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1.
Controls on the formation of coastal ventifacts 总被引：3，自引：0，他引：3
Jasper Knight 《Geomorphology》2005,64(3-4):243-253
Ventifacted boulders are present within the intertidal zone of a mixed sand and boulder beach in Gweebarra Bay, northwest Ireland. The boulders show features typical of wind abrasion by sand including polished surfaces, pits and grooves. Orientation of ventifact keels was measured and direction of prevailing winds responsible for ventifaction was inferred from a sample of 50 boulders in each of two adjoining locations on the beach (30 m apart). The keel orientations and inferred wind direction are both strongly clustered but results from each location differ by 90° from one another, and neither corresponds closely to the present-day regional wind regime. Since wind flow patterns were not significantly different during the Little Ice Age, when the ventifacts were likely formed, the orientation of ventifact keels cannot be used uncritically, as in many studies, as a proxy record of prevailing wind direction. It is likely that ventifact development in Gweebarra Bay was controlled by sediment availability rather than by wind direction. 相似文献
2.
An area north of Lake Fryxell in the Taylor Valley, Antarctica, was surveyed to determine the frequency of occurrence of rocks that show strong evidence of wind abrasion and ventifaction, which is defined here as rocks having well-developed faceting, to define their relative abundance in this area of the ice-free McMurdo Dry Valley system and to provide an indication of the role of wind as a geomorphic agent in this area. The orientation of abrasion-caused features (facets, keels, and grooves) with respect to the present day wind regime is also described. Rocks were examined on five linear transects ranging from 300 to 510 m in length. A total of 1324 rocks were examined. On average, 60% of all rocks exhibited distinct wind abrasion features with polish being the most common feature and polished rocks were distributed equally between survey lines, suggesting abrasion was ubiquitous in the study area. Approximately 4% of the rocks had distinct facets and/or keels, and fine-grained ultramafic peridotite-type rocks produced the most finely-featured forms (i.e., sharp facet edges and keels). A larger percentage, ≈ 12.5%, had grooves. Grooves were typically associated with a tabular form of mafic diabase-type igneous rock. The distribution of faceted ventifacts and grooved rocks was not uniform for the five transects, suggesting that the distribution mechanism for the surface rocks and the source areas determined, to a large extent, what form of ventifact could be produced at a location. The orientation of the grooves and dip directions of the facets indicates the direction of the abrasive winds had a strong westerly component, which coincides with the modern wind regime of winter katabatic flows that move down valley toward the Ross Sea. The orientation of the facets and grooves suggests that the rate of formation of the ventifacts proceeds at a pace greater than other surficial processes (e.g., down-slope soil movement, cryoturbation), which should tend to remove trends in the facet and groove orientations, or that the down-slope movement of the surface is approximately perpendicular to the wind allowing preservation of the alignment. 相似文献
3.
Julie E. Laity 《自然地理学》2013,34(2):113-132
I nvestigations into processes of ventifact formation in the east-central Mojave Desert, California confirm the importance of topography as a control in the location, orientation, and intensity of ventifact abrasion. Ventifacts in the region appear to be relict in nature and probably formed during a period that ended several thousand years ago. Comparison of groove orientations with available wind data shows that regional flow direction has not changed in the recent past. Although west to northwest winds are the most frequent and intense, and therefore dictate the regional erosion pattern, low to moderate southeasterly flow is recorded on ventifacts near the crests of hills owing to the effects of velocity acceleration. Two conditions that affect ventifact development are considered in this paper: (1) wind acceleration through topographic constrictions; and (2) wind acceleration up the windward flanks of hills. Constrictions in the Barstow-Bristol trough allowed velocity increases that resulted in ventifaction on 70–90 percent of all exposed cobbles and boulders. Velocity acceleration towards the crests of hills caused a marked increase in sand transport and resultant abrasion, as expressed by increases in groove and pit dimensions. [Key words: Aeolian geomorphology, ventifacts, Mojave Desert, California.] 相似文献
4.
《Geomorphology》2007,83(1-2):136-151
The Schmidt Rock Test Hammer was used to study the effect of abrasion on shore platforms in Galicia, northwestern Spain. On platforms where tidally-induced weathering (salt, wetting and drying, etc.) is dominant, rock strength is significantly lower than in areas where abrasion is, or has been active in the recent past. This suggests that abrasion removes weathered surface material, exposing the stronger, less weathered rock below. Abrasion downwearing, measured with a transverse micro-erosