Perpendicular Transport of Charged Particles in Composite Model Turbulence: Recovery of Diffusion
By Gang Qin, William H. Matthaeus, J. Bieber. 2002
231 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/e7aba5c79cc1dace688e110ff6c33fbc5847de53
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- William H. Matthaeus
- Huirong Yan
- Gang Qin
- A. Shalchi
- A. Lazarian
- Gary Zank
- J. Bieber
- Charles W. Smith
In Molecular Biology
- William H. Matthaeus
- A. Shalchi
- Gang Qin
- Gary Zank
- J. Bieber
- Charles W. Smith
- A. Lazarian
- Huirong Yan
Citations in the corpus
- Cosmic-Ray Propagation: Nonlinear Diffusion Parallel and Perpendicular to Mean Magnetic Field (2007, background): “It was also proposed that with substantial transverse structure, i.e., transverse displacement of field lines, perpendicular diffusion is recovered (Qin et al 2002).”
- Nonlinear Collisionless Perpendicular Diffusion of Charged Particles (2003, methodology): “The two-dimensional component is generated similarly in a 4096# Fourier series in a box of size 102l (see Qin et al. 2002b).4096 7 Particles are integrated using a fourth-order adaptive-step Runge-Kutta method with a relative error control set to 1 part per billion.”
- Nonlinear Parallel and Perpendicular Diffusion of Charged Cosmic Rays in Weak Turbulence (2004, methodology): “Recent numerical studies (Qin 2002; Qin et al. 2002a, 2002b) have demonstrated that theoretical results of quasilinear theory (QLT; Jokipii 1966) for the parallel mean free path do not agree with results from simulations (see Minnie 2002 for a detailed review) if a general turbulence geometry is…”
- PROPAGATION OF SOLAR ENERGETIC PARTICLES IN THREE-DIMENSIONAL INTERPLANETARY MAGNETIC FIELDS (2009, background): “It has been confirmed from test particle simulations that the perpendicular to parallel diffusion coefficient ratio could indeed be as large as unity with some prescribed magnetic turbulence (Giacalone & Jokipii 1999; Qin et al. 2002; Qin 2002).”
- Particle acceleration at perpendicular shock waves: Model and observations (2005, background): “ Qin et al. [2002a, 2002b] showed using numerical simulations that perpendicular diffusion could occur only in the presence of a transverse complex magnetic field; that is, if field lines sampled by the gyromotion of a particle experiencing parallel and antiparallel scattering along the field are s”