Articolo in rivista, 2022, ENG, 10.1209/0295-5075/ac7250
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
Chaotic advection, turbulence, magnetohydrodynamics, chaos
Carbone Francesco, Sorriso Valvo Luca
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
CNR authors
External links
OAI-PMH: Dublin Core
OAI-PMH: Mods
OAI-PMH: RDF
URL: https://iopscience.iop.org/article/10.1209/0295-5075/ac7250/meta
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