CLIMATE SIMULATION OF THE LATEST PERMIAN: IMPLICATIONS FOR MASS EXTINCTION

dc.contributor.author	Kiehl J.T.
dc.contributor.author	Shields C.A.
dc.date.accessioned	2023-11-26T02:22:38Z
dc.date.available	2023-11-26T02:22:38Z
dc.date.issued	2005
dc.identifier	https://www.elibrary.ru/item.asp?id=14564806
dc.identifier.citation	Geology, 2005, 33, 9, 757-760
dc.identifier.issn	0091-7613
dc.identifier.uri	https://repository.geologyscience.ru/handle/123456789/41987
dc.description.abstract	Life at the Permian-Triassic boundary (ca. 251 Ma) underwent the largest disruption in Earth's history. Paleoclimatic data indicate that Earth was significantly warmer than present and that much of the ocean was anoxic or euxinic for an extended period of time. We present results from the first fully coupled comprehensive climate model using paleo- geography for this time period. The coupled climate system model simulates warm high- latitude surface air temperatures related to elevated carbon dioxide levels and a stagnate global ocean circulation in concert with paleodata indicating low oxygen levels at ocean depth. This is the first climate simulation that captures these observed features of this time period.
dc.subject	Permian
dc.title	CLIMATE SIMULATION OF THE LATEST PERMIAN: IMPLICATIONS FOR MASS EXTINCTION
dc.type	Статья
dc.identifier.doi	10.1130/G21654.1
dc.subject.age	Paleozoic::Permian

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