首页> 外文期刊>Journal of Geophysical Research, C. Oceans: JGR >Airborne thickness and freeboard measurements over the McMurdo Ice Shelf, Antarctica, and implications for ice density
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Airborne thickness and freeboard measurements over the McMurdo Ice Shelf, Antarctica, and implications for ice density

机译:南极麦克默多冰架上的机载厚度和干舷测量值,以及对冰密度的影响

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摘要

[1] We present airborne measurements to investigate the thickness of the western McMurdo Ice Shelf in the western Ross Sea, Antarctica. Because of basal accretion of marine ice and brine intrusions conventional radar systems are limited in detecting the ice thickness in this area. In November 2009, we used a helicopter-borne laser and electromagnetic induction sounder (EM bird) to measure several thickness and freeboard profiles across the ice shelf. The maximum electromagnetically detectable ice thickness was about 55 m. Assuming hydrostatic equilibrium, the simultaneous measurement of ice freeboard and thickness was used to derive bulk ice densities ranging from 800 to 975 kg m~(-3). Densities higher than those of pure ice can be largely explained by the abundance of sediments accumulated at the surface and present within the ice shelf, and are likely to a smaller extent related to the overestimation of ice thickness by the electromagnetic induction measurement related to the presence of a subice platelet layer. The equivalent thickness of debris at a density of 2800 kg m~(-3) is found to be up to about 2 m thick. A subice platelet layer below the ice shelf, similar to what is observed in front of the ice shelf below the sea ice, is likely to exist in areas of highest thickness. The thickness and density distribution reflects a picture of areas of basal freezing and supercooled Ice Shelf Water emerging from below the central ice shelf cavity into McMurdo Sound.
机译:[1]我们目前进行空中测量,以调查南极西部罗斯海西部麦克默多冰架的厚度。由于海冰和盐水侵入的基础积聚,常规雷达系统在检测该区域的冰厚方面受到限制。 2009年11月,我们使用了直升机上的激光和电磁感应测深仪(EM鸟)来测量冰架上的多个厚度和干舷轮廓。电磁检测的最大冰厚度约为55 m。假设静水平衡,同时测量干舷和干冰厚度可得出800至975 kg m〜(-3)的体积冰密度。高于纯冰的密度很大程度上可以由表层和冰架内堆积的大量沉积物来解释,并且可能在较小程度上与通过与存在有关的电磁感应测量高估了冰的厚度有关子血小板层的一部分。发现密度为2800 kg m〜(-3)的碎屑的等效厚度最大为约2 m厚。冰架下面的一个子血小板层,类似于在海冰之下的冰架前面所观察到的那样,可能存在于厚度最大的区域。厚度和密度分布反映了从中央冰架腔的下方涌入麦克默多峡湾的基础冻结和过冷的冰架水区域的图像。

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