{
  "annotation_id": "dd6a6c79-e82e-48f0-9a6d-e89b6c5227ed",
  "date_created": "2026-03-02T18:01:10.682000Z",
  "date_modified": "2026-03-02T18:01:10.682000Z",
  "file_hash": "93017d04c0ce6e297b569c0395400c1702281b7bff6febe39952a0dcc859040c",
  "private": false,
  "record": {
    "abstract": "The anisotropy of magnetophydrodynamic turbulence is investigated by using\nsolar wind data from the Helios 2 spacecraft. We investigate the behaviour of\nthe complete high-order moment tensors of magnetic field increments and we\ncompare the usual longitudinal structure functions which have both isotropic\nand anisotropic contributions, to the fully anisotropic contribution. Scaling\nexponents have been extracted by an interpolation scaling function. Unlike the\nusual turbulence in fluid flows, small-scale magnetic fluctuations remain\nanisotropic. We discuss the radial dependence of both anisotropy and\nintermittency and their relationship.",
    "arxiv_id": "physics/0607128",
    "authors": [
      "Luca Sorriso-Valvo",
      "Vincenzo Carbone",
      "Roberto Bruno",
      "Pierluigi Veltri"
    ],
    "categories": [
      "physics.space-ph",
      "physics.data-an",
      "physics.plasm-ph"
    ],
    "doi": "10.1209/epl/i2006-10172-y",
    "title": "Persistence of small-scale anisotropy of magnetic turbulence as observed   in the solar wind",
    "url": "https://arxiv.org/abs/physics/0607128"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "48a7209d-fadc-4553-bb83-7b81c5a23eb8",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}