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1.
A series of experiments was conducted to determine the potential for aeolian abrasion of natural dune sands to produce fine particles (< 125 µm) by (1) the release of resident fines; (2) spalling, chipping and breakage of particles; and (3) the removal of grain surface coatings. Parent samples were obtained from the surfaces of four active continental dunes and abraded using a glass ‘test tube’ chamber for up to 120 h. The fine particles produced by this abrasion process were trapped at varying time intervals and subject to detailed particle‐size analyses using a Coulter Multisizer. The abrasion of untreated parent samples produced fine particles in one of two main size classes, < 10 µm and > 50 µm, but when the parent sample was sieved to exclude particles < 250 µm, relatively more material in the range 10–50 µm was produced. For unsieved parent samples, the size range associated with the dominant mode varied according to the length of the abrasion time. The coarsest mode (> 63 µm) was dominant during the first 16 h of abrasion, then became less significant and is thought to be associated with the release of resident fines into suspension. The finest mode (< 10 µm) was absent or very weak during the first 16 h of abrasion, then became more significant and, in some instances, dominated the distribution as abrasion continued. Removal of grain surface coatings is the main source of fine material < 10 µm, and this may be a significant source of fine material in areas where sands are dominated by subrounded and rounded particles. By comparison with previous studies of aeolian particle abrasion, these natural dune sands produced very low quantities of fine material (by weight), but their spatial extent makes them potentially a significant source of dust‐sized particles at the global scale.  相似文献   

2.
A series of experiments to determine the direct emission of dust-sized particles from Gobi surfaces by clean wind (wind without sand), and the potential for aeolian abrasion of Gobi surfaces and beds of gravel and mobile sand to produce fine (<100 μm) and dust-sized (<10 μm, PM10) particles under sand-laden winds were conducted. Parent material was obtained from Gobi areas of the Ala Shan Plateau, the region with high dust emissions in arid China. The fine particles produced by aeolian processes were collected using sand traps and sieved the captured materials to exclude particles >100 μm in diameter and then PM10 by sedimentation was acquired. The Gobi surface provided most of the emitted fine particles during the initial dust emission processes, but subsequently, release of the clay coatings of particles by abrasion becomes the dominant source of fine materials. Under sand-laden winds, PM10 production rates produced by aeolian abrasion of Gobi surfaces ranged between 0.002 and 0.244% of blown materials. After removal of sand, silt, or clay with low resistance to erosion from the Gobi surfaces by the wind, the PM10 production rates caused by aeolian abrasion were similar to those from gravel and sand beds. The results also indicated that after the dust-sized particles with low resistance to erosion were removed, the production of dust-sized particles was unrelated to wind velocity. Under aeolian processes, Gobi deserts in this region therefore play a major role in dust emissions from arid and semiarid China.  相似文献   

3.
Quaternary desert loess and sandstone-loessite relationships in the geological record raise questions regarding causes and mechanisms of silt formation and accretion. In the northern Sinai-Negev desert carbonate terrain, only sand abrasion in active erg could have produced the large quantities of quartzo-feldspathic silts constituting the late Quaternary northwestern Negev loess. In the continuum of source (medium to fine sand of dunes) to sink (silts in loess) the very fine sand is unaccounted for in the record. This weakens the sand abrasion model of silt formation as a global process. Here, we demonstrate that, as predicted by experiments, abrasion by advancing dunes generated large quantities of very fine sand (60-110 μm) deposited within the dune field and in close proximity downwind. This very fine sand was generated 13-11 ka, possibly synchronous with the Younger Dryas under gusty sand/dust storms in the southeastern Mediterranean and specifically in the northern Sinai-Negev erg. These very fine sands were washed down slope and filled small basins blocked by the advancing dunes; outside these sampling basins it is difficult to identify these sands as a distinct product. We conclude that ergs are mega-grinders of sand into very fine sand and silt under windy Quaternary and ancient aeolian desert environments.  相似文献   

