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The effect of adsorbed liquid and material density on saltation threshold: Insight from laboratory and wind tunnel experiments

机译:吸附液体密度对盐水阈值的影响:实验室和风洞实验中的洞察力

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Saltation threshold, the minimum wind speed for sediment transport, is a fundamental parameter in aeolian processes. Measuring this threshold using boundary layer wind tunnels, in which particles are mobilized by flowing air, for a subset of different planetary conditions can inform our understanding of physical processes of sediment transport. The presence of liquid, such as water on Earth or methane on Titan, may affect the threshold values to a great extent. Sediment density is also crucial for determining threshold values. Here we provide quantitative data on density and water content of common wind tunnel materials (including chromite, basalt, quartz sand, beach sand, glass beads, gas chromatograph packing materials, walnut shells, iced tea powder, activated charcoal, instant coffee, and glass bubbles) that have been used to study conditions on Earth, Titan, Mars, and Venus. The measured density values for low density materials are higher compared to literature values (e.g., similar to 30% for walnut shells), whereas for the high density materials, there is no such discrepancy. We also find that low density materials have much higher water content and longer atmospheric equilibration timescales compared to high density sediments. We used thermogravimetric analysis (TGA) to quantify surface and internal water and found that over 80% of the total water content is surface water for low density materials. In the Titan Wind Tunnel (TWT), where Reynolds number conditions similar to those on Titan can be achieved, we performed threshold experiments with the standard walnut shells (125-150 pm, 7.2% water by mass) and dried walnut shells, in which the water content was reduced to 1.7%. The threshold results for the two scenarios are almost the same, which indicates that humidity had a negligible effect on threshold for walnut shells in this experimental regime. When the water content is lower than 11.0%, the interparticle forces are dominated by adsorption forces, whereas at higher values the interparticle forces are dominated by much larger capillary forces. For materials with low equilibrium water content, like quartz sand, capillary forces dominate. When the interparticle forces are dominated by adsorption forces, the threshold does not increase with increasing relative humidity (RH) or water content. Only when the interparticle forces are dominated by capillary forces does the threshold start to increase with increasing RH/water content. Since tholins have a low methane content (0.3% at saturation, [Curtis, D. B., Hatch, C. D., Hasenkopf, C. A., et al., 2008. Laboratory studies of methane and ethane adsorption and nucleation onto organic particles: Application to Titan's clouds. Icarus, 195, 792. http://dx.doi.org/10.1016/j.icarus.2008.02.003]), we believe tholins would behave similarly to quartz sand when subjected to methane moisture. (C) 2017 Elsevier Inc. All rights reserved.
机译:盐水阈值,沉积物运输的最小风速,是风海程过程中的基本参数。使用边界层风隧道测量该阈值,其中通过流动空气使粒子流动,对于不同行星条件的子集可以通知我们对沉积物运输物理过程的理解。液体的存在,例如土壤或甲烷上的水,可以在很大程度上影响阈值。沉积物密度也是确定阈值的至关重要。在这里,我们提供了普通风洞材料的密度和含水量的定量数据(包括铬铁矿,玄武岩,石英砂,海滩砂,玻璃珠,气相色谱包装材料,核桃壳,冰茶粉,活性炭,速溶咖啡和玻璃泡沫)已被用于研究地球,泰坦,火星和金星的条件。与文学值相比,低密度材料的测量密度值更高(例如,与核桃壳相似的30%),而对于高密度材料,没有这种差异。与高密度沉积物相比,我们还发现低密度材料具有更高的含水量和较长的大气平衡时间尺寸。我们使用热量标注分析(TGA)来量化表面和内水,发现超过80%的总含水量是低密度材料的地表水。在泰坦风隧道(TWT)中,可以实现与泰坦上类似的雷诺数条件,我们通过标准核桃壳(125-150pm,7.2%水质量)进行阈值实验,以及干核桃壳,其中水含量降至1.7%。两种情况的阈值结果几乎是相同的,这表明湿度在该实验制度中对核桃壳的阈值具有可忽略不计的影响。当水含量低于11.0%时,颗粒力量由吸附力支配,而在较高的值下,颗粒力颗粒颗粒是较大的毛细力。对于低平衡水含量的材料,如石英砂,毛细管力占主导地位。当颗粒力由吸附力支配时,阈值随着相对湿度(RH)或水含量的增加而不会增加。只有当颗粒力由毛细管力支配时,阈值开始随着Rh /含水含量的增加而增加。由于甲肾上腺素含量低(饱和度为0.3%,[Curtis,DB,孵化,Cd,Hasenkopf,Ca等,2008.甲烷和乙烷吸附和成核在有机颗粒上的实验室研究:在泰坦云的应用。 ICARUS,195,792。http://dx.doi.org/10.1016/j.icarus.2008.02.003]),我们相信当甲烷水分进行甲烷水分时,噻吩并将表现出与石英沙相似。 (c)2017年Elsevier Inc.保留所有权利。

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