{
  "annotation_id": "e1477dc5-1f8f-4dd3-a2cf-963520c643ae",
  "date_created": "2026-03-02T18:01:18.556000Z",
  "date_modified": "2026-03-02T18:01:18.556000Z",
  "file_hash": "3781027285f5ccdb203a366fb00b82e3c878ff06b4bba73d4d2eb519715128da",
  "private": false,
  "record": {
    "abstract": "A simple model collisionless, dissipative, compressible MHD (Alfvenic)\nturbulence in a magnetized system is investigated. In contrast to more familiar\nparadigms of turbulence, dissipation arises from Landau damping, enters via\nnonlinearity, and is distributed over all scales. The theory predicts that two\ndifferent regimes or phases of turbulence are possible, depending on the ratio\nof steepening to damping coefficient (m_1/m_2). For strong damping\n(|m_1/m_2|\u003c1), a regime of smooth, hydrodynamic turbulence is predicted. For\n|m_1/m_2|\u003e1, steady state turbulence does not exist in the hydrodynamic limit.\nRather, spikey, small scale structure is predicted.",
    "arxiv_id": "physics/9612005",
    "authors": [
      "M. V. Medvedev",
      "P. H. Diamond"
    ],
    "categories": [
      "physics.plasm-ph",
      "adap-org",
      "astro-ph",
      "nlin.AO",
      "physics.space-ph"
    ],
    "doi": "10.1103/PhysRevE.56.R2371",
    "journal_ref": "Phys. Rev. E 56, R2371-R2374 (1997)",
    "title": "Towards a Simple Model of Compressible Alfvenic Turbulence",
    "url": "https://arxiv.org/abs/physics/9612005"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "0f5dcffd-4ca7-468a-b4eb-99fd4995eadf",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}