4.
Dry lakes, degraded sandy grasslands, abandoned farmland and mobile dunes which are widely distributed throughout the arid areas of northern China have been investigated in this work. Gain-size distribution of the surface sediments of Manas lake in Junggar basin, Juyan lake in the Alxa plateau, Zhuye lake in Minqin basin and most deserts (such as Mu Us desert, Otindag desert, Horqin desert and Hulun Buir desert) in China have been analyzed. The results show clay with particle sized <10 μm on the surface sediments of dry lakebed and sandy grassland developed from dry lakebed, respectively, account for >60% and ∼50% of the total mass. Since the tiny particles on the surface of abandoned farmland are blown away easily and rapidly, the content of clay particles in Minqin basin is <14%. The grain-size distribution of mobile dunes in northern China mainly consists of particles >63 μm and few particles <10 μm. Consequently, although sand/dust storms originate primarily in the western deserts, the gobi areas of the Alxa plateau, the north and east of Hexi Corridor and in central Mongolia, the widely distributed dry lakebeds, sandy grasslands and abandoned farmland adjacent to the deserts also contribute to aeolian dusts. Hence, the material sources for sand dust storm in East Asia include inland deserts, but also dry lakes, sandy grasslands and abandoned farmland, which are widely distributed throughout the arid inlands of northern China.  相似文献   

5.
《Sedimentology》2018,65(4):1322-1330
This study examines the role of quartz sand in the production of dust using mixtures of quartz sand from the Sahara and diatomite aggregates from the Bodélé Depression in Chad. An aeolian abrasion chamber is used to reproduce the physical processes of aeolian abrasion and test the hypothesis that the breakdown of saltating diatomite flakes as they collide in saltation, and with the surface, is the most prolific mechanism of dust production (auto‐abrasion). This hypothesis is tested against the competing hypothesis that a hard, higher‐density quartz sand impactor is required to abrade fine‐grained sediments to generate dust. The results show that dust can be produced by a mixture of saltating diatomite and quartz sand particles. However, quartz sand is not required for saltating aggregates to produce dust. Indeed, these results, which used a mixture of very coarse‐grained aggregate (1 to 2 mm diameter) with fine quartz sand, indicate that the addition of quartz sand can decrease dust production. For a very coarse aggregate (1 to 2 mm), a pure diatomite aggregate produced the most dust, although using a coarse‐grained aggregate (0·5 to 1·0 mm) with a mixture of 20% quartz and 80% aggregate was found to produce the most dust overall. The results of this study confirm the auto‐abrasion hypothesis for the breakdown of diatomite particles in the Bodélé Depression, which is the single biggest source of atmospheric mineral dust on Earth.  相似文献   

6.
Creep and saltation are the primary modes of surface transport involved in the fluid‐like movement of aeolian sands. Although numerous studies have focused on saltation, few studies have focused on creep, primarily because of the experimental difficulty and the limited amount of theoretical information available on this process. Grain size and its distribution characteristics are key controls on the modes of sand movement and their transport masses. Based on a series of wind tunnel experiments, this paper presents new data regarding the saltation flux, obtained using a flat sampler, and on the creeping mass, obtained using a specifically designed bed trap, associated with four friction velocities (0·41, 0·47, 0·55 and 0·61 m sec?1). These data yielded information regarding creeping and saltating sand grains and their particle size characteristics at various heights, which led to the following conclusions: (i) the creeping masses increased as a power function (q = ?1·02 + 14·19u*3) of friction wind velocities, with a correlation (R2) of 0·95; (ii) the flux of aeolian sand flow decreases exponentially with increasing height (q = a exp(–z/b)) and increases as a power function (q = ?26·30 + 428·40 u*3) of the friction wind velocity; (iii) the particle size of creeping sand grains is ca 1·15 times of the mean diameter of salting sand grains at a height of 0 to 2 cm, which is 1·14 times of the mean diameter of sand grains in a bed; and (iv) the mean diameter of saltating sand grains decreases rapidly with increasing height whereas, while at a given height, the mean diameter of saltating sand grains is positively correlated with the friction wind velocity. Although these results require additional experimental validation, they provide new information for modelling of aeolian sand transport processes.  相似文献   

