CLIMATE SIMULATION OF THE LATEST PERMIAN: IMPLICATIONS FOR MASS EXTINCTION

dc.contributor.authorKiehl J.T.
dc.contributor.authorShields C.A.
dc.date.accessioned2023-11-26T02:22:38Z
dc.date.available2023-11-26T02:22:38Z
dc.date.issued2005
dc.description.abstractLife 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.identifierhttps://www.elibrary.ru/item.asp?id=14564806
dc.identifier.citationGeology, 2005, 33, 9, 757-760
dc.identifier.doi10.1130/G21654.1
dc.identifier.issn0091-7613
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/41987
dc.subjectPermian
dc.subject.agePaleozoic::Permian
dc.titleCLIMATE SIMULATION OF THE LATEST PERMIAN: IMPLICATIONS FOR MASS EXTINCTION
dc.typeСтатья

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