pith. sign in

arxiv: nlin/0204026 · v1 · submitted 2002-04-14 · 🌊 nlin.CD · astro-ph· cond-mat

Comment on "On two-dimensional magnetohydrodynamic turbulence" [Phys. Plasmas, 8, 3282 (2001)]

classification 🌊 nlin.CD astro-phcond-mat
keywords magnetohydrodynamicphenomenologyturbulencetwo-dimensionalcommentenergyiroshnikov-kraichnanphys
0
0 comments X
read the original abstract

Biskamp and Schwarz [Phys. Plasmas, 8, 3282 (2001)] have reported that the energy spectrum of two-dimensional magnetohydrodynamic turbulence is proportional to $k^{-3/2}$, which is a prediction of Iroshnikov-Kraichnan phenomenology. In this comment we report some earlier results which conclusively show that for two-dimensional magnetohydrodynamic turbulence, Kolmogorov-like phenomenology (spectral index 5/3) is better model than Iroshnikov-Kraichnan phenomenology; these results are based on energy flux analysis.

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.