{
  "id": "1607.02073",
  "version": "v1",
  "published": "2016-07-07T16:26:50.000Z",
  "updated": "2016-07-07T16:26:50.000Z",
  "title": "MHD turbulence and distributed chaos",
  "authors": [
    "A. Bershadskii"
  ],
  "categories": [
    "physics.flu-dyn"
  ],
  "abstract": "It is shown, using results of recent direct numerical simulations, that spectral properties of distributed chaos in MHD turbulence with zero mean magnetic field are similar to those of hydrodynamic turbulence. An exception is MHD spontaneous breaking of space translational symmetry, when the stretched exponential spectrum $\\exp(-k/k_{\\beta})^{\\beta}$ has $\\beta=4/7$.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2016-07-07T16:26:50.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "mhd turbulence",
      "distributed chaos",
      "zero mean magnetic field",
      "space translational symmetry",
      "direct numerical simulations"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}