{
  "annotation_id": "06383701-83d6-4f16-8683-244ab303a567",
  "date_created": "2026-03-02T18:00:50.320000Z",
  "date_modified": "2026-03-02T18:00:50.320000Z",
  "file_hash": "1b71a32bf4a3eaa410ba347dbf37c0c842dbcbf89110b6a0091f3b152e907a58",
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  "record": {
    "abstract": "The interplanetary induced electric field e=vxb is studied, using solar wind\ntime series. The probability distribution functions (PDFs) of the electric\nfield components are measured from the data and their non-gaussianity is\ndiscussed. Moreover, for the first time we show that the electric field\nturbulence is characterized by intermittency. This point is addressed by\nstudying, as usual, the scaling of the PDFs of field increments, which allows a\nquantitative characterization of intermittency.",
    "arxiv_id": "physics/0405138",
    "authors": [
      "Luca Sorriso-Valvo",
      "Vincenzo Carbone",
      "Roberto Bruno"
    ],
    "categories": [
      "physics.space-ph",
      "astro-ph",
      "nlin.CD",
      "physics.plasm-ph"
    ],
    "doi": "10.1209/epl/i2003-10294-8",
    "journal_ref": "Europhys.Lett. 67 (2004) 504",
    "title": "One-point statistics and intermittency of induced electric field in the   solar wind",
    "url": "https://arxiv.org/abs/physics/0405138"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "d3319cca-0827-4c75-994c-c32e22621dc2",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}