{ "format" : "linked-data-api", "version" : "0.2", "result" : {"_about" : "https://vocabs.ardc.edu.au/repository/api/lda/aas/the-unified-astronomy-thesaurus/5-0-0/resource.text?uri=http%3A%2F%2Fastrothesaurus.org%2Fuat%2F2038", "definition" : "https://vocabs.ardc.edu.au/repository/api/lda/aas/the-unified-astronomy-thesaurus/5-0-0/resource.text?uri=http%3A%2F%2Fastrothesaurus.org%2Fuat%2F2038", "extendedMetadataVersion" : "https://vocabs.ardc.edu.au/repository/api/lda/aas/the-unified-astronomy-thesaurus/5-0-0/resource.text?_metadata=all&uri=http%3A%2F%2Fastrothesaurus.org%2Fuat%2F2038", "primaryTopic" : {"_about" : "http://astrothesaurus.org/uat/2038", "broader" : [{"_about" : "http://astrothesaurus.org/uat/1483", "narrower" : ["http://astrothesaurus.org/uat/2038"]} ], "contributor" : "http://editor.vocabs.ands.org.au/user/AAS_Frey.Katie_Admin", "creator" : "http://editor.vocabs.ands.org.au/user/AAS_Frey.Katie", "dctermsCreated" : "Fri, 07 Sep 2018 17:36:26 GMT+0000", "dctermsModified" : "Wed, 04 Nov 2020 15:05:33 GMT+0000", "definition" : "An emission line in the spectrum of the solar corona caused by highly ionized metal ions; especially those of iron, such as the red and green lines at 6375 Å and 5303 Å [Fe X] and [Fe XIV], respectively. From their discovery in 1870 until 1939, it was believed that these forbidden lines would be due to an unknown element, called coronium. Ultraviolet and X-ray coronal lines are also detectable in stars.", "prefLabel" : {"_value" : "Solar coronal lines", "_lang" : "en"} , "related" : [{"_about" : "http://astrothesaurus.org/uat/308", "related" : ["http://astrothesaurus.org/uat/2038"]} ], "type" : ["http://www.w3.org/2000/01/rdf-schema#Resource", "http://www.w3.org/2004/02/skos/core#Concept"]} , "type" : ["http://purl.org/linked-data/api/vocab#ItemEndpoint", "http://purl.org/linked-data/api/vocab#Page"]} }