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ICESat measurements of sea ice freeboard and estimates of sea ice thickness in the Weddell Sea

机译:ICESat测量海冰干舷并估算韦德尔海的海冰厚度

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Sea ice freeboard heights in the Weddell Sea of Antarctica are derived from the Ice, Cloud, and Land Elevation Satellite (ICESat) laser altimeter measurements, which have a unique range precision to flat surfaces of 2 cm within 70 m footprints spaced at 172 m along track. Although elevations of flat surfaces can be obtained to an accuracy of ~10 cm (1σ) per footprint, direct determination of freeboard heights is precluded by errors in knowledge of the geoid and temporal variability of the ocean surface. Therefore freeboards are determined relative to an ocean reference level detected over areas of open water and very thin ice within the sea ice pack using an along-track filtering method. The open water/thin ice selections show good agreement in the combined analysis of ICESat segments and Envisat Synthetic Aperture Radar (SAR) imagery. The average residual between the ICESat-measured ocean level and the EGM96 geoid is 1.4 m. Estimates of snow depth on the sea ice from AMSR-E passive microwave data along with nominal densities of snow, water, and sea ice are used to estimate sea ice thickness. Four periods of ICESat data in May–June (fall) and October–November (late winter) of 2004 and 2005 between longitudes 298°E and 360°E are analyzed. In the fall the mean freeboards are 0.28 m in 2004 and 0.29 m in 2005, and the mean thicknesses are 1.33 m in 2004 and 1.52 m in 2005. In late winter the freeboards grew to 0.37 m in 2004 and 0.35 in 2005, and the thicknesses grew to 2.23 m in 2004 and 2.31 m in 2005. The interannual differences in freeboard are small, and the larger interannual change in estimated thickness mainly represents differences in the snow depth estimates. Seasonal changes in the spatial patterns of freeboard and thickness over the 4 months correlate with the expected circulation of sea ice in the Weddell Sea, as indicated by sea ice velocity fields.
机译:南极洲韦德尔海的海冰干舷高度来自冰,云和陆地高程卫星(ICESat)激光高度计的测量结果,该高度对2 cm的平坦表面具有独特的范围精度,在70 m覆盖范围内沿172 m沿跟踪。尽管可以获得的平坦表面的高度精确度为每个足迹约10 cm(1σ),但由于对大地水准面和时间变化的认识错误,无法直接确定干舷高度。因此,使用沿航迹过滤方法,相对于在海冰包内的开阔水域和极薄冰上检测到的海洋参考水平来确定干舷。在结合ICESat航段和Envisat合成孔径雷达(SAR)图像进行分析时,开放水/稀冰的选择显示出良好的一致性。 ICESat测得的海平面与EGM96大地水准面之间的平均残差为1.4 m。根据AMSR-E无源微波数据估算海冰上的积雪深度,并使用雪,水和海冰的标称密度估算海冰厚度。分析了2004年和2005年5月至6月(秋季)和10月至11月(冬季末)在经度298°E和360°E之间的四个ICESat数据。秋季,平均干舷在2004年为0.28 m,在2005年为0.29 m,平均厚度在2004年为1.33 m,在2005年为1.52 m。在冬季末,干舷在2004年增加到0.37 m,在2005年增加到0.35,厚度在2004年增加到2.23 m,在2005年增加到2.31 m。干舷的年际差异很小,而估计厚度的较大年际变化主要表示雪深估计的差异。如海冰速度场所示,过去4个月干舷和厚度空间格局的季节性变化与Weddell海中预期的海冰环流相关。

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