{
  "annotation_id": "442a69af-c732-4530-970a-e1c9021da981",
  "date_created": "2026-03-02T18:01:18.025000Z",
  "date_modified": "2026-03-02T18:01:18.025000Z",
  "file_hash": "ae636bd48becd4b6fcac06cf33c383dde023541daedbf538730dbfc71f56e92f",
  "private": false,
  "record": {
    "abstract": "We derive a new shell model of magnetohydrodynamic (MHD) turbulence in which\nthe energy transfers are not necessary local. Like the original MHD equations,\nthe model conserves the total energy, magnetic helicity, cross-helicity and\nvolume in phase space (Liouville\u0027s theorem) apart from the effects of external\nforcing, viscous dissipation and magnetic diffusion. In the absence of magnetic\nfield the model exhibits a statistically stationary kinetic energy solution\nwith a Kolmogorov spectrum. The dynamo action from a seed magnetic field by the\nturbulent flow and the non linear interactions are studied for a wide range of\nmagnetic Prandtl numbers in both kinematic and dynamic cases. The non locality\nof the energy transfers are clearly identified.",
    "arxiv_id": "physics/0701141",
    "authors": [
      "F. Plunian",
      "R. Stepanov"
    ],
    "categories": [
      "physics.flu-dyn",
      "physics.plasm-ph"
    ],
    "title": "A non local shell model of turbulent dynamo",
    "url": "https://arxiv.org/abs/physics/0701141"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "031fde97-0b44-4f94-aefd-daa5ad7d1925",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}