{
  "annotation_id": "b9d54e06-08ed-4d56-b5b8-7e6ddcd7f13a",
  "date_created": "2026-03-02T18:00:35.871000Z",
  "date_modified": "2026-03-02T18:00:35.871000Z",
  "file_hash": "0722d595cf5c56325c2738d1db37f77dd7f494484d6a6bebaf305d217632ad94",
  "private": false,
  "record": {
    "abstract": "In this paper, the evolution of the induced axial magnetization due to the\npropagation of an electromagnetic (em) wave along the static background\nmagnetic field in a two-component plasma has been investigated using the Block\nequation. The evolution process induces a strong magnetic anisotropy in the\nplasma medium, depending nonlinearly on the incident wave amplitude. This\ninduced magnetic anisotropy can modify the dispersion relation of the incident\nem wave, which has been obtained in this paper. In the low frequency Alfven\nwave limit, this dispersion relation shows that the resulting phase velocity of\nthe incident wave depends on the square of the incident wave amplitude and on\nthe static background magnetic field of plasma. The analytical results are in\nwell agreement with the numerically estimated values in solar corona and\nsunspots.",
    "arxiv_id": "physics/0111011",
    "authors": [
      "S. Sarkar",
      "P. Mukhopadhyay",
      "M. Khan",
      "J. Ortner",
      "M. Steinberg",
      "W. Ebeling"
    ],
    "categories": [
      "physics.plasm-ph"
    ],
    "doi": "10.1103/PhysRevE.64.046401",
    "journal_ref": "Phys. Rev. E vol. 64 (2001), 046401",
    "title": "Evolution of induced axial magnetization in a two-component magnetized   plasma",
    "url": "https://arxiv.org/abs/physics/0111011"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "9ff3ef9b-31f4-4267-a741-c98c54c51475",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}