{
  "annotation_id": "7b1f44eb-6b08-478d-a0ce-a871c069cbf0",
  "date_created": "2026-03-02T18:00:36.214000Z",
  "date_modified": "2026-03-02T18:00:36.214000Z",
  "file_hash": "6ca1a0a6586dd54ad4e82378401ad21afa4f5ffd1344fe4da63065cde2ea9a3e",
  "private": false,
  "record": {
    "abstract": "We discuss the question as to how the magnetospheric energy source feeds the\nionospheric current system.\n  It is shown that a consistent application and further development of Kennel\u0027s\nideas makes it possible to successfully solve the magnetosphere-ionosphere\ncoupling problem in regard to the formation of auroral electrojets by steady\nvolume currents generated in the magnetosphere by the magnetospheric MHD\ngenerator in the case of a simple model which, nevertheless, retains the\nessential features of the reality. It is concluded that the whole of the\ncomplicated magnetospheric \u0027\u0027design\u0027\u0027 only acts to redistribute, in space and\ntime, currents and energy fluxes which must be supplied by external sources to\nfeed the dissipative processes in the ionosphere.",
    "arxiv_id": "physics/0110048",
    "authors": [
      "P. A. Sedykh",
      "E. A. Ponomarev"
    ],
    "categories": [
      "physics.geo-ph"
    ],
    "title": "Magnetosphere-Ionosphere Coupling in the Region of Auroral Electrojets",
    "url": "https://arxiv.org/abs/physics/0110048"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "a154109b-e9b1-47ba-858c-225ca8dd64ff",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}