pith. sign in

arxiv: 1306.1380 · v1 · pith:67HIQLW7new · submitted 2013-06-06 · ⚛️ physics.flu-dyn · astro-ph.SR· physics.plasm-ph

The origins of k⁻² spectrum in the decaying Taylor-Green magnetohydrodynamic turbulent flows

classification ⚛️ physics.flu-dyn astro-ph.SRphysics.plasm-ph
keywords flowmagneticspectrumtaylor-greencurrentdecayingdiscontinuitiesenergy
0
0 comments X
read the original abstract

We investigate the origins of $k^{-2}$ spectrum in a decaying Taylor-Green magnetohydrodynamic flow with zero large scale magnetic flux that was reported in Lee et al. (2010). A possible candidate for this scaling exponent has been the weak turbulence phenomenology. From our numerical simulations, we observe that current sheets in the magnetic Taylor-Green flow are formed in regions of magnetic discontinuities. Based on this observation and by studying the influence of the current sheets on the energy spectrum, using a filtering technique, we argue that the discontinuities are responsible for the $-2$ power law scaling of the energy spectra of this flow.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.