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Antarctic Sea-Ice Thickness Retrieval from ICESat: Inter-Comparison of Different Approaches

机译:从ICESat检索南极海冰厚度:不同方法的相互比较

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Accurate circum-Antarctic sea-ice thickness is urgently required to better understand the different sea-ice cover evolution in both polar regions. Satellite radar and laser altimetry are currently the most promising tools for sea-ice thickness retrieval. We present qualitative inter-comparisons of winter and spring circum-Antarctic sea-ice thickness computed with different approaches from Ice Cloud and land Elevation Satellite (ICESat) laser altimeter total (sea ice plus snow) freeboard estimates. We find that approach A, which assumes total freeboard equals snow depth, and approach B, which uses empirical linear relationships between freeboard and thickness, provide the lowest sea-ice thickness and the smallest winter-to-spring increase in seasonal average modal and mean sea-ice thickness: A: 0.0 m and 0.04 m, B: 0.17 and 0.16 m, respectively. Approach C uses contemporary snow depth from satellite microwave radiometry, and we derive comparably large sea-ice thickness. Here we observe an unrealistically large winter-to-spring increase in seasonal average modal and mean sea-ice thickness of 0.68 m and 0.65 m, respectively, which we attribute to biases in the snow depth. We present a conceptually new approach D. It assumes that the two-layer system (sea ice, snow) can be represented by one layer. This layer has a modified density, which takes into account the influence of the snow on sea-ice buoyancy. With approach D we obtain thickness values and a winter-to-spring increase in average modal and mean sea-ice thickness of 0.17 m and 0.23 m, respectively, which lay between those of approaches B and C. We discuss retrieval uncertainty, systematic uncertainty sources, and the impact of grid resolution. We find that sea-ice thickness obtained with approaches C and D agrees best with independent sea-ice thickness information—if we take into account the potential bias of in situ and ship-based observations.
机译:迫切需要准确的南极洲海冰厚度,以更好地了解两个极地地区不同的海冰覆盖变化。卫星雷达和激光测高仪是目前最有前途的海冰厚度检索工具。我们介绍了冬季和春季南极海冰厚度的定性比较,这些冰冷厚度是根据冰云和陆地高程卫星(ICESat)激光高度计总干高(海冰加雪)干舷估算值计算得出的。我们发现方法A(假设总干舷等于雪深)和方法B(使用干舷与厚度之间的经验线性关系)提供了最低的海冰厚度,并且季节平均模态和均值最小的冬至春季增加海冰厚度:A:0.0 m和0.04 m,B:0.17和0.16 m。方法C使用卫星微波辐射法测量的现代降雪深度,我们得出了相当大的海冰厚度。在这里,我们观察到冬季到春季季节平均模态和平均海冰厚度分别为0.68 m和0.65 m出现了不切实际的大增加,这归因于雪深的偏差。我们提出了一种概念上新的方法D。它假定两层系统(海冰,雪)可以由一层表示。该层具有改进的密度,该密度考虑了雪对海冰浮力的影响。使用方法D,我们获得的厚度值和冬至春季的平均模态和平均海冰厚度分别为方法B和方法C的0.17 m和0.23 m。我们讨论了取回不确定性,系统不确定性来源,以及网格分辨率的影响。我们发现,如果考虑到原位和舰船观测的潜在偏差,则采用方法C和D获得的海冰厚度与独立的海冰厚度信息最为吻合。

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