{
  "annotation_id": "eb22a61e-36db-4bb8-92ad-d7ea4f0c7df7",
  "date_created": "2026-03-02T18:00:42.674000Z",
  "date_modified": "2026-03-02T18:00:42.674000Z",
  "file_hash": "13ae9b9434729b582d519be2f919f57285f5d1b88ed5bca9c43f536f5cd15d47",
  "private": false,
  "record": {
    "abstract": "The magnetic disturbances are associated with electric currents as it is well\nchecked at laboratory room scales and described by the Maxwell\u0027s equations of\nelectromagnetic field. The analysis of spacecraft observations for more than a\nquarter of a century failed to provide a self-consistent three-dimensional\npicture of the solar wind-magnetosphere dynamo generated magnetospheric and\nionospheric current systems. The proposed solar wind and the interplanetary\nmagnetic field (IMF) driven reconfiguration of the earth\u0027s magnetosphere\ndirectly accounts for the observed magnetic disturbances. So role of the\nmagnetospheric currents in creation of the magnetic disturbances is\nreconsidered in accordance with some poorly understood observations. A\nquantitative agreement with observations is demonstrated and a laboratory\nexperiment to test the suggested model of the solar wind/IMF-magnetosphere\ninteraction is described.",
    "arxiv_id": "physics/0212107",
    "authors": [
      "Eugene Savov"
    ],
    "categories": [
      "physics.space-ph",
      "physics.gen-ph"
    ],
    "title": "The Interplanetary Magnetic Field and Solar Wind Driven Magnetospheric   Reconfiguration",
    "url": "https://arxiv.org/abs/physics/0212107"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "bddd3bf1-c63b-4e01-98ff-fbfaee01d242",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}