7.
Grain size analyses of three hilltop, primary eolian loess sequences in the Negev desert, southern Israel, show a bimodal grain-size distribution at 50-60 μm and 3-8 μm. Using analyses of mineralogy and OSL ages we demonstrate that the coarse mode is composed mostly of quartz grains and its relative magnitude increases regionally with time, suggesting an enhancement of a time-transgressive proximal dust source compared to a distal, Saharan fine-grain dust. The only proximal dust source for large amount of coarse silt quartz grains is the sands that advanced into Sinai and the Negev concurrently with the loess accretion during the late Pleistocene as a result of the exposure of the Mediterranean shelf. We therefore propose that the coarse silt quartz grains were formed through eolian abrasion within the margins of an advancing sand sea. This relationship between desert sand seas as a source for proximal coarse dust and desert margin loess deposits can be applicable to other worldwide deserts such as Northern Africa, China and Australia.  相似文献   

8.
猪野泽全新世沉积物剖面中存在砂层和灰绿色湖相沉积层相间分布的现象。本研究对猪野泽QTH01、QTH02剖面砂层的石英砂样品进行扫描电镜分析,且与古湖泊岸堤和现代沙丘砂样做了对比,探讨了猪野泽全新世剖面中部和底部砂层的成因。研究发现,猪野泽QTH01、QTH02剖面样品中大部分石英砂兼具风成结构和水成结构,且水成特征大都覆盖于风成特征之上,V型坑分布频率相对较小,磨圆度特征与现代沙丘样品较为相似,与岸堤石英砂具有相似的结构特征,但剖面砂层不具岸堤典型的斜纹层理。结果说明,猪野泽砂层先经历了风成环境,后期转向湖相沉积,也有少部分砂是通过河流沉积于剖面位置;剖面砂层与岸堤砂层的成因相似,但剖面所在位置并非湖泊岸堤;剖面砂层形成时期风沙活动强烈,湖泊水动力条件稳定,河流对湖泊影响较小。  相似文献   

9.
FIKRY KHALAF 《Sedimentology》1989,36(2):253-271
Several types of aeolian deposits have been recognized in Kuwait: (a) smooth sand sheets that resemble desert floor sand, (b) immobile sands that include rugged vegetated sand sheets and wadi fill deposits, and (c) mobile sands that form active sand sheets and sand dunes. Simple size frequency curves illustrate the genetic relationship between the various aeolian sediment types. The four size parameters, namely, mean size, sorting, skewness and kurtosis, were calculated. Scatter plot diagrams of sorting versus mean size and sorting versus kurtosis are effective in differentiating smooth sand sheet deposits from dune sands. Active sand sheet deposits can also be recognized because they are usually located between the two end members–smooth sand sheets and dune sands. Size parameters change with location regardless of their types. Coarsening and positive skewness usually increase downwind. Mineralogical and textural characteristics of the aeolian deposits in Kuwait revealed that they are mostly derived from the lower Mesopotamian muddy flood plain deposits, the sand fraction of the Al-Dibdibba gravelly deposits and the disintegrated material from calcretic and gypcretic duricrusts. Distribution of depositional and deflational areas indicates that the northern desert of Kuwait is characterized by a positive sand budget, whereas the southern desert has a negative sand budget.  相似文献   

10.
董玉祥 《沉积学报》2002,20(4):656-662
现代海岸风成砂的粒度特征是海岸风沙研究的重要问题,本文以我国温带海岸为研究区域,利用 136个现代海岸风成砂样数据,通过粒度组成、平均粒径、标准偏差和偏差、峰态等粒度参数分析了其粒度特征。结果表明,我国温带海岸的现代风成砂并非过去认为的几乎全由分选很好的细砂组成,是以正偏为主,粒度参数的地域差异明显,并随沙丘类型、规模及距海岸线的远近不同等而变化。与海滩砂比较,风成砂具有普遍含有粉沙、略细、多正偏、峰态偏窄等特点,但利用粒度参数散点图和因子分析法二者均无法区分。我国温带海岸现代海岸风成砂粒度参数的上述特征与其特有的发育条件和演化过程密切相关,其中主要与季风气候特征显著、形成时间短、风力作用时间有限以及风沙活动空间狭小并受到水力与重力作用的干扰等有关。  相似文献   

