English

Weak Alfven-Wave Turbulence Revisited

Plasma Physics 2015-08-26 v1 Solar and Stellar Astrophysics Chaotic Dynamics Fluid Dynamics Space Physics

Abstract

Weak Alfvenic turbulence in a periodic domain is considered as a mixed state of Alfven waves interacting with the two-dimensional (2D) condensate. Unlike in standard treatments, no spectral continuity between the two is assumed and indeed none is found. If the 2D modes are not directly forced, k^{-2} and k^{-1} spectra are found for the Alfven waves and the 2D modes, respectively, with the latter less energetic than the former. The wave number at which their energies become comparable marks the transition to strong turbulence. For imbalanced energy injection, the spectra are similar and the Elsasser ratio scales as the ratio of the energy fluxes in the counterpropagting Alfven waves. If the 2D modes are forced, a 2D inverse cascade dominates the dynamics at the largest scales, but at small enough scales, the same weak and then strong regimes as described above are achieved.

Keywords

Cite

@article{arxiv.1110.6682,
  title  = {Weak Alfven-Wave Turbulence Revisited},
  author = {A. A. Schekochihin and S. V. Nazarenko and T. A. Yousef},
  journal= {arXiv preprint arXiv:1110.6682},
  year   = {2015}
}

Comments

revtex, 5 pages, 2 figures; submitted

R2 v1 2026-06-21T19:28:10.595Z