 2009
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Prediction of the shock arrival times with SEP observations, G. Qin,
M. Zhang, and H.K. Rassoul, J. Geophys. Res., 114, A09104,
doi:10.1029/2009JA014332, 2009,
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Pitch angle diffusion coefficients of charged particles from computer
simulations, G. Qin and A. Shalchi, Astrophys. J., 707, 61-66,
2009
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Random Walk of Magnetic Field Lines: Analytical Theory versus
Simulations, A. Shalchi and G. Qin, Astrophys. Space Sci.,
330, 279, 2010
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A Simple Analytical Method to Determine Solar Energetic
Particles Mean Free Path, H.-Q. He and G. Qin, Astrophys. J.,
730:46 (6pp), 2011
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Effect of current sheets on the solar wind magnetic field power
spectrum from the Ulysses observation: from Kraichnan to Kolmogorov scaling,
G. Li, B. Miao, Q. Hu, and G. Qin, Phys. Rev. Lett., 106, 125001, 2011
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Propagation of Solar Energetic Particles in 3-dimensional
Interplanetary Magnetic Fields: In View of Characteristics of
Sources, H.-Q. He, G. Qin and M. Zhang, Astrophys. J., 734, 74, 2011
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An effect of perpendicular diffusion on the anisotropy of solar
energetic particles from unconnected sources, G. Qin, H.-Q. He, and M. Zhang,
Astrophys. J., 738, 28, 2011
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A realistic solar wind model with current sheets, G. Li, and G. Qin,
Proceedings of 5th Astrophysics Numerical Conference,
Numerical Modeling of Space Plasma Flows: ASTRONUM-2010,
Nikolai V. Pogorelov, Edouard Audit, and Gary P. Zank, eds,
ASP Conference Series, 444, 117, 2011
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Modeling the effect of current sheets on the power spectrum of
the solar wind magnetic field using a cell model, G. Li, G. Qin, Q. Hu, and
B. Miao, Geophys. Res. Lett., submitted
Numerical investigation of the infulence of large turbulence scales on
the parallel and perpendicular transport of cosmic rays, G. Qin, and A.
Shalchi, Astrophys. J., submitted
Using Soft X-ray observations to help the prediction of flare related
interplanetary shocks arrival times at the Earth, H.-L. Liu, and G. Qin, J.
Geophys. Res., submitted
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Effect of perpendicular diffusion on energetic particles accelerated by
the interplanetary coronal mass ejection shock, Y. Wang, G. Qin, and M. Zhang,
Astrophys. J., submitted
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Modulation of Galactic cosmic rays during the unusual solar
minimum of cycle 24, L.-L. Zhao, G. Qin, and M. Zhang, Astrophys. J.,
to be submitted
Simulation of reservoir phenomenon in gradual solar energetic particle
events, G. Qin, Y. Wang, and M. Zhang, J. Geophys. Res., to be
submitted