{
  "annotation_id": "faf03108-41da-4ed8-b4d7-e739bab15461",
  "date_created": "2026-03-02T18:00:42.995000Z",
  "date_modified": "2026-03-02T18:00:42.995000Z",
  "file_hash": "e22455db015b4d55d28fa1633f72afbfdae9196a98bbe07f92d154a1c869f3dd",
  "private": false,
  "record": {
    "abstract": "Analytical solutions for reconnective annihilation in curvilinear geometry\nare presented. These solutions are characterized by current density\ndistributions varying both along the radial and azimuthal coordinates. They\nrepresent an extension of previously proposed models, based on purely radially\ndependent current densities. Possible applications of these solutions to the\nmodeling of solar flares are also discussed.",
    "arxiv_id": "physics/0305105",
    "authors": [
      "E. Tassi",
      "V. S. Titov",
      "G. Hornig"
    ],
    "categories": [
      "physics.plasm-ph",
      "physics.space-ph"
    ],
    "doi": "10.1016/S0375-9601(03)01104-6",
    "title": "New classes of exact solutions for magnetic reconnective annihilation",
    "url": "https://arxiv.org/abs/physics/0305105"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "62265c25-4602-43e5-baa7-7e3c1dce1b9e",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}