"hyperflare" meaning in All languages combined

{
  "etymology_templates": [
    {
      "args": {
        "1": "en",
        "2": "hyper",
        "3": "flare"
      },
      "expansion": "hyper- + flare",
      "name": "prefix"
    }
  ],
  "etymology_text": "hyper- + flare",
  "forms": [
    {
      "form": "hyperflares",
      "tags": [
        "plural"
      ]
    }
  ],
  "head_templates": [
    {
      "args": {},
      "expansion": "hyperflare (plural hyperflares)",
      "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": "English terms prefixed with hyper-",
          "parents": [],
          "source": "w"
        },
        {
          "kind": "topical",
          "langcode": "en",
          "name": "Astronomy",
          "orig": "en:Astronomy",
          "parents": [
            "Sciences",
            "Space",
            "All topics",
            "Nature",
            "Fundamental"
          ],
          "source": "w"
        }
      ],
      "examples": [
        {
          "ref": "2005, Arnon Dar, Hyperstars - Main Origin of Short Gamma Ray Bursts?, page 8",
          "text": "Such hyperflares may be the result of phase transitions from neutron matter to hyperon or strange-quark matter in hyperstars.",
          "type": "quotation"
        },
        {
          "ref": "2006, Tod E. Strohmeyer, Anna L. Watts, The 2004 Hyperflare from SGR 1806-20: Further Evidence for Global Torsional Vibrations, page 1",
          "text": "We report an analysis of archival RXTE data from the 2004 December hyperflare from SGR 1806-20.",
          "type": "quotation"
        },
        {
          "ref": "2014, Advanced Interferometers and the Search for Gravitational Waves: Lectures from the First VESF School on Advanced Detectors for Gravitational Waves, Springer International Publishing, page 41",
          "text": "For hyperflare events occurring at the time of advanced detector operation, the observable GW energetics at 100 Hz would be close to to 10⁻³⁶J, leading to stringent constraints on the magnetar model.",
          "type": "quotation"
        },
        {
          "ref": "2019, Particle Physics At The Silver Jubilee of Lomonosov Conferences - Proceedings of The Eighteenth Lomonosov Conference On Elementary Particle Physics, World Scientific Publishing Company, page 294",
          "text": "This seems very plausible, as statistical and energetic considerations allow one to explain basic properties of FRBs with transformation of a tiny fraction (~10⁻⁵) of the magnetar hyperflare (~10⁻⁴⁴ -10⁻⁴⁶ erg) into a short radio burst.",
          "type": "quotation"
        }
      ],
      "glosses": [
        "An extraordinarily powerful, massive flare, usually produced by a magnetar."
      ],
      "id": "en-hyperflare-en-noun-IaeGPdMe",
      "links": [
        [
          "astronomy",
          "astronomy"
        ],
        [
          "extraordinarily",
          "extraordinarily"
        ],
        [
          "powerful",
          "powerful"
        ],
        [
          "massive",
          "massive"
        ],
        [
          "flare",
          "flare"
        ],
        [
          "magnetar",
          "magnetar"
        ]
      ],
      "raw_glosses": [
        "(astronomy, very rare) An extraordinarily powerful, massive flare, usually produced by a magnetar."
      ],
      "synonyms": [
        {
          "word": "hyper flare"
        },
        {
          "word": "hyper-flare"
        }
      ],
      "tags": [
        "rare"
      ],
      "topics": [
        "astronomy",
        "natural-sciences"
      ]
    }
  ],
  "sounds": [
    {
      "ipa": "/ˈhaɪ.pə(ɹ)flɛə̯/"
    }
  ],
  "word": "hyperflare"
}

{
  "etymology_templates": [
    {
      "args": {
        "1": "en",
        "2": "hyper",
        "3": "flare"
      },
      "expansion": "hyper- + flare",
      "name": "prefix"
    }
  ],
  "etymology_text": "hyper- + flare",
  "forms": [
    {
      "form": "hyperflares",
      "tags": [
        "plural"
      ]
    }
  ],
  "head_templates": [
    {
      "args": {},
      "expansion": "hyperflare (plural hyperflares)",
      "name": "en-noun"
    }
  ],
  "lang": "English",
  "lang_code": "en",
  "pos": "noun",
  "senses": [
    {
      "categories": [
        "English 3-syllable words",
        "English countable nouns",
        "English entries with incorrect language header",
        "English lemmas",
        "English nouns",
        "English terms prefixed with hyper-",
        "English terms with IPA pronunciation",
        "English terms with quotations",
        "English terms with rare senses",
        "Quotation templates to be cleaned",
        "en:Astronomy"
      ],
      "examples": [
        {
          "ref": "2005, Arnon Dar, Hyperstars - Main Origin of Short Gamma Ray Bursts?, page 8",
          "text": "Such hyperflares may be the result of phase transitions from neutron matter to hyperon or strange-quark matter in hyperstars.",
          "type": "quotation"
        },
        {
          "ref": "2006, Tod E. Strohmeyer, Anna L. Watts, The 2004 Hyperflare from SGR 1806-20: Further Evidence for Global Torsional Vibrations, page 1",
          "text": "We report an analysis of archival RXTE data from the 2004 December hyperflare from SGR 1806-20.",
          "type": "quotation"
        },
        {
          "ref": "2014, Advanced Interferometers and the Search for Gravitational Waves: Lectures from the First VESF School on Advanced Detectors for Gravitational Waves, Springer International Publishing, page 41",
          "text": "For hyperflare events occurring at the time of advanced detector operation, the observable GW energetics at 100 Hz would be close to to 10⁻³⁶J, leading to stringent constraints on the magnetar model.",
          "type": "quotation"
        },
        {
          "ref": "2019, Particle Physics At The Silver Jubilee of Lomonosov Conferences - Proceedings of The Eighteenth Lomonosov Conference On Elementary Particle Physics, World Scientific Publishing Company, page 294",
          "text": "This seems very plausible, as statistical and energetic considerations allow one to explain basic properties of FRBs with transformation of a tiny fraction (~10⁻⁵) of the magnetar hyperflare (~10⁻⁴⁴ -10⁻⁴⁶ erg) into a short radio burst.",
          "type": "quotation"
        }
      ],
      "glosses": [
        "An extraordinarily powerful, massive flare, usually produced by a magnetar."
      ],
      "links": [
        [
          "astronomy",
          "astronomy"
        ],
        [
          "extraordinarily",
          "extraordinarily"
        ],
        [
          "powerful",
          "powerful"
        ],
        [
          "massive",
          "massive"
        ],
        [
          "flare",
          "flare"
        ],
        [
          "magnetar",
          "magnetar"
        ]
      ],
      "raw_glosses": [
        "(astronomy, very rare) An extraordinarily powerful, massive flare, usually produced by a magnetar."
      ],
      "tags": [
        "rare"
      ],
      "topics": [
        "astronomy",
        "natural-sciences"
      ]
    }
  ],
  "sounds": [
    {
      "ipa": "/ˈhaɪ.pə(ɹ)flɛə̯/"
    }
  ],
  "synonyms": [
    {
      "word": "hyper flare"
    },
    {
      "word": "hyper-flare"
    }
  ],
  "word": "hyperflare"
}