{
  "annotation_id": "cf82f4fe-cbfd-49f9-bfeb-88824c539de7",
  "date_created": "2026-03-02T18:00:39.220000Z",
  "date_modified": "2026-03-02T18:00:39.220000Z",
  "file_hash": "3fe4bace0b344dc4b266d83c4dae819d1600a634ceee28768491a6802f4727f9",
  "private": false,
  "record": {
    "abstract": "This work is devoted to the study of solar light that experiences single and\nmultiple scattering in the atmosphere at the twilight time. The work is based\non polarimetric observations of the twilight sky that were conducted in 1997\nand 2000 for different color bands. Basing on the results of observations, the\ncontribution of single-scattered light depending on the wavelength for the\nlight stage of twilight is obtained. The correlation of color and polarization\nproperties of the twilight sky is investigated with an account of multiple\nscattering",
    "arxiv_id": "physics/0112090",
    "authors": [
      "O. S. Ougolnikov",
      "I. A. Maslov"
    ],
    "categories": [
      "physics.ao-ph",
      "physics.geo-ph"
    ],
    "title": "Multi-Color Polarimetry of the Twilight Sky. The Role of Multiple   Scattering as the Function of Wavelength",
    "url": "https://arxiv.org/abs/physics/0112090"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "31d92d5f-e5c8-4c18-a46c-1af8823fe5e0",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}