{
  "annotation_id": "87f4a556-83f4-460d-a8a0-010b8ab22088",
  "date_created": "2026-03-02T18:01:10.129000Z",
  "date_modified": "2026-03-02T18:01:10.129000Z",
  "file_hash": "42cb2ee43b5c2662a57212849d9e78457270d35b46684946d693574ae5622c28",
  "private": false,
  "record": {
    "abstract": "Solar wind turbulence is dominated by Alfv\\\u0027{e}nic fluctuations but the power\nspectral exponents somewhat surprisingly evolve toward the Kolmogorov value of\n-5/3, that of hydrodynamic turbulence. We show that at 1AU the turbulence\ndecomposes linearly into two coexistent components perpendicular and parallel\nto the local average magnetic field. The first of these is consistent with\npropagating Alfv\\\u0027{e}n wavepackets and shows the scaling expected of\nAlfv\\\u0027{e}nic turbulence, namely Irosnikov- Kraichnan. The second shows\nKolmogorov scaling which we also find in the number and magnetic energy\ndensity, and Poynting flux.",
    "arxiv_id": "physics/0606106",
    "authors": [
      "S. C. Chapman",
      "B. Hnat"
    ],
    "categories": [
      "physics.plasm-ph",
      "physics.flu-dyn"
    ],
    "doi": "10.1029/2007GL030518",
    "journal_ref": "Chapman, S. C., and B. Hnat (2007), Quantifying scaling in the\n  velocity field of the anisotropic turbulent solar wind, Geophys. Res. Lett.,\n  34, L17103",
    "title": "Kolmogorov and Irosnikov-Kraichnan scaling in the anisotropic turbulent   solar wind",
    "url": "https://arxiv.org/abs/physics/0606106"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "3dc0d73a-08e3-45db-99ea-6cd68846c711",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}