首页> 外文会议>Conference on land surface and cryosphere remote sensing III >Light absorbing impurity deposition over the Himalayan-Karakoram-Hindu Kush-Tibetan cryosphere: A review and satellite-based characterization
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Light absorbing impurity deposition over the Himalayan-Karakoram-Hindu Kush-Tibetan cryosphere: A review and satellite-based characterization

机译:光吸收杂质沉积在喜马拉雅岛 - 喀喇昆仑 - 印度教古氏菌冰区:综述和卫星基于卫星的特征

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Light absorbing impurities such as black carbon and dust reduce the reflectance of snow/ice surface. The impurities absorb the incoming solar radiation thereby accelerating snow aging and melting. This further accelerates the processes of snow albedo reduction and melting. A recently-conducted ice core study in Mera Peak shows that annual dust mass fluxes (10.4+/-2.8 g m~(-2) yr~(-1)) are a few orders of magnitude higher than black carbon (7.9+/-2.8 g m~(-2) yr~(-1)). A similar study conducted in the Tibetan Plateau showed a decrease in the amount of mineral dust deposition since 1940s indicating that the increased glacier melt can be attributed to increased black carbon emission than dust. The concentrations of black carbon and dust peak during the pre-monsoon season. Spectral reflectance curves derived from satellite imagery for the Himalayan Tibetan Plateau showed domination of dust-induced solar absorption during the pre-monsoon season. Spatial distribution of reflectance also depends on the transport pathway of impurities, with the south western Hindu Kush and Himalaya experiencing greater dust influx, deposition and snow albedo reduction than northern regions of Karakoram. In this study, we characterize the light absorbing impurities deposited in Himalayan regions using multi spectral data from MODIS and LANDSAT. On comparing the spectral reflectance curves derived from MODIS and LANDSAT for the overlapping periods and areas and by observing the VIS-NIR gradient of spectral reflectance, determination of the type of light absorbing impurity, mainly mineral dust, and its relation to snow properties are derived.
机译:黑色碳和粉尘等光吸收杂质减少了雪/冰面的反射率。杂质吸收进入的太阳辐射,从而加速雪衰老和熔化。这进一步加速了雪反照镜的过程减少和融化的过程。 Mera Peak最近进行的冰核心研究表明,年粉尘质量助量(10.4 +/- 2.8 gm〜(-2)Yr〜(-1))是比黑碳高的数量级(7.9 +/- 2.8 gm〜(-2)Yr〜(-1))。在西藏高原中进行的类似研究表明,自20世纪40年代以来,矿物粉尘沉积量表明增加的冰川熔体可以归因于增加黑炭排放而不是灰尘。季铵季季节中黑碳和灰尘峰的浓度。来自喜马拉雅藏高原的卫星图像的光谱反射曲线显示出在季风季节期间的灰尘引起的太阳能吸收的统治。反射率的空间分布也取决于杂质的运输途径,西部印度教犬和喜马拉雅省经历了大量的尘埃流入,沉积和雪反照科,而不是卡拉姆姆北部地区。在这项研究中,我们在使用来自MODIS和Landsat的多谱数据沉积在喜马拉雅地区的光吸收杂质。比较从MODIS和LANDSAT的光谱反射曲线对重叠时段和区域的谱反射曲线以及通过观察光谱反射率的VIR-NIR梯度,得出了光学杂质类型的测定,主要是矿物粉尘及其与雪特性的关系。

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