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首页> 外文期刊>Icarus: International Journal of Solar System Studies >Evidence for Amazonian northern mid-latitude regional glacial landsystems on Mars: Glacial flow models using GCM-driven climate results and comparisons to geological observations
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Evidence for Amazonian northern mid-latitude regional glacial landsystems on Mars: Glacial flow models using GCM-driven climate results and comparisons to geological observations

机译:火星亚马逊河北半球中纬度区域冰川系统的证据:使用GCM驱动的气候结果的冰川流模型以及与地质观测的比较

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摘要

A fretted valley system on Mars located at the northern mid-latitude dichotomy boundary contains lineated valley fill (LVF) with extensive flow-like features interpreted to be glacial in origin. We have modeled this deposit using glacial flow models linked to atmospheric general circulation models (GCM) for conditions consistent with the deposition of snow and ice in amounts sufficient to explain the interpreted glaciation. In the first glacial flow model simulation, sources were modeled in the alcoves only and were found to be consistent with the alpine valley glaciation interpretation for various environments of flow in the system. These results supported the interpretation of the observed LVF deposits as resulting from initial ice accumulation in the alcoves, accompanied by debris cover that led to advancing alpine glacial landsystems to the extent observed today, with preservation of their flow texture and the underlying ice during downwasting in the waning stages of glaciation. In the second glacial flow model simulation, the regional accumulation patterns predicted by a GCM linked to simulation of a glacial period were used. This glacial flow model simulation produced a much wider region of thick ice accumulation, and significant glaciation on the plateaus and in the regional plains surrounding the dichotomy boundary. Deglaciation produced decreasing ice thicknesses, with flow centered on the fretted valleys. As plateaus lost ice, scarps and cliffs of the valley and dichotomy boundary walls were exposed, providing considerable potential for the production of a rock debris cover that could preserve the underlying ice and the surface flow patterns seen today. In this model, the lineated valley fill and lobate debris aprons were the product of final retreat and downwasting of a much larger, regional glacial landsystem, rather than representing the maximum extent of an alpine valley glacial landsystem. These results favor the interpretation that periods of mid-latitude glaciation were characterized by extensive plateau and plains ice cover, rather than being restricted to alcoves and adjacent valleys, and that the observed lineated valley fill and lobate debris aprons represent debris-covered residual remnants of a once more extensive glaciation.
机译:位于北半球中纬度二分法边界的火星上的一个带锯齿状的山谷系统包含带衬里的山谷填充物(LVF),其内部具有广泛的似流特征,被认为是冰川起源。我们使用与大气普通循环模型(GCM)关联的冰川流模型对这种沉积物进行了建模,其条件与冰雪的沉积量一致,足以解释解释的冰川作用。在第一个冰川流动模型模拟中,仅在壁co中对源进行了建模,并且发现其与系统中各种流动环境的高山山谷冰川形成解释相一致。这些结果支持了对观测到的LVF沉积物的解释,这些沉积物是由于壁ice中最初的冰积聚,并伴随着碎屑覆盖而导致的,从而使高山冰川土地系统发展到今天所观察到的程度,并保留了它们在冰川消融期间的流动结构和底层冰层。冰川消退的阶段。在第二次冰川流动模型模拟中,使用了由GCM预测的与冰川期模拟相联系的区域累积模式。这种冰川流动模型模拟产生了一个更大范围的厚冰积聚区域,并在高原和二分法边界周围的区域平原上形成了明显的冰川作用。冰川融化导致冰层厚度减小,流向集中在有褶皱的山谷上。当高原流失冰块时,山谷的陡崖和悬崖以及二分法的边界墙都暴露在外,这为生产岩石碎片覆盖物提供了巨大的潜力,该岩石碎片覆盖物可以保留当今的地下冰层和地表流型。在此模型中,带衬里的山谷填充物和叶状碎屑围裙是更大面积的区域冰川土地系统最终撤退和消减的产物,而不是代表高山山谷冰川土地系统的最大范围。这些结果支持以下解释:中纬度冰川期的特征是高原和平原冰雪覆盖广泛,而不是局限于凹室和邻近的山谷,并且观察到的带衬里的山谷填充物和叶状碎屑围裙代表了残骸覆盖的残存残of。再次大范围的冰川化。

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