11.
Deserts are one of the most important dust sources in the world. Because dust content changes as a function of height at low levels in the atmosphere, this affects long‐term dust transport. In this paper, field data measured above shifting sands in the south‐eastern Tengger Desert were used to analyse the vertical distribution of sediment fluxes in the near‐surface layer (0 to 48 m). It was possible to express horizontal sediment flux as a power function, but aeolian deposition as a function of height could be expressed as an exponential function. There are two curve types for the particle size distributions in the horizontal sediment flux and aeolian deposition: bimodal and unimodal curves. For the horizontal sediment flux and aeolian deposition, heights of 24 m and 32 m, respectively, were the key heights in the size distribution curve; below these heights, the curve was bimodal, whereas above these heights, it was unimodal. At heights of 4 to 16 m, and especially between 8 m and 12 m, the data were particularly interesting because the sediment size, transport mode, degree of sorting, and the skewness and kurtosis change. For the horizontal sediment flux, wind turbulence moved saltating particles higher than expected.  相似文献   

12.
基于微观结构的青藏高原风积沙导热系数变化机理研究   总被引：1，自引：0，他引：1  
陈琳  喻文兵  杨成松  易鑫  刘伟博 《冰川冻土》2014,36(5):1220-1226
风积沙作为青藏高原一种重要的局地因素, 改变了多年冻土的赋存条件. 风积沙的导热系数特征对预报分析其对冻土赋存有利或者不利具有重要作用. 采用非稳态法对青藏高原红梁河风积沙进行了导热系数测试, 并结合电镜扫描/能谱分析, 从微观结构的角度探讨了风积沙的导热系数变化机理. 结果表明: 研究区风积沙平均粒度为242.427 μm; 标准偏差值为0.125, 分选极好; 偏度为0.359, 接近对称; 峰度值为1.086, 峰态中等; 颗粒粒径主要分布在75～500 μm之间, 沙粒均匀, 不含黏土及砾石成分, 自然堆积状态下其孔隙率为0.391. 天然状态下的风积沙颗粒呈类球形, 颗粒磨圆度高, 点与点接触, 颗粒间孔隙较大; 表面有明显撞击坑和擦痕, 这导致颗粒的比表面积增大, 连通性增强, 孔隙率增加. 干燥状态下风积沙颗粒的相互接触面积较小, 孔隙由空气填充, 导热系数较低; 而在湿润状态下, 正温时孔隙中的水间接增大了风积沙的接触面积, 导致其导热系数增大; 负温时, 孔隙内的水变成冰, 从而导致导热系数进一步增大. 天然状态下, 暖季地表风积沙含水量较低, 导热系数较低, 而冷季地表风积沙含水量较大, 导热系数较大. 此外, 风积沙为颗粒物质, 表面光滑, 颗粒之间粘性小, 孔隙未被填堵, 结构松散, 这些因素导致自然堆积状态下其渗透系数较一般细砂大, 透水性良好, 保水性差, 是防冻胀较好的换填材料.  相似文献   

13.
长春市城区近地表灰尘粒度特征及其环境意义   总被引：1，自引：0，他引：1  
为剖析长春市城区近地表灰尘粒度特征,分别沿南北和东西轴线采集了34件城市近地表灰尘样品,采用激光粒度仪对样品进行了粒度测试分析。结果表明：长春市近地表灰尘颗粒物平均中值粒径和算术平均粒径分别为21.58 μm和24.24 μm,分选极差;以粗粉粒（10.00～80.00 μm）为主,平均约占71.28%,黏粒组（<5.00 μm）和细粉粒组（5.00～10.00 μm）分别约占14.75%和13.05%。频率曲线呈正偏双峰型分布,峰态中等偏窄,与现代尘暴和城市街道灰尘分布特征相一致,反映出其起源的多元性和相对稳定性,表明近地表灰尘沉积仍是风积作用的继续。近地表灰尘颗粒物粒径均小于100.00 μm,极易在外动力条件下再次扬起并悬浮搬运,PM10和PM2.5所占比例分别为27.76%和7.32%,其生态环境效应不应被忽视。粒径分布无显著空间变化,但城市中心区域粒径变化范围小,这可能说明城市边缘区域较中心区域近地表灰尘的起源更具多源性和复杂性。  相似文献   

14.
风积沙作为路基填料的静力特性研究   总被引：3，自引：0，他引：3  
张生辉  李志勇  彭帝  陈忠明 《岩土力学》2007,28(12):2511-2516
风积沙颗粒细小、级配差、无粘性。使用风积沙作为沙漠公路的路基填料具有与一般路基填料不同的力学性质。选用新疆、内蒙、陕西3省（区）典型风积沙,进行了原材料的级配、天然含水量、相对密度等试验。在此基础上进行了风积沙的CBR、回弹模量、压缩以及室内剪切试验。根据风积沙的特性制定了有别于常规的试验仪器和试验方法。利用图表和回归分析的方法分析了风积沙的贯入压力-贯入应变、单位压力-回弹变形、垂直压力-抗剪强度、压力-压缩模量等性质。考虑到沙漠地区干旱少雨的特点,试验过程中对于风积沙采用了不同的干密度和含水量,得出了不同压实标准情况下的“沙基应力-变形特性”。  相似文献   

15.
Major-element composition, mineral composition and grain-size distribution have been studied for Quaternary aeolian sediments from the Taklimakan Desert, north-western China, together with the variation of chemical and mineralogical compositions of different grain-size fractions. Aeolian sediments from the Taklimakan Desert have higher ratios of feldspar/quartz and calcite/quartz, finer grain size, poorer roundness of quartz and feldspar grains and lower abundances of frosted quartz, than found in aeolian sediments from other deserts such as the Saudi Arabian Desert. In spite of these immature mineralogical and sedimentological features, the aeolian sediments from the Taklimakan Desert show low regional variations in major-element and mineral compositions and are homogenized. These observations confirm that two processes, glacial activity within surrounding mountains and aeolian activity at the Tarim Basin, are important in the homogenization of the Taklimakan Desert sands. Taklimakan Desert sediments are constantly and effectively supplied from basement rocks in the surrounding mountains by glacial erosion. The supplied sediments are further homogenized by aeolian activity in the desert and are partly blown away, serving as the source of Chinese aeolian loess. Compositional differences are observed between loess (mainly 10–40 μm particles) and the <45 μm fraction of the Taklimakan Desert sediments, as well as between loess and whole rock of the Taklimakan Desert sediments. These observations provide constraints for precise modelling of loess formation, and for assessment of the chemical composition of the upper continental crust based on the chemical composition of aeolian loess.  相似文献   

16.
Twenty-one surficial sand samples from the Altar Desert coastal and desert dune systems were analysed for rare earth elements (REE) content. This was done to observe the provenance signatures for four strategic dune localities near the Colorado River Delta, the El Pinacate dune fields, and the beaches of the north of the Gulf of California in the state of Sonora, Mexico. Our goals are to show which mechanisms (i.e., aeolian, marine) exert more influence on the composition of the Altar Desert dune sands. This study also shows the usefulness of REE spatial distribution to determine the relative mobility of the sand. Some sand samples from the dune systems in San Luis Río Colorado (SLRC), Golfo de Santa Clara (GSC), and Puerto Peñasco (PP) displayed dissimilar REE concentrations with respect to the rest of the sand samples from the same sites. These differences can be related to short aeolian transport distance in the sands with high REE concentrations and long aeolian transport distance in the sands with low REE concentrations. Besides, high REE concentration in the sands might be due to their closeness to the Colorado River Delta sediments and to recycled sands derived from granitic rocks. In contrast, all the sand samples from the El Pinacate (EP) site have similar REE concentration values, suggesting that the El Pinacate dune sands are influenced by more selective aeolian processes and less diverse heavy mineral content. The Altar Desert dune sands are derived from granitic sources eroded by the Colorado River. Our results also indicate that the Altar Desert dune sands are low in heavy mineral content (with the exception of Fe and Ti bearing minerals) and enriched in carbonates with phosphates (especially at the PP site) yielding poor correlations between REE and major element concentrations. The REE geographical distribution values in the Altar Desert dune sands indicate that light and heavy REE concentration values are related to aeolian transport, maturity of the sands, their low weathering rates, proximity of the source rocks, and the biogenic debris input from beach sands into the dune.  相似文献   

