{
  "annotation_id": "8ff1d03b-08a9-4605-b592-d5b4e86b5772",
  "date_created": "2026-03-02T18:00:29.382000Z",
  "date_modified": "2026-03-02T18:00:29.382000Z",
  "file_hash": "39472fc00b24836b04ec854944655babdb1dd34b61778e61edd3119e996a0bb8",
  "private": false,
  "record": {
    "abstract": "During major megnetic storms, enhanced flux of relativistic electrons in the\ninner magnetosphere have been observed to correleated with ULF waves. The\nenhancements can take place over a period of several hours. In order to account\nfor such a rapid generation of relativistic electrons, we examine the mechanism\nof transit-time acceleration of electrons by low-frequency fast-mode MHD waves,\nhere the assumed form of ULF waves. Calcaulations of the acceleration\ntimescales in the model show that fast-mode waves in the Pc4 to Pc5 frequency\nrange, with typically observed wave amplitudes 10--20 nT, can accelerate the\nseed electrons to energies of order MeV in a period of a few hours.",
    "arxiv_id": "physics/0003099",
    "authors": [
      "Danny Summers",
      "Chunyu Ma"
    ],
    "categories": [
      "physics.plasm-ph",
      "physics.space-ph"
    ],
    "doi": "10.1029/1999JA000408",
    "title": "Rapid acceleration of electrons in the magnetosphere by fast-mode MHD   waves",
    "url": "https://arxiv.org/abs/physics/0003099"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "32d481b9-32d6-4716-8452-ed709b85b91b",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}