Sand-water flows on cold-climate eolian dunes: Environmental analogs for the eolian rock record and martian sand dunes

被引:15
|
作者
Hugenholtz, Chris H. [1 ]
Wolfe, Stephen A.
Moorman, Brian J.
机构
[1] Univ Calgary, Dept Geol & Geophys, Calgary, AB T2N 1N4, Canada
[2] Geol Survey Canada, Nat Resources Canada, Ottawa, ON K1A 0E8, Canada
[3] Univ Calgary, Dept Geog, Calgary, AB T2N 1N4, Canada
关键词
D O I
10.2110/jsr.2007.063
中图分类号
P5 [地质学];
学科分类号
0709 ; 081803 ;
摘要
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.
引用
收藏
页码:607 / 614
页数:8
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