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首页> 外文期刊>Journal of sedimentary research >Sand-water flows on cold-climate eolian dunes: Environmental analogs for the eolian rock record and martian sand dunes
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Sand-water flows on cold-climate eolian dunes: Environmental analogs for the eolian rock record and martian sand dunes

机译:风寒沙丘上的沙水流动:风沙记录和火星沙丘的环境类似物

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Sand-water flows were observed on the slopes of cold-climate eolian dunes in southwestern Saskatchewan, Canada, during episodes of intense thawing in the winters of 2004 and 2005. Meltwater produced flows with varying grain-water contents on slopes of active blowout hollows and parabolic dunes. The sand-water flows emplaced small, structureless, lobate- and tongue-shaped deposits and alluvial fans. The greatest concentration of deposits occurred on south-facing slopes, which frequently thaw in winter from intense insolation. Transport modes ranged from high-density, viscous slurry flows to low-density, hyperconcentrated flows. The triggering cause of these flows is high pore-water pressure that develops in thawed near-surface sand due to impeded infiltration by frozen sand with pore ice at depth. These observations broaden the environmental context of sand-water flows on dunes and contribute to interpretations of these deposits in the eolian rock record and to recent alluvial features observed on Martian sand dunes.
机译:在2004年和2005年冬季,加拿大萨斯喀彻温省西南部的冷气候风沙丘斜坡上观察到了沙水流。在活跃的喷吹空洞和斜坡上,融化水产生了不同谷物水含量的流。抛物线沙丘。沙水流包裹着小的,无结构的,叶状和舌状的沉积物和冲积扇。沉积物的最大浓度出现在朝南的山坡上,在冬季,由于强烈的日照,它们经常融化。输送模式的范围从高密度,粘性浆液流到低密度,高浓度流。这些流动的触发原因是融化的近地表砂由于在深层有孔隙冰的冻结砂的渗透受阻而产生高孔隙水压力。这些观测结果拓宽了沙丘上沙水流动的环境背景,有助于解释风积岩记录中的这些沉积物,并有助于在火星沙丘上观测到最近的冲积特征。

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