English

Magnetic fields from Multiplicative Chaos

Astrophysics of Galaxies 2020-06-10 v1 Cosmology and Nongalactic Astrophysics Solar and Stellar Astrophysics Fluid Dynamics Plasma Physics

Abstract

An analytical model for fully developed three-dimensional incompressible turbulence was recently proposed in the hydrodynamics community, based on the concept of multiplicative chaos. It consists of a random field represented by means of a stochastic integral, which, with only a few parameters, shares many properties with experimental and numerical turbulence, including in particular energy transfer through scales (the cascade) and intermittency (non-Gaussianity) which is most conveniently controlled with a single parameter. Here, we propose three models extending this approach to MHD turbulence. Our formulae provide physically motivated 3D models of a turbulent velocity field and magnetic field coupled together. Besides its theoretical value, this work is meant to provide a tool for observers: a dozen of physically meaningful free parameters enter the description, which is useful to characterize astrophysical data.

Keywords

Cite

@article{arxiv.2005.11972,
  title  = {Magnetic fields from Multiplicative Chaos},
  author = {J. -B. Durrive and P. Lesaffre and K. Ferrière},
  journal= {arXiv preprint arXiv:2005.11972},
  year   = {2020}
}

Comments

22 pages, 9 figures, Accepted for publication in MNRAS

R2 v1 2026-06-23T15:47:00.915Z