首页> 外文期刊>The Cryosphere Discussions >Spatial and temporal distributions of surface mass balance between Concordia and Vostok stations, Antarctica, from combined radar and ice core data: first results and detailed error analysis
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Spatial and temporal distributions of surface mass balance between Concordia and Vostok stations, Antarctica, from combined radar and ice core data: first results and detailed error analysis

机译:从雷达和冰芯组合数据看南极康考迪亚站和沃斯托克站之间表面质量平衡的时空分布:初步结果和详细误差分析

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Results from ground-penetrating radar (GPR) measurements and shallow ice cores carried out during a scientific traverse between Dome Concordia (DC) and Vostok stations are presented in order to infer both spatial and temporal characteristics of snow accumulation over the East Antarctic Plateau. Spatially continuous accumulation rates along the traverse are computed from the identification of three equally spaced radar reflections spanning about the last 600 years. Accurate dating of these internal reflection horizons (IRHs) is obtained from a depth–age relationship derived from volcanic horizons and bomb testing fallouts on a DC ice core and shows a very good consistency when tested against extra ice cores drilled along the radar profile. Accumulation rates are then inferred by accounting for density profiles down to each IRH. For the latter purpose, a careful error analysis showed that using a single and more accurate density profile along a DC core provided more reliable results than trying to include the potential spatial variability in density from extra (but less accurate) ice cores distributed along the profile. The most striking feature is an accumulation pattern that remains constant through time with persistent gradients such as a marked decrease from 26 mm?w.e.?yr sup?1/sup at DC to 20 mm?w.e.?yr sup?1/sup at the south-west end of the profile over the last 234 years on average (with a similar decrease from 25 to 19 mm?w.e.?yr sup?1/sup over the last 592 years). As for the time dependency, despite an overall consistency with similar measurements carried out along the main East Antarctic divides, interpreting possible trends remains difficult. Indeed, error bars in our measurements are still too large to unambiguously infer an apparent time increase in accumulation rate. For the proposed absolute values, maximum margins of error are in the range 4 mm?w.e.?yr sup?1/sup (last 234 years) to 2 mm?w.e.?yr sup?1/sup (last 592 years), a decrease with depth mainly resulting from the time-averaging when computing accumulation rates. Please read the corrigendum first before continuing.
机译:本文介绍了在Dome Concordia(DC)和Vostok站之间进行科学穿越时进行的探地雷达(GPR)测量和浅冰芯的结果,以推断南极东部高原积雪的时空特征。通过确定跨越大约600年的三个等距雷达反射,可以计算出遍历空间连续的累积速率。这些内部反射层(IRH)的准确测年是从火山层和DC冰芯上的炸弹测试落差得出的深度-年龄关系中获得的,当与沿雷达剖面钻出的额外冰芯进行测试时,显示出非常好的一致性。然后,通过考虑到每个IRH的密度分布来推断累积速率。对于后一个目的,仔细的误差分析表明,沿着DC核心使用单个更准确的密度分布图比尝试包括沿分布图分布的额外(但精度较差)冰芯的密度潜在的空间变异性提供了更可靠的结果。 。最显着的特征是随着时间的流逝而保持不变的累积模式,例如从DC的26 mm?we?yr ?1 显着减小到20 mm?we?yr ?。在过去234年中,剖面的西南端平均为1 (在过去592年中,we 从25毫米减少到19毫米) 。关于时间依赖性,尽管总体上与沿南极东部主要鸿沟进行的类似测量相一致,但难以解释可能的趋势。确实,我们测量中的误差线仍然太大,无法明确地推断出累积速率的明显时间增加。对于建议的绝对值,最大误差范围在4 mm?we?yr ?1 (最近234年)到2 mm?we?yr ?1 的范围内(最近592年),随深度的减小主要是由于计算累积速率时的时间平均造成的。请先阅读勘误表,然后再继续。

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