{
  "annotation_id": "ee876766-c811-474f-af5d-2709f09f2f76",
  "date_created": "2026-03-02T18:00:42.215000Z",
  "date_modified": "2026-03-02T18:00:42.215000Z",
  "file_hash": "00033eb56444b7b7bdcc5b44b389627dc21830800029192987ad955920595105",
  "private": false,
  "record": {
    "abstract": "New exact solutions of the steady and incompressible 2D MHD equations in\npolar coordinates are presented. The solutions describe the process of\nreconnective magnetic annihilation in a curved current layer. They are\nparticularly interesting for modeling magnetic reconnection in solar flares\ncaused by the interaction of three photospheric magnetic sources.",
    "arxiv_id": "physics/0212017",
    "authors": [
      "E. Tassi",
      "V. S. Titov",
      "G. Hornig"
    ],
    "categories": [
      "physics.plasm-ph",
      "physics.space-ph"
    ],
    "doi": "10.1016/S0375-9601(02)01174-X",
    "journal_ref": "Physics Letters A 302 (5-6) (2002) pp. 313-317",
    "title": "Exact solutions for magnetic annihilation in curvilinear geometry",
    "url": "https://arxiv.org/abs/physics/0212017"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "36c9e130-a57e-4924-95cc-ddcf408796fa",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}