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高分辨率同位素证据表明格陵兰冰川粉尘可能来自撒哈拉沙漠。

High-resolution isotopic evidence for a potential Saharan provenance of Greenland glacial dust.

机构信息

Department of Ocean Sciences, Inha University, 100 Inha-ro, Michuhol-gu, Incheon, 22212, Korea.

Korea Polar Research Institute, 26 Songdomirae-ro, Yeonsu-gu, Incheon, 21990, Korea.

出版信息

Sci Rep. 2018 Oct 22;8(1):15582. doi: 10.1038/s41598-018-33859-0.

DOI:10.1038/s41598-018-33859-0
PMID:30348975
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC6197225/
Abstract

Dust concentrations in Greenland ice show pronounced glacial/interglacial variations with almost two orders of magnitude increase during the Last Glacial Maximum. Greenland glacial dust was previously sourced to two East Asian deserts: the Taklimakan and Gobi deserts. Here we report the first high-resolution Pb and Sr isotopic evidence for a significant Saharan dust influence in Greenland during the last glacial period, back to 31 kyr ago, from the Greenland NEEM ice core. We find that during Greenland Stadials 3-5.1 (31 to 23 kyr ago), the primary dust provenance was East Asia, as previously proposed. Subsequently, the Saharan isotopic signals emerge during Greenland Stadials 2.1a-2.1c (22.6 to 14.7 kyr ago) and from the late Bølling-Allerød to the Younger Dryas periods (13.6 to 12 kyr ago), coincident with increased aridity in the Sahara and efficient northward transport of dust during these cold periods. A mixing isotopic model proposes the Sahara as an important source, accounting for contribution to Greenland glacial dust of up to 50%, particularly during Greenland Stadial 2.1b and the late Bølling-Allerød to the Younger Dryas periods. Our findings provide new insights into climate-related dust provenance changes and essential paleoclimatic constraints on dust-climate feedbacks in northern high latitudes.

摘要

格陵兰冰芯中的尘埃浓度表现出明显的冰期/间冰期变化,在上一个冰期最大值期间增加了近两个数量级。格陵兰冰芯尘埃源以前被认为来自两个东亚沙漠:塔克拉玛干沙漠和戈壁沙漠。在这里,我们报告了第一个高分辨率的 Pb 和 Sr 同位素证据,表明在上一个冰期期间,撒哈拉尘埃对格陵兰有显著影响,可以追溯到约 31 千年前,来自格陵兰 NEEM 冰芯。我们发现,在上一个冰期的格陵兰冰期 3-5.1 期间(约 31 到 23 千年前),主要的尘埃来源是东亚,如前所述。随后,撒哈拉的同位素信号在格陵兰冰期 2.1a-2.1c 期间出现(约 22.6 到 14.7 千年前),并且从 Bolling-Allerød 晚期到 Younger Dryas 期间(约 13.6 到 12 千年前),与撒哈拉地区干旱加剧和这些寒冷时期尘埃向北有效传输相吻合。混合同位素模型提出撒哈拉是一个重要的来源,对格陵兰冰芯尘埃的贡献高达 50%,特别是在格陵兰冰期 2.1b 和 Bolling-Allerød 晚期到 Younger Dryas 期间。我们的发现提供了有关气候相关尘埃来源变化的新见解,并为北部高纬度地区尘埃-气候反馈提供了重要的古气候约束。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/143f/6197225/d4a48dc5c1a2/41598_2018_33859_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/143f/6197225/be31d746b56b/41598_2018_33859_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/143f/6197225/805edb6294b0/41598_2018_33859_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/143f/6197225/7da7b9ea112a/41598_2018_33859_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/143f/6197225/d4a48dc5c1a2/41598_2018_33859_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/143f/6197225/be31d746b56b/41598_2018_33859_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/143f/6197225/805edb6294b0/41598_2018_33859_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/143f/6197225/7da7b9ea112a/41598_2018_33859_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/143f/6197225/d4a48dc5c1a2/41598_2018_33859_Fig4_HTML.jpg

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