@prefix skos: <http://www.w3.org/2004/02/skos/core#> .
@prefix dc: <http://purl.org/dc/terms/> .
@prefix xsd: <http://www.w3.org/2001/XMLSchema#> .

<http://astrothesaurus.org/uat/1662>
  skos:prefLabel "Supergranulation"@en ;
  a skos:Concept ;
  skos:broader <http://astrothesaurus.org/uat/1498> .

<http://astrothesaurus.org/uat/2102>
  skos:prefLabel "Stellar granulation"@en ;
  a skos:Concept ;
  skos:related <http://astrothesaurus.org/uat/1498> .

<http://astrothesaurus.org/uat/1028>
  skos:prefLabel "Mesogranulation"@en ;
  a skos:Concept ;
  skos:broader <http://astrothesaurus.org/uat/1498> .

<http://astrothesaurus.org/uat/1498>
  dc:modified "2020-11-04T15:22:27.01Z"^^xsd:dateTime, "2020-11-04T15:22:15.205Z"^^xsd:dateTime ;
  skos:prefLabel "Solar granulation"@en ;
  skos:related <http://astrothesaurus.org/uat/1875>, <http://astrothesaurus.org/uat/2102> ;
  skos:broader <http://astrothesaurus.org/uat/1476> ;
  skos:editorialNote [ ] ;
  dc:contributor <http://editor.vocabs.ands.org.au/user/AAS_Frey.Katie_Admin> ;
  skos:narrower <http://astrothesaurus.org/uat/1662>, <http://astrothesaurus.org/uat/1028> ;
  a skos:Concept ;
  skos:definition "The mottled appearance of the solar photosphere, caused by convective cells, resembling granules, which rises from the interior of the Sun. Each granule has a mean size of about 1,000 km and an upward velocity of about 0.5 km/sec. Granules are separated by intergranular walls about 400 K colder. They emerge from the fragments of the preceding granules and their lifetimes are about 20 minutes."@en .

<http://astrothesaurus.org/uat/1875>
  skos:prefLabel "Solar granules"@en ;
  a skos:Concept ;
  skos:related <http://astrothesaurus.org/uat/1498> .

<http://astrothesaurus.org/uat/1476>
  skos:prefLabel "Solar physics"@en ;
  a skos:Concept ;
  skos:narrower <http://astrothesaurus.org/uat/1498> .