17.
长江中下游地区第四纪红土磁学特征及其环境意义   总被引：1，自引：0，他引：1  
通过采集长江中下游湖南长沙(CS)、岳阳(HN)、江西南昌(NC)、新余(XY)和浙江金华高村(GC)5个剖面不同层位的红土样品,对其粒度和多种磁学参数进行测量和分析,探讨了红土剖面随深度变化的成土作用强弱以及多磁学参数在揭示我国南方红土第四纪气候演化信息的价值。结果表明:①粒度分析显示,红黄土交接带(约28°~31°N)的CS、HN、NC、GC 4个剖面的红土粒度与北方黄土和下蜀黄土有很好的可比性,具有明显的风成特性;位置更偏南的XY剖面红土颗粒较粗,10~50 μm粒组富集不明显,具有典型的冲积相特征。②各红土剖面的多磁学参数分析表明,成土过程中产生的磁铁矿、磁赤铁矿和赤铁矿是红土磁性的主要载体。③同一红土剖面内,不同沉积结构的磁性矿物含量和组成具有很大差异。下部网纹红土中赤铁矿的含量较高,磁赤铁矿的含量较上覆均质红土或黄棕色土低,揭示了网纹红土形成于中国南方一个极端湿润期,长期剧烈的水分活动导致均质红土中磁赤铁矿的溶解和铁质的流失,同时较强的成土作用使强磁性的磁赤铁矿向弱磁性的赤铁矿转化,从而导致网纹红土的磁化率比上覆均质红土或黄棕色土低了一个数量级。④具有冲积相特征的XY剖面磁学特征与其他风尘成因红土(特别是NC剖面)差异甚大,可能成为它具有不同物质来源的一个佐证。  相似文献   

18.
The relation between the crystallography of artificially abraded quartz sand grains and aeolian surface textures has been studied using an X-ray precession camera and the scanning electron microscope (SEM). Crushed Brazilian quartz was sieved to between 250 and 350 μm, eroded in a paddle wheel device which simulated aeolian action at 8 m s?1 for 3 h, and photographed with the SEM. A typical grain was selected and over 1100 photographs were combined to create a 3 × 3 m photomosaic; because of the large size, it was possible to observe and measure the angular and linear relations between the various features. After the c axis direction in the grain was determined by precession X-ray analysis, the most important aeolian features were related to the crystallography of quartz. The upturned plates or cleavage plates probably represent traces parallel to r(10ī1) and z(01ī1) cleavages in quartz. Blocky areas appear to be an expression of a cleavage parallel to m(10ī0). In addition, plate spacing on thirty-five experimental, modern, and ancient quartz sand grains is fairly constant. Assuming that abrasion in most sedimentary environments acts in the same manner with respect to quartz crystallography, much of the fine silt and clay in sediments and sedimentary rocks may be the result of cleavage following abrasion parallel to the r and z cleavage planes, while the less common blocky particles are probably the result of cleavage parallel to the m planes.  相似文献   

19.
海南岛东北海岸风沙沉积的光释光年代学意义   总被引：1，自引：0，他引：1  
选取海南岛东北部JSD2和PQR2两个典型海岸沙质沉积剖面进行研究,共采集10个测年样品和89个指标分析样品,在室内进行了光释光（OSL）测年和粒度分析。结果表明:1）JSD2和PQR2剖面砂样以中细沙为主,粒度众数在225~400 μm之间。风沙沉积后受化学风化作用呈现淡红棕色至红棕色;2）JSD2剖面OSL年龄范围为（2.20±1.09）~（9.89±1.65） ka,属于全新世风沙沉积;PQR2剖面年龄范围为（3.41±0.78）~（22.50±1.07） ka,上部为全新世风沙沉积,下部为末次冰期和晚冰期的老红砂层;3）综合海南岛和华南其他海岸沙丘、海岸风沙年龄数据分析,研究区全新世海岸风沙沉积年代序列可划分为10.5~6.0 ka B.P.和6.0 ka B.P.以来两个阶段,华南热带与亚热带海岸风沙活动趋势基本一致。  相似文献   

20.
首次对毛乌素沙地东南部边缘沙漠—黄土地带的土地沙漠化进行系统的地质学分类,提出了沙地内部就地起沙型沙漠化、河流谷地就地起沙型沙漠化、风化残积就地起沙型沙漠化和风沙侵入型沙漠化等四种土地沙漠化类型。通过深入分析不同地质成因类型土地沙漠化的粒度特征,探讨了不同地质作用对土地沙漠化的贡献及其对土地沙漠化防治方面的重要意义。研究表明,研究区的土地沙漠化以就地起沙型为主,河流的水力搬运是沙漠化物质搬运的主要途径,风力作用则是对河流湖泊沉积物的进一步分选和再沉积。最后,提出了不同类型的土地沙漠化防治对策建议。  相似文献   

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