"Stefan-Boltzmann law" meaning in All languages combined

{
  "etymology_text": "Named after Josef Stefan and Ludwig Boltzmann.",
  "forms": [
    {
      "form": "the Stefan-Boltzmann law",
      "tags": [
        "canonical"
      ]
    }
  ],
  "head_templates": [
    {
      "args": {
        "def": "1"
      },
      "expansion": "the Stefan-Boltzmann law",
      "name": "en-proper noun"
    }
  ],
  "lang": "English",
  "lang_code": "en",
  "pos": "name",
  "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": "Physics",
          "orig": "en:Physics",
          "parents": [
            "Sciences",
            "All topics",
            "Fundamental"
          ],
          "source": "w"
        }
      ],
      "glosses": [
        "A law stating that the total energy radiated per unit surface area of a black body across all wavelengths per unit time is directly proportional to the fourth power of the black body's thermodynamic temperature."
      ],
      "id": "en-Stefan-Boltzmann_law-en-name--wMiAczX",
      "links": [
        [
          "physics",
          "physics"
        ],
        [
          "energy",
          "energy"
        ],
        [
          "radiate",
          "radiate"
        ],
        [
          "unit",
          "unit"
        ],
        [
          "surface area",
          "surface area"
        ],
        [
          "black body",
          "black body"
        ],
        [
          "wavelength",
          "wavelength"
        ],
        [
          "time",
          "time"
        ],
        [
          "directly proportional",
          "directly proportional"
        ],
        [
          "power",
          "power"
        ],
        [
          "thermodynamic",
          "thermodynamic"
        ],
        [
          "temperature",
          "temperature"
        ]
      ],
      "raw_glosses": [
        "(physics) A law stating that the total energy radiated per unit surface area of a black body across all wavelengths per unit time is directly proportional to the fourth power of the black body's thermodynamic temperature."
      ],
      "related": [
        {
          "word": "Stefan-Boltzmann constant"
        }
      ],
      "topics": [
        "natural-sciences",
        "physical-sciences",
        "physics"
      ],
      "wikipedia": [
        "Josef Stefan",
        "Ludwig Boltzmann",
        "Stefan-Boltzmann law"
      ]
    }
  ],
  "word": "Stefan-Boltzmann law"
}

{
  "etymology_text": "Named after Josef Stefan and Ludwig Boltzmann.",
  "forms": [
    {
      "form": "the Stefan-Boltzmann law",
      "tags": [
        "canonical"
      ]
    }
  ],
  "head_templates": [
    {
      "args": {
        "def": "1"
      },
      "expansion": "the Stefan-Boltzmann law",
      "name": "en-proper noun"
    }
  ],
  "lang": "English",
  "lang_code": "en",
  "pos": "name",
  "related": [
    {
      "word": "Stefan-Boltzmann constant"
    }
  ],
  "senses": [
    {
      "categories": [
        "English entries with incorrect language header",
        "English eponyms",
        "English lemmas",
        "English multiword terms",
        "English proper nouns",
        "English uncountable nouns",
        "Pages with 1 entry",
        "Pages with entries",
        "en:Physics"
      ],
      "glosses": [
        "A law stating that the total energy radiated per unit surface area of a black body across all wavelengths per unit time is directly proportional to the fourth power of the black body's thermodynamic temperature."
      ],
      "links": [
        [
          "physics",
          "physics"
        ],
        [
          "energy",
          "energy"
        ],
        [
          "radiate",
          "radiate"
        ],
        [
          "unit",
          "unit"
        ],
        [
          "surface area",
          "surface area"
        ],
        [
          "black body",
          "black body"
        ],
        [
          "wavelength",
          "wavelength"
        ],
        [
          "time",
          "time"
        ],
        [
          "directly proportional",
          "directly proportional"
        ],
        [
          "power",
          "power"
        ],
        [
          "thermodynamic",
          "thermodynamic"
        ],
        [
          "temperature",
          "temperature"
        ]
      ],
      "raw_glosses": [
        "(physics) A law stating that the total energy radiated per unit surface area of a black body across all wavelengths per unit time is directly proportional to the fourth power of the black body's thermodynamic temperature."
      ],
      "topics": [
        "natural-sciences",
        "physical-sciences",
        "physics"
      ],
      "wikipedia": [
        "Josef Stefan",
        "Ludwig Boltzmann",
        "Stefan-Boltzmann law"
      ]
    }
  ],
  "word": "Stefan-Boltzmann law"
}