{
  "annotation_id": "2b75ed87-75e6-439b-aa5f-56de947a98e6",
  "date_created": "2026-03-02T18:00:56.870000Z",
  "date_modified": "2026-03-02T18:00:56.870000Z",
  "file_hash": "1239ca267a556eeec2da7ed8f0192f69e23077119f062c1eb2ece5c627c8a086",
  "private": false,
  "record": {
    "abstract": "In addition to traditional regimes with monotonously increasing magnetic\nfield, regimes with \"magnetic wells\" also occur in spherical tokamaks (STs).\nThe magnetic field profile inversion modifies significantly the whole picture\nof the wave propagation and damping. Since the magnetic wells may become quite\ncommon with further improvement of ST performance, analysis of such\nconfigurations is of interest for assessment of EBW plasma heating an CD\nperspectives. In this paper the basic features of the EBWs propagation and\ndamping for the second cyclotron harmonic in a slab model are considered.",
    "arxiv_id": "physics/0412173",
    "authors": [
      "A. D. Piliya",
      "A. Yu. Popov",
      "E. N. Tregubova"
    ],
    "categories": [
      "physics.plasm-ph",
      "physics.gen-ph"
    ],
    "doi": "10.1088/0741-3335/47/11/011",
    "title": "Electron Bernstein waves in spherical tokamak plasmas with \"magnetic   wells\"",
    "url": "https://arxiv.org/abs/physics/0412173"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "17cbe50c-8646-44df-b79d-50ae5a605c78",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}