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34000年以来南极汞沉降通量的估算
引用本文:尹雪斌,孙立广,谢周清.34000年以来南极汞沉降通量的估算[J].极地研究,2003,15(3):207-213.
作者姓名:尹雪斌  孙立广  谢周清
作者单位:中国科学技术大学极地环境研究室,合肥,230026
基金项目:国家自然科学基金资助项目 (批准号:40 0 760 3 2 ),科技部公益项目(批准号 :2 0 0 1DIA5 0 0 40— 0 9)
摘    要:本文统计分析了南极DomeC冰芯中汞含量和降水指征参数δ1 8O值、1 0 Be浓度的关系 ,发现冰芯中Hg含量和δ1 8O值、1 0 Be浓度变化一致 ,表明DomeC冰芯汞含量受到冰雪积累率的影响 ,而且三者变化的高度同步性可能说明其原始驱动力也是一致的 ,从而冰芯中Hg含量可以和1 0 Be浓度一样作为冰雪积累率估算的替代性指标。此外 ,利用δ1 8O数据 ,系统估算了 340 0 0年以来南极汞沉降通量的变化。结果表明 ,DomeC冰芯汞沉降通量在末次冰盛期 (LGM)最高 ,为 3.80pgcm- 2 a- 1 ,约是全新世汞沉降通量 ( 1 .0 8pgcm- 2 a- 1 )的 3.5倍 ,该变化可能主要受到汞的自然排放量影响。

关 键 词:汞沉降通量  降水速率  末次冰盛期  全新世  南极冰芯  
修稿时间:2003年6月1日

AN ASSESSMENT OF VARIATIONS IN MERCURY DEPOSITION TO ANTARCTICA OVER THE PAST 34000 YEARS
Yin Xuebin,Sun Liguang and Xie Zhouqing.AN ASSESSMENT OF VARIATIONS IN MERCURY DEPOSITION TO ANTARCTICA OVER THE PAST 34000 YEARS[J].Chinese Journal of Polar Research,2003,15(3):207-213.
Authors:Yin Xuebin  Sun Liguang and Xie Zhouqing
Abstract:Comparing the variation of the Hg concentrations in 14 subsamples from Antarctic Dome C ice core (Vandal et al., 1993) with the precipitation proxies such as δ 18 O values and 10 Be concentrations in the Dome C ice more, we found a significant correlation between Hg concentrations and δ 18 O values, 10 Be concentrations. And this clearly indicates that the accumulation rate in Dome C is one of the key factors to the variations of Hg concentrations. Therefore, Hg concentrations in ice core can be used as a proxy of precipitation rate. In this paper, we reassess the variations in mercury deposition flux in Antarctica over the past 34,000 years on the base of the high resolution δ 18 O values, which can be used as a good proxy reconstructing the precipitation rates. In our results, the highest mercury deposition flux is about 3.80pg cm -2 a -1 during the Last Glacial Maxium (LGM), as high as 3.5 times of the mercury deposition flux (about 1.08 pg cm -2 a -1 ) in Holocene. And this is because of the fluctuations in natural mercury emissions such as the oceanic biological emission.
Keywords:mercury deposition flux  precipitation rate  LGM  Holocene  Antarctic Dome C ice core
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