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Comparing past accumulation rate reconstructions in East Antarctic ice cores using sup10/supBe, water isotopes and CMIP5-PMIP3 models

机译:使用 10 Be,水同位素和CMIP5-PMIP3模型比较南极东部冰芯过去的蓄水速率重建

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Ice cores are exceptional archives which allow us to reconstruct a wealth of climatic parameters as well as past atmospheric composition over the last 800 kyr in Antarctica. Inferring the variations in past accumulation rate in polar regions is essential both for documenting past climate and for ice core chronology. On the East Antarctic Plateau, the accumulation rate is so small that annual layers cannot be identified and accumulation rate is mainly deduced from the water isotopic composition assuming constant temporal relationships between temperature, water isotopic composition and accumulation rate. Such an assumption leads to large uncertainties on the reconstructed past accumulation rate. Here, we use high-resolution beryllium-10 (10Be) as an alternative tool for inferring past accumulation rate for the EPICA Dome C ice core, in East Antarctica. We present a high-resolution 10Be record covering a full climatic cycle over the period 269 to 355 ka from Marine Isotope Stage (MIS) 9 to 10, including a period warmer than pre-industrial (MIS 9.3 optimum). After correcting 10Be for the estimated effect of the palaeomagnetic field, we deduce that the 10Be reconstruction is in reasonably good agreement with EDC3 values for the full cycle except for the period warmer than present. For the latter, the accumulation is up to 13% larger (4.46 cm ie yr?1 instead of 3.95). This result is in agreement with the studies suggesting an underestimation of the deuterium-based accumulation for the optimum of the Holocene (Parrenin et al. 2007a). Using the relationship between accumulation rate and surface temperature from the saturation vapour relationship, the 10Be-based accumulation rate reconstruction suggests that the temperature increase between the MIS 9.3 optimum and present day may be 2.4 K warmer than estimated by the water isotopes reconstruction. We compare these reconstructions to the available model results from CMIP5-PMIP3 for a glacial and an interglacial state, i.e. for the Last Glacial Maximum and pre-industrial climates. While 3 out of 7 models show relatively good agreement with the reconstructions of the accumulation–temperature relationships based on 10Be and water isotopes, the other models either underestimate or overestimate it, resulting in a range of model results much larger than the range of the reconstructions. Indeed, the models can encounter some difficulties in simulating precipitation changes linked with temperature or water isotope content on the East Antarctic Plateau during glacial–interglacial transition and need to be improved in the future.
机译:冰芯是非凡的档案,使我们能够重建南极洲最后800年来的大量气候参数以及过去的大气成分。推断极地地区过去累积速率的变化对于记录过去的气候和冰芯年代都至关重要。在南极东部高原,积聚速率很小,以至于无法确定年层,并且假设温度,水同位素组成和积聚速率之间存在恒定的时间关系,则积聚速率主要由水的同位素组成推导。这样的假设导致重建的过去积累率存在很大的不确定性。在这里,我们使用高分辨率铍10( 10 Be)作为推断南极东部EPICA Dome C冰芯过去累积速率的替代工具。我们提供了高分辨率的 10 Be记录,涵盖了从海洋同位素阶段(MIS)9到10到269 ka至355 ka的整个气候周期,其中包括一个比工业化前期更暖的时期(MIS 9.3最佳)。在校正了 10 Be对古磁场的估计影响之后,我们推断出 10 Be的重建与整个周期的EDC3值在合理的程度上吻合,除了周期比现在温暖。对于后者,累积量最多增加13%(4.46厘米,即yr ?1 而不是3.95)。这一结果与研究相吻合,表明低估了基于氘的全新世最佳沉积(Parrenin等,2007a)。基于饱和蒸汽关系,利用累积速率和表面温度之间的关系,基于 10 Be的累积速率重构表明,MIS 9.3最佳温度与当日温度之间的温度可能比估计的高2.4 K由水同位素重建。我们将这些重建结果与CMIP5-PMIP3的冰川状态和冰川间状态(即最后一次冰川最大和工业化前的气候)的可用模型结果进行了比较。尽管7个模型中有3个与基于 10 Be和水同位素的蓄积-温度关系的重建相对较好,但是其他模型要么低估要么高估了模型结果比重建范围大得多。实际上,该模型在模拟冰川-冰川间过渡过程中与南极高原东部温度或水同位素含量有关的降水变化时会遇到一些困难,因此将来需要改进。

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