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Pleistocene surface-ocean changes across the Southern subtropical front recorded by cryptic species of Orbulina universa

dc.contributor.authorNirmal, B.
dc.contributor.authorMohan, K.
dc.contributor.authorPrakasam, M.
dc.contributor.authorTripati, Aradhna
dc.contributor.authorMortyn, P Graham
dc.contributor.authorRodriguez-Sanz, Laura
dc.date.accessioned2024-03-21T00:30:48Z
dc.date.issued2021
dc.date.updated2022-11-13T07:17:41Z
dc.description.abstractThe largest ocean temperature gradients occur in the Southern Ocean, where the Antarctic circumpolar current frontal systems serve as hydrographic barriers with distinctive flora and fauna. During Pleistocene glacial-interglacial cycles, the position and intensity of these frontal systems are thought to have changed. This study examines the occurrence of distinct cryptic species of Orbulina universa during the Mid-Pleistocene Transition at two sites in the South Atlantic, Ocean Drilling Program Holes 1088B and 1090B that are separated by 2° latitude. We discuss abundance records of the Caribbean and Mediterranean species and their relationship to Total Organic Carbon and stable isotope records to further understand the sea-surface changes of this region during the Pleistocene. Data from 1090B, the more southerly Hole, shows the presence of few Mediterranean species together with aberrant and Biorbulina bilobata forms. At ODP Hole1088B, on the other hand, the presence of both cryptic species are observed throughout the Pleistocene, indicating distinct surface water sources and properties. The abnormal forms indicate the possible disappearance of O. universa under stressful environmental conditions in the sub-antarctic zone with reseeding of the species at glacial-interglacial transitions (Marine isotopic stages 23/22, 14/13, 8/7 and 2/1). Although nutrient-rich surface waters and shallow nutricline favours high productivity in this region during glacial intervals, it is possible that Mediterranean species at 1090B would have been restricted by cold sub-polar surface waters. Comparison with published data suggests that the presence of subtropical Caribbean species at 1088B was driven by the prominence of northern sourced waters and interocean exchange south of Africa. Our data point to the presence of sub-tropical waters at 1088B during each glacial-interglacial transition with maxima occurring at three intervals (1200 ka, 700–600 ka and 250–100 ka) that coincide with the inception of the Mid-Pleistocene Transition and sea surface temperatures changes at the subtropical front. The interocean transfer and surface water changes at the subtropical front in the late Pleistocene are consistent with modulation by eccentricity-induced changes from a 41-ky world to a 100-ky world.en_AU
dc.description.sponsorshipThis work would not have been possible without the efforts of the IODP Program (request no. #035841IODP and #051341IODP). The research work was funded by the Science and Engineering Research Board (SERB), New Delhi, India (Reference No: SERB/F/8907/2016- 17). BN is supported by a SERB fellowship. Isotope measurements were accomplished from Wadia Institute of Himalayan Geology, Dehradun, India during INSA Visiting Scientist Fellowship by KM (INSA/SP/VSP- 07/2018-19).en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0377-8398en_AU
dc.identifier.urihttp://hdl.handle.net/1885/316184
dc.language.isoen_AUen_AU
dc.publisherElsevieren_AU
dc.rights© 2021 Elsevier B.V.en_AU
dc.sourceMarine Micropaleontologyen_AU
dc.subjectSouth Atlanticen_AU
dc.subjectPleistoceneen_AU
dc.subjectOrbulina universaen_AU
dc.subjectCaribbean speciesen_AU
dc.subjectMediterranean speciesen_AU
dc.titlePleistocene surface-ocean changes across the Southern subtropical front recorded by cryptic species of Orbulina universaen_AU
dc.typeJournal articleen_AU
local.bibliographicCitation.lastpage12en_AU
local.bibliographicCitation.startpage1en_AU
local.contributor.affiliationNirmal, B., Vellore Institute of Technologyen_AU
local.contributor.affiliationMohan, K., Vellore Institute of Technologyen_AU
local.contributor.affiliationPrakasam, M., Wadia Institute of Himalayan Geologyen_AU
local.contributor.affiliationTripati, Aradhna, University of Californiaen_AU
local.contributor.affiliationMortyn, P Graham, Universitat Autonoma de Barcelonaen_AU
local.contributor.affiliationRodriguez Sanz, Laura, College of Science, ANUen_AU
local.contributor.authoruidRodriguez Sanz, Laura, u5383979en_AU
local.description.embargo2099-12-31
local.description.notesImported from ARIESen_AU
local.identifier.absfor370799 - Hydrology not elsewhere classifieden_AU
local.identifier.absfor370506 - Palaeontology (incl. palynology)en_AU
local.identifier.absseo280107 - Expanding knowledge in the earth sciencesen_AU
local.identifier.ariespublicationa383154xPUB23723en_AU
local.identifier.citationvolume168en_AU
local.identifier.doi10.1016/j.marmicro.2021.102056en_AU
local.identifier.scopusID2-s2.0-85117412121
local.publisher.urlhttps://www.elsevier.com/en_AU
local.type.statusPublished Versionen_AU

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