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The ice thickness distribution of a debris-covered glacier: Tasman Glacier, New Zealand

机译:覆盖有冰川的冰川的冰厚度分布:新西兰塔斯曼冰川

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摘要

The ice thickness distribution of mountain valley glaciers is an important physical constraint for modelling their flow. Ice thickness measurements are used to calculate the geometry and ultimately the driving stress of a glacier. This information is all required if realistic models are to forecast the response of glaciers to climate forcings. For New Zealand's Tasman Glacier, two factors complicate its response to climate: 1) A layer of insulative rocky debris covers the lower half of the glacier, retarding surface melt, and 2) the glacier has recently entered a period of iceberg calving into a proglacial lake, introducing complex mechanical processes. These complications, along with the uncertainty of the current bed topography of the Tasman Glacier, make future predictions of its retreat behaviour difficult. The bed of the Tasman Glacier has not been fully imaged but ice thickness measurements obtained through seismic and gravity surveys have provided constraints for parts of the glacier. This study applies a range of geophysical methods (gravity and refraction seismics) to measure and model the ice thickness distribution of the lower Tasman Glacier. We surveyed orthogonal to glacier flow to obtain 12 transects within the lower 5 km of the glacier. Two-dimensional and three-dimensional gravity models generally indicate a U-shaped valley with ice thicknesses of 92-722 m from the present day terminus to the most upstream transect respectively. These results were used as input data to a simple mass flux model to assess its performance in estimating ice thickness and volume for the Tasman Glacier. The mass-flux model estimated a volume of 14.96 km3 for the Tasman Glacier, but generally underestimated ice thickness with an RMSE of 148 m between the modelled and the gravity-derived ice thickness. This discrepancy could be reduced by constraining ice thickness for a larger area of the glacier and providing a more recent DEM to the mass flux model. Studies such as this highlight the importance of constraining ice thickness in order to improve glacio-dynamic models and global volume estimates.
机译:山谷冰川的冰厚分布是模拟其流动的重要物理约束。冰厚的测量值用于计算几何形状,并最终计算出冰川的驱动应力。如果要通过实际模型来预测冰川对气候强迫的响应,则需要所有这些信息。对于新西兰的塔斯曼冰川,有两个因素使它对气候的响应更加复杂:1)一层绝缘的岩石碎屑覆盖了冰川的下半部分,阻碍了表面融化; 2)冰川最近进入了一段冰山崩裂成冰川状的时期湖,引入了复杂的机械过程。这些复杂性,加上塔斯曼冰川目前河床地形的不确定性,使得未来对其退缩行为的预测变得困难。塔斯曼冰川的河床尚未完全成像,但通过地震和重力勘测获得的冰厚测量值为部分冰川提供了约束。这项研究应用了一系列地球物理方法(重力和折射地震)来测量和模拟塔斯曼河下部冰川的冰厚度分布。我们调查了与冰川流正交的方向,以在冰川下5公里内获得12个样点。二维和三维重力模型通常表示从当前终点到最上游断面的冰厚为92-722 m的U形谷。这些结果被用作简单质量通量模型的输入数据,以评估其在估算塔斯曼冰川冰厚度和体积时的性能。质量通量模型估计塔斯曼冰川的体积为14.96 km3,但通常低估了冰层的厚度,其模型与重力得出的冰层厚度之间的均方根误差(RMSE)为148 m。可以通过限制更大面积冰川的冰厚度并为质量通量模型提供更新的DEM来减少这种差异。诸如此类的研究强调了限制冰厚对改善冰川动力学模型和整体体积估计的重要性。

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    Hart Rory;

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  • 年度 2014
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  • 正文语种 en_NZ
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