Articolo in rivista, 2022, ENG, 10.1209/0295-5075/ac7250

Chaotic advection and particle pairs diffusion in a low-dimensional truncation of two-dimensional magnetohydrodynamics

Carbone F.; Telloni D.; Zank G.; Sorriso-Valvo L.

CNR, Institute of Atmospheric Pollution Research, C/o University of Calabria, Rende, Italy; National Institute for Astrophysics, Astrophysical Observatory of Torino, Pino Torinese, Italy; Center for Space Plasma and Aeronomic Research (CSPAR), University of Alabama in Huntsville, AL USA; Department of Space Science, University of Alabama in Huntsville, AL USA; Swedish Institute of Space Physics, Angstrom Laboratory, Uppsala, Sweden; CNR, Istituto per la Scienza e Tecnologia dei Plasmi, Section of Bari, Italy.

The chaotic advection of fluid particle pairs is investigated though a low-order model of two-dimensional magnetohydrodynamic (MHD), where only five nonlinearly interacting modes are retained. The model is inthrinsically inhomogeneous and anisotropic because of the influence of large-scale fluctuations. Therefore, even though dynamically chaotic, the fields are unable to form the typical scaling laws of fully developed turbulence. Results show that a super-ballistic dynamics, reminiscent of the Richardson law of particle-pairs diffusion in turbulent flows, is robustly obtained using the truncated model. Indeed, even in the strongly reduced truncation presented here, particle diffusion in MHD turbulence has the same laws as the separation of velocity of particle pairs. The inherent anisotropy only affects the scaling of diffusivity, by enhancing the diffusion properties along one direction for small time-scales. Finally, when further anisotropy is introduced in the system through Alfvén waves, fluid particles are trapped by these, and super-ballistic diffusion is replaced by Brownian-like diffusion. On the other hand, when the magnetic field is removed, the kinetic counterpart of the model does not show super-ballistic dynamics.

Europhysics letters (Print) 138 (5), pp. 53001-1–53001-7

Keywords

Chaotic advection, turbulence, magnetohydrodynamics, chaos

CNR authors

Carbone Francesco, Sorriso Valvo Luca

CNR institutes

IIA – Istituto sull'inquinamento atmosferico, ISTP – Istituto per la Scienza e Tecnologia dei Plasmi

ID: 468731

Year: 2022

Type: Articolo in rivista

Creation: 2022-06-27 13:39:34.000

Last update: 2022-06-30 16:44:12.000

External IDs

CNR OAI-PMH: oai:it.cnr:prodotti:468731

DOI: 10.1209/0295-5075/ac7250

Scopus: 2-s2.0-85132127821

ISI Web of Science (WOS): 000810183900001