{
  "annotation_id": "d1fb0d41-acc1-4f52-bbd3-f174d87eae97",
  "date_created": "2026-03-02T18:01:07.026000Z",
  "date_modified": "2026-03-02T18:01:07.026000Z",
  "file_hash": "4c08f19ae6d881838a755254dc55a66c84fb6259ab934e85f2d75966d905614b",
  "private": false,
  "record": {
    "abstract": "Measurements of fluctuations of electric fields in the frequency range from a\nfraction of one Hz to 12.5 Hz are presented, and corrected for the Lorentz\ntransformation of magnetic fluctuations to give the electric fields in the\nplasma frame. The electric fields are large enough to provide the dominant\nforce on the ions of the solar wind in the region near the ion cyclotron\nfrequency of protons, larger than the force due to magnetic fluctuations. They\nprovide sufficient velocity space diffusion or heating to counteract\nconservation of magnetic moment in the expanding solar wind to maintain nearly\nisotropic velocity distributions.",
    "arxiv_id": "physics/0602179",
    "authors": [
      "P. J. Kellogg",
      "S. D. Bale",
      "F. S. Mozer",
      "T. S. Horbury",
      "H. Reme"
    ],
    "categories": [
      "physics.space-ph"
    ],
    "doi": "10.1086/499265",
    "title": "Solar Wind Electric Fields in the Ion Cyclotron Frequency Range",
    "url": "https://arxiv.org/abs/physics/0602179"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "d76c063a-5d08-461c-9d63-db2c013c6a7c",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}