Random walk of magnetic field lines: analytical theory versus simulations

DOI10.1007/S10509-010-0397-8zbMath1255.85007OpenAlexW2053162260MaRDI QIDQ613090

Sumit K. Garg

Publication date: 17 December 2010

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10509-010-0397-8

zbMATH Keywords

diffusionmagnetic fieldsturbulence

Mathematics Subject Classification ID

Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Computational methods for problems pertaining to astronomy and astrophysics (85-08) Stability and instability of geophysical and astrophysical flows (76E20) Statistical astronomy (85A35)

Related Items (1)

Magnetic field line random walk in non-axisymmetric turbulence

Cites Work

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• Nonlinear field line random walk for non-Gaussian statistics
• Nearly incompressible fluids. II: Magnetohydrodynamics, turbulence, and waves
• The influence of a mean magnetic field on three-dimensional magnetohydrodynamic turbulence
• Generalized compound transport of charged particles in turbulent magnetized plasmas
• A new theory for perpendicular transport of cosmic rays
• Field line wandering and perpendicular scattering of charged particles in Alfvénic slab turbulence
• Analytical description of nonlinear cosmic ray scattering: isotropic and quasilinear regimes of pitch-angle diffusion

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