首页> 外文会议>International symposium on remote sensing of environment;ISRSE-33 >A physically-based method for mapping glacial debris-cover thickness from ASTER satellite imagery: development and testing at Miage Glacier, Italian Alps
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A physically-based method for mapping glacial debris-cover thickness from ASTER satellite imagery: development and testing at Miage Glacier, Italian Alps

机译:一种基于物理的方法来从ASTER卫星图像中绘制冰川碎片覆盖厚度:在意大利阿尔卑斯山的Miage Glacier开发和测试

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Debris-covered glaciers (>50% of the ablation zone covered by debris) are common in many of the world's major mountain ran ges an d rep resent an imp ortant fres hwater resource. Previous studies have established that surface melt rates decrease strongly for an increase in supraglacial debris thickness from a fe wcmupto 20-30 cm, whereas, th in an d patchy debris cover enhances melt due to albedo reduction. It is therefore important to develop methods to map and monitor changes in debris cover to en able predictions of glacier responses to climate change through numerical modelling. It is not possible to achieve this from ground-based measurements alone. Therefore, a m ethod to estimate debris thickness from an ASTER thermal band surface temperature image, based on a physical solution of the energy balance at the debris surface, has been developed. The model performs well in comparison to previous em pirical methods showing good agreem ent with measured debris thicknesses.
机译:覆盖有碎屑的冰川(超过碎屑覆盖的消融区的50%)在世界上许多主要山区水资源和重要的淡水资源中很常见。先前的研究已经确定,表面融化速率会大大降低,从而使冰川岩碎屑的厚度从fe wcmupup增加到20-30 cm,而片状碎片覆盖层由于反照率的降低而增强了融化作用。因此,重要的是要开发出一种方法来绘制和监测残骸覆盖率的变化,以便能够通过数值模拟来预测冰川对气候变化的响应。单靠地面测量是不可能做到这一点的。因此,已经开发了一种方法,其基于碎片表面处的能量平衡的物理解,从ASTER热能带表面温度图像估计碎片厚度。与以往的经验方法相比,该模型表现良好,与测量的碎屑厚度显示出良好的一致性。

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