{
  "annotation_id": "fb931f57-756c-433f-881a-df5d82a3c915",
  "date_created": "2026-03-02T18:00:56.450000Z",
  "date_modified": "2026-03-02T18:00:56.450000Z",
  "file_hash": "4d03394c1f024ee0f898951084e1ed72ba9cb0ad583ac53e54e5c4a73d7890e8",
  "private": false,
  "record": {
    "abstract": "We will in this paper report on suggestive similarities between density\nfluctuation power versus wavenumber on small (mm) and large (Mpc) scales. The\nsmall scale measurements were made in fusion plasmas and compared to\npredictions from classical fluid turbulence theory. The data is consistent with\nthe dissipative range of 2D turbulence. Alternatively, the results can be\nfitted to a functional form that can not be explained by turbulence theory. The\nlarge scale measurements were part of the Sloan Digital Sky Survey galaxy\nredshift examination. We found that the equations describing fusion plasmas\nalso hold for the galaxy data. The comparable dependency of density fluctuation\npower on wavenumber in fusion plasmas and galaxies might indicate a common\norigin of these fluctuations.",
    "arxiv_id": "physics/0501114",
    "authors": [
      "N. P. Basse"
    ],
    "categories": [
      "physics.plasm-ph",
      "astro-ph"
    ],
    "doi": "10.1016/j.physleta.2005.04.033",
    "journal_ref": "Phys.Lett. A340 (2005) 456-460",
    "title": "Density fluctuations on mm and Mpc scales",
    "url": "https://arxiv.org/abs/physics/0501114"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "24feb7d2-1c81-4628-8043-8f78d2d2016a",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}