{
  "annotation_id": "ffbb963e-bcb2-4fc3-a8ad-4c169c086b64",
  "date_created": "2026-03-02T18:01:18.485000Z",
  "date_modified": "2026-03-02T18:01:18.485000Z",
  "file_hash": "106b4d0ec25044ebd2827b0c877323732c7e82bfa102d15b0a4a41c99753ec5e",
  "private": false,
  "record": {
    "abstract": "The saturation of ion cyclotron Alfven turbulence excited by beam particles\nis investigated using resonance broadening theory. The stochastic scattering\nwhich decorrelates particles, includes both random acceleration by electric\nfields and a turbulent magnetic mirroring effect. Turbulent mirroring is shown\nto yield non-Gaussian corrections to the orbits even if the random electric and\nmagnetic fields are Gaussian. The predicted steady-state turbulence level\nexhibits a peaked anglular distribution, with a maximum near Theta ~ 60\ndegrees.",
    "arxiv_id": "physics/9612019",
    "authors": [
      "M. V. Medvedev",
      "P. H. Diamond"
    ],
    "categories": [
      "physics.plasm-ph",
      "adap-org",
      "astro-ph",
      "nlin.AO",
      "physics.space-ph"
    ],
    "doi": "10.1016/0375-9601(96)00465-3",
    "journal_ref": "Phys. Letters A, v.219, p.293 (1996)",
    "title": "Resonance Broadening Induced Nonlinear Saturation of Kinetic Alfven   Turbulence in the Interplanetary Plasma",
    "url": "https://arxiv.org/abs/physics/9612019"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "c5fb7a14-5a72-4577-81ee-8457ad88ceb1",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}