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Albedo over rough snow and ice surfaces

机译:在粗糙的冰雪表面上的反照率

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摘要

Both satellite and ground-based broadband albedo measurements over rough and complex terrain show several limitations concerning feasibility and representativeness. To assess these limitations and understand the effect of surface roughness on albedo, firstly, an intrasurface radiative transfer (ISRT) model is combined with albedo measurements over different penitente surfaces on Glaciar Tapado in the semi-arid Andes of northern Chile. Results of the ISRT model show effective albedo reductions over the penitentes up to 0.4 when comparing the rough surface albedo relative to the albedo of the flat surface. The magnitude of these reductions primarily depends on the opening angles of the penitentes, but the shape of the penitentes and spatial variability of the material albedo also play a major role. Secondly, the ISRT model is used to reveal the effect of using albedo measurements at a specific location (i.e., apparent albedo) to infer the true albedo of a penitente field (i.e., effective albedo). This effect is especially strong for narrow penitentes, resulting in sampling biases of up to ±0.05. The sampling biases are more pronounced when the sensor is low above the surface, but remain relatively constant throughout the day. Consequently, it is important to use a large number of samples at various places and/or to locate the sensor sufficiently high in order to avoid this sampling bias of surface albedo over rough surfaces. Thirdly, the temporal evolution of broadband albedo over a penitente-covered surface is analyzed to place the experiments and their uncertainty into a longer temporal context. Time series of albedo measurements at an automated weather station over two ablation seasons reveal that albedo decreases early in the ablation season. These decreases stabilize from February onwards with variations being caused by fresh snowfall events. The 2009/2010 and 2011/2012 seasons differ notably, where the latter shows lower albedo values caused by larger penitentes. Finally, a comparison of the ground-based albedo observations with Landsat and MODIS (Moderate Resolution Imaging Spectroradiometer)-derived albedo showed that both satellite albedo products capture the albedo evolution with root mean square errors of 0.08 and 0.15, respectively, but also illustrate their shortcomings related to temporal resolution and spatial heterogeneity over small mountain glaciers.
机译:在崎and不平的地形上进行的卫星和地面宽带反照率测量都显示出一些关于可行性和代表性的限制。为了评估这些局限性并了解表面粗糙度对反照率的影响,首先,在智利北部半干旱安第斯山脉的Glaciar Tapado上,在不同的pen悔表面上采用了面内辐射传输(ISRT)模型和反照率测量。 ISRT模型的结果显示,当比较粗糙表面的反照率与平坦表面的反照率时,在阴茎上的有效反照率降低到0.4。这些减少的幅度主要取决于the悔节的张开角度,但the悔节的形状和反照率物质的空间变异性也起主要作用。其次,ISRT模型用于揭示在特定位置(即表观反照率)使用反照率测量来推断a悔场的真实反照率(即有效反照率)的效果。对于狭窄的it齿,此效果尤其明显,导致采样偏差高达±0.05。当传感器位于地面上方较低时,采样偏差会更明显,但整天保持相对恒定。因此,重要的是在不同位置使用大量样本和/或将传感器放置在足够高的位置,以避免表面反照率在粗糙表面上的这种采样偏差。第三,分析了覆盖在pen悔表面上的宽带反照率的时间演化,以将实验及其不确定性置于较长的时间范围内。在两个消融季节中,自动气象站的反照率测量的时间序列显示,在消融季节的早期反照率下降。这些减少从2月开始稳定下来,原因是新的降雪事件引起了变化。 2009/2010年和2011/2012年季节明显不同,后者显示出较大的pen悔导致较低的反照率。最后,将地面反照率观测值与Landsat和MODIS(中等分辨率成像光谱仪)反照率进行比较后发现,这两个卫星反照率产品均捕获了反照率演化,其均方根误差分别为0.08和0.15,而且还说明了它们的均方根误差。与小型冰川的时间分辨率和空间异质性有关的缺点。

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