Abstract

The stochastic behavior of magnetic field lines in turbulence is explored analytically and numerically. This problem is a fundamental aspect of turbulence research but also highly relevant in the theory of energetic particles. In the current paper, previous approaches are reviewed and some simple heuristic arguments are provided helping the reader to understand the reason for the form of analytical results. The importance of the so-called Kubo number in field line random walk theory is also discussed. Furthermore, analytical results for a position-dependent field line diffusion coefficient are provided. For more realistic turbulence configurations, the field line diffusion coefficients are computed numerically. This includes quasi-slab, quasi-2D, two-component, and three-dimensional turbulence. Specific aspects of the field line random walk in each model are also discussed. Results based on a diffusion approximation are compared with numerical results obtained without employing this approximation with the aim to explore its validity and accuracy. Numerical results based on simulations for incompressible and compressible turbulence are also discussed.

Highlights

  • A fundamental problem of modern space and astrophysics is the understanding of turbulence

  • We focus on the basic physics of field line random walk (FLRW), the importance of the Kubo number, and present some simple heuristic arguments with the aim to find analytical forms for the field line diffusion coefficient

  • We have reviewed the random walk of magnetic field lines

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Summary

Shalchi

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INTRODUCTION
BASIC EQUATIONS AND HEURISTIC ARGUMENTS
More on the physics of FLRW
Field line equations and the Kubo number
The initial ballistic regime
Heuristic arguments
The non-linear field line random walk equation
B20 ð d3k ð d3k0
Slab turbulence
The quasi-linear approximation
Two-dimensional turbulence
The diffusion approximation
Two-component turbulence
Three-dimensional turbulence
Magnetic correlations along the field lines
SIMULATIONS OF FLRW
Magnetic field generation for two-component turbulence
Obtaining field lines and their statistics
Compressible isotropic turbulence
SUMMARY AND CONCLUSION
À 1K2 6
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