Reconstruction of millennial changes in dust emission, transport and regional sea ice coverage using the deep EPICA ice cores from the Atlantic and Indian Ocean sector of Antarctica

被引:180
作者
Fischer, Hubertus
Fundel, Felix
Ruth, Urs
Twarloh, Birthe
Wegner, Anna
Udisti, Roberto
Becagli, Silvia
Castellano, Emiliano
Morganti, Andrea
Severi, Mirko
Wolff, Eric
Littot, Genevieve
Roethlisberger, Regine
Mulvaney, Rob
Hutterli, Manuel A.
Kaufmann, Patrik
Federer, Urs
Lambert, Fabrice
Bigler, Matthias
Hansson, Margareta
Jonsell, Ulf
de Angelis, Martine
Boutron, Claude
Siggaard-Andersen, Marie-Louise
Steffensen, Jorgen Peder
Barbante, Carlo
Gaspari, Vania
Gabrielli, Paolo
Wagenbach, Dietmar
机构
[1] Alfred Wegener Inst Polar & Marine Res, D-27568 Bremerhaven, Germany
[2] Univ Florence, Dept Chem, I-50019 Florence, Italy
[3] British Antarctic Survey, Cambridge CB3 0ET, England
[4] Univ Bern, Inst Phys, CH-3012 Bern, Switzerland
[5] Univ Stockholm, Dept Phys Geog & Quaternary Geol, S-10691 Stockholm, Sweden
[6] UJF, CNRS, LGGE, F-38402 St Martin Dheres, France
[7] Univ Copenhagen, Niels Bohr Inst, DK-2100 Copenhagen OE, Denmark
[8] Univ Venice, Dept Environm Sci, I-30123 Venice, Italy
[9] CNR, Inst Dynam Environm Proc, I-30123 Venice, Italy
[10] Heidelberg Univ, Inst Environm Phys, D-69120 Heidelberg, Germany
基金
英国自然环境研究理事会;
关键词
paleoclimate; ice core; Antarctica; sea salt; mineral dust;
D O I
10.1016/j.epsl.2007.06.014
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Continuous sea salt and mineral dust aerosol records have been studied on the two EPICA (European Project for Ice Coring in Antarctica) deep ice cores. The joint use of these records from opposite sides of the East Antarctic plateau allows for an estimate of changes in dust transport and emission intensity as well as for the identification of regional differences in the sea salt aerosol source. The mineral dust flux records at both sites show a strong coherency over the last 150 kyr related to dust emission changes in the glacial Patagonian dust source with three times higher dust fluxes in the Atlantic compared to the Indian Ocean sector of the Southern Ocean (SO). Using a simple conceptual transport model this indicates that transport can explain only 40% of the atmospheric dust concentration changes in Antarctica, while factor 5-10 changes occurred. Accordingly, the main cause for the strong glacial dust flux changes in Antarctica must lie in environmental changes in Patagonia. Dust emissions, hence environmental conditions in Patagonia, were very similar during the last two glacials and interglacials, respectively, despite 2-4 degrees C warmer temperatures recorded in Antarctica during the penultimate interglacial than today. 2-3 times higher sea salt fluxes found in both ice cores in the glacial compared to the Holocene are difficult to reconcile with a largely unchanged transport intensity and the distant open ocean source. The substantial glacial enhancements in sea salt aerosol fluxes can be readily explained assuming sea ice formation as the main sea salt aerosol source with a significantly larger expansion of (summer) sea ice in the Weddell Sea than in the Indian Ocean sector. During the penultimate interglacial, our sea salt records point to a 50% reduction of winter sea ice coverage compared to the Holocene both in the Indian and Atlantic Ocean sector of the SO. However, from 20 to 80 ka before present sea salt fluxes show only very subdued millennial changes despite pronounced temperature fluctuations, likely due to the large distance of the sea ice salt source to our drill sites. (c) 2007 Elsevier B.V. All rights reserved.
引用
收藏
页码:340 / 354
页数:15
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