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Potential and limitations of marine and ice core sea ice proxies: an example from the Indian Ocean sector

dc.contributor.authorRothlisberger, Regine
dc.contributor.authorCrosta, Xavier
dc.contributor.authorAbram, Nerilie
dc.contributor.authorArmand, Leanne
dc.contributor.authorWolff, E.W.
dc.date.accessioned2015-12-13T22:43:07Z
dc.date.issued2010
dc.date.updated2016-02-24T09:36:00Z
dc.description.abstractDiatom assemblages in marine cores and sea salt deposition fluxes in ice cores have been used as sea ice proxies in the southern hemisphere. Here, a marine and an ice core proxy record for the Indian Ocean covering the last two glacial cycles are compared in order to illustrate their potential and limitations. The marine core was extracted in a location completely ice free under present-day conditions, and therefore was unable to record changes to the recent sea ice extent. Similarly, no sea ice was recorded at that location during the previous interglacial period. During the last glacial period, however, the site was seasonally covered by sea ice, and the diatom assemblages allowed an estimation of average seasonal sea ice presence. The ice core data originated from the East Antarctic plateau. The marine sodium present in the ice core was used as a proxy of the sea-ice coverage and, on average, a larger sea ice surface led to an increased sea-salt aerosol flux, seen e.g. at the last glacial inception. However, the response of the sea salt flux to increasing sea ice extent diminished during peak glacial conditions when only minimal variability was recorded in the ice core record. A first-order approximation is used to take this non-linear response of the ice core sea ice proxy into account. Based on the ice core proxy record, sea ice extent was reduced considerably during the warm episodes of the previous two interglacial periods compared to modern sea ice extent, in particular during the peak warmth of the Last Interglacial. The ice core proxy also showed a very strong precessional variability (pronounced spectral peak at 23 ka period) over the past 240 ka. The advantage of combining the two proxy records lies in the complementary nature of their response. While the ice core proxy showed limited sensitivity during full glacial conditions, the marine proxy recorded the seasonal sea-ice coverage. Once the sea ice retreated south of the location of the marine core, the ice core proxy responded to changes in sea ice extent. A composite of marine and ice core records may thus provide a data basis for a more detailed reconstruction of sea ice around Antarctica over the last few glacial-interglacial cycles.
dc.identifier.issn0277-3791
dc.identifier.urihttp://hdl.handle.net/1885/79059
dc.publisherPergamon-Elsevier Ltd
dc.sourceQuaternary Science Reviews
dc.subjectKeywords: Antarctic plateau; Antarctica; Diatom assemblage; First-order approximations; Glacial cycles; Glacial-interglacial cycles; Ice core; Ice core records; Indian ocean; Interglacial periods; Last glacial inception; Last glacial period; Last interglacial; Limi
dc.titlePotential and limitations of marine and ice core sea ice proxies: an example from the Indian Ocean sector
dc.typeJournal article
local.bibliographicCitation.issue1-2
local.bibliographicCitation.lastpage302
local.bibliographicCitation.startpage296
local.contributor.affiliationRothlisberger, Regine, British Antarctic Survey
local.contributor.affiliationCrosta, Xavier, Universite Bordeaux
local.contributor.affiliationAbram, Nerilie, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationArmand, L, Antarctic Climate and Ecosystem Cooperative Research Centre
local.contributor.affiliationWolff, E.W., British Antarctic Survey
local.contributor.authoruidAbram, Nerilie, u9718469
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor040599 - Oceanography not elsewhere classified
local.identifier.absseo970104 - Expanding Knowledge in the Earth Sciences
local.identifier.ariespublicationf5625xPUB7593
local.identifier.citationvolume29
local.identifier.doi10.1016/j.quascirev.2009.10.005
local.identifier.scopusID2-s2.0-73549116150
local.type.statusPublished Version

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