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Distinguishing ice-rich and ice-poor permafrost to map ground temperatures and ground ice occurrence in the Swiss Alps

机译:将富含冰和冰贫穷的永久冻土区分将地面温度和地面冰发生在瑞士阿尔卑斯山区

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摘要

Mountain permafrost is invisible, and mapping it is stilla challenge. Available permafrost distribution maps often overestimate thepermafrost extent and include large permafrost-free areas in theirpermafrost zonation. In addition, the representation of the lower belt ofpermafrost consisting of ice-rich features such as rock glaciers or ice-richtalus slopes can be challenging. These problems are caused by considerabledifferences in genesis and thermal characteristics between ice-poorpermafrost, occurring for example in rock walls, and ice-rich permafrost.While ice-poor permafrost shows a strong correlation of ground temperaturewith elevation and potential incoming solar radiation, ice-rich ground doesnot show such a correlation. Instead, the distribution of ice-rich ground iscontrolled by gravitational processes such as the relocation of ground iceby permafrost creep or by ground ice genesis from avalanche deposits orglacierets covered with talus. We therefore developed a mapping method which distinguishes between ice-poorand ice-rich permafrost and tested it for the entire Swiss Alps. Forice-poor ground we found a linear regression formula based on elevation andpotential incoming solar radiation which predicts borehole groundtemperatures at multiple depths with an accuracy higher than 0.6 ∘C. The zone of ice-rich permafrost was defined by modelling the depositionzones of alpine mass wasting processes. This dual approach allows thecartographic representation of permafrost-free belts, which are boundedabove and below by permafrost. This enables a high quality of permafrostmodelling, as is shown by the validation of our map. The dominatinginfluence of the two rather simple connected factors, elevation (as a proxyfor mean annual air temperature) and solar radiation, on the distribution ofice-poor permafrost is significant for permafrost modelling in differentclimate conditions and regions. Indicating temperatures of ice-poorpermafrost and distinguishing between ice-poor and ice-rich permafrost on anational permafrost map provides new information for users.
机译:Mountain Permafrost是看不见的,并映射它是静止的挑战。可用的Modafrost分销地图通常高估ThePermRost范围,并在普利弗氏乳房分区中包含大型永久性区域。此外,由富含冰冰川或冰塔卢斯斜坡等富含冰块的富羊毛冻结特征的较低带的表示可能是挑战性的。这些问题是由于在冰墙上的成因和热特征中的考虑引起,例如在岩壁中发生,而富含冰冻的永久冻土。冰穷永久冻土显示出升高和潜在的传入的太阳辐射,冰 - 丰富的地面不显示这种相关性。取而代之的是,的富含冰的地面的分布通过重力过程iscontrolled如地面iceby的从覆盖有距骨雪崩存款orglacierets搬迁多年冻土蠕变或通过地面冰成因。因此,我们开发了一种映射方法,该方法区分了冰川富含冰冻的永久冻土,并为整个瑞士阿尔卑斯山进行了测试。 Forice-Point Ground我们发现了一种基于高度和势入口的太阳辐射的线性回归公式,其预测多个深度的钻孔研磨术,精度高于0.6μC。富含冰冻的永久冻土区域是通过建模高山质量浪费工艺的沉积酮来定义的。这种双重方法允许无毛冻土腰带的图表表示,其在Permafrost下方和下方。这使得能够高品质的Permafrostmodelling,如我们地图的验证所示。两个相当简单的连接因素,仰角(作为proxyfor年平均空气温度)和太阳辐射,在分配ofice贫冻土的dominatinginfluence是用于differentclimate条件和地区永久冻土建模显著。表明冰川覆盖物的温度和区分Analation Modafrost地图上的冰穷人和冰富冰冻冻土提供了对用户的新信息。

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