Abstract
The correlation time of the velocity in a magnetohydrodynamic flow plays an important role in several models of dynamo theory. In particular δ-correlated flows and asymptotic analyses for very small correlation times have been often considered in the study of kinematic dynamos with random plasma flows. It is rigorously proved here that the correlation time in a real flow is bounded below by a positive quantity depending only on the total enstrophy. As a consequence, two-dimensional flows as well as physically realistic three-dimensional ones, including the classical models of homogeneous turbulence, posses a minimum correlation time weakly dependent on the initial condition. This emphasises the need to be cautious when taking random flows as depicting real physical processes.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.