"coreshine" meaning in All languages combined

{
  "etymology_templates": [
    {
      "args": {
        "1": "en",
        "2": "core",
        "3": "shine"
      },
      "expansion": "core + shine",
      "name": "compound"
    }
  ],
  "etymology_text": "From core + shine.",
  "head_templates": [
    {
      "args": {
        "1": "-"
      },
      "expansion": "coreshine (uncountable)",
      "name": "en-noun"
    }
  ],
  "lang": "English",
  "lang_code": "en",
  "pos": "noun",
  "senses": [
    {
      "categories": [
        {
          "kind": "other",
          "name": "English entries with incorrect language header",
          "parents": [
            "Entries with incorrect language header",
            "Entry maintenance"
          ],
          "source": "w"
        },
        {
          "kind": "other",
          "name": "Pages with 1 entry",
          "parents": [],
          "source": "w"
        },
        {
          "kind": "other",
          "name": "Pages with entries",
          "parents": [],
          "source": "w"
        },
        {
          "kind": "topical",
          "langcode": "en",
          "name": "Astronomy",
          "orig": "en:Astronomy",
          "parents": [
            "Sciences",
            "Space",
            "All topics",
            "Nature",
            "Fundamental"
          ],
          "source": "w"
        }
      ],
      "examples": [
        {
          "ref": "2015, J. Steinacker, M. Andersen, W.-F. Thi, R. Paladini, M. Juvela, A. Bacmann, V.-M. Pelkonen, L. Pagani, C. Lefèvre, Th. Henning, A. Noriega-Crespo, “Grain size limits derived from 3.6 μm and 4.5 μm coreshine”, in arXiv:",
          "text": "In the case of Rho Oph 9, we were unable to reliably disentangle the coreshine emission from background variations and the strong local PAH emission.",
          "type": "quote"
        }
      ],
      "glosses": [
        "infrared light scattered by unusually large grains of dust in the denser core regions of molecular clouds"
      ],
      "id": "en-coreshine-en-noun-53-XGFvN",
      "links": [
        [
          "astronomy",
          "astronomy"
        ],
        [
          "infrared",
          "infrared"
        ],
        [
          "light",
          "light"
        ],
        [
          "scatter",
          "scatter"
        ],
        [
          "grain",
          "grain"
        ],
        [
          "dust",
          "dust"
        ],
        [
          "molecular cloud",
          "molecular cloud"
        ]
      ],
      "raw_glosses": [
        "(astronomy) infrared light scattered by unusually large grains of dust in the denser core regions of molecular clouds"
      ],
      "tags": [
        "uncountable"
      ],
      "topics": [
        "astronomy",
        "natural-sciences"
      ],
      "wikipedia": [
        "coreshine"
      ]
    }
  ],
  "word": "coreshine"
}

{
  "etymology_templates": [
    {
      "args": {
        "1": "en",
        "2": "core",
        "3": "shine"
      },
      "expansion": "core + shine",
      "name": "compound"
    }
  ],
  "etymology_text": "From core + shine.",
  "head_templates": [
    {
      "args": {
        "1": "-"
      },
      "expansion": "coreshine (uncountable)",
      "name": "en-noun"
    }
  ],
  "lang": "English",
  "lang_code": "en",
  "pos": "noun",
  "senses": [
    {
      "categories": [
        "English compound terms",
        "English entries with incorrect language header",
        "English lemmas",
        "English nouns",
        "English terms with quotations",
        "English uncountable nouns",
        "Pages with 1 entry",
        "Pages with entries",
        "en:Astronomy"
      ],
      "examples": [
        {
          "ref": "2015, J. Steinacker, M. Andersen, W.-F. Thi, R. Paladini, M. Juvela, A. Bacmann, V.-M. Pelkonen, L. Pagani, C. Lefèvre, Th. Henning, A. Noriega-Crespo, “Grain size limits derived from 3.6 μm and 4.5 μm coreshine”, in arXiv:",
          "text": "In the case of Rho Oph 9, we were unable to reliably disentangle the coreshine emission from background variations and the strong local PAH emission.",
          "type": "quote"
        }
      ],
      "glosses": [
        "infrared light scattered by unusually large grains of dust in the denser core regions of molecular clouds"
      ],
      "links": [
        [
          "astronomy",
          "astronomy"
        ],
        [
          "infrared",
          "infrared"
        ],
        [
          "light",
          "light"
        ],
        [
          "scatter",
          "scatter"
        ],
        [
          "grain",
          "grain"
        ],
        [
          "dust",
          "dust"
        ],
        [
          "molecular cloud",
          "molecular cloud"
        ]
      ],
      "raw_glosses": [
        "(astronomy) infrared light scattered by unusually large grains of dust in the denser core regions of molecular clouds"
      ],
      "tags": [
        "uncountable"
      ],
      "topics": [
        "astronomy",
        "natural-sciences"
      ],
      "wikipedia": [
        "coreshine"
      ]
    }
  ],
  "word": "coreshine"
}