Cascade model for intermittency in fully developed magnetohydrodynamic turbulence

Vincenzo Carbone
Phys. Rev. Lett. 71, 1546 – Published 6 September 1993
PDFExport Citation

Abstract

Evidence of intermittency in the interplanetary space plasma has been recently pointed out. We present a magnetohydrodynamic (MHD) cascade model, derived from a binomial process, whose results fit the observed scaling law for the qth power of the structure functions. Using this model we modify the oldest Kraichnan theory showing, for the first time, the multifractal structure of fully developed MHD turbulence.

  • Received 8 June 1993

DOI:https://doi.org/10.1103/PhysRevLett.71.1546

©1993 American Physical Society

Authors & Affiliations

Vincenzo Carbone

  • Dipartimento di Fisica, Università della Calabria, I-87030 Rende (CS), Italy

References (Subscription Required)

Click to Expand
Issue

Vol. 71, Iss. 10 — 6 September 1993

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review Letters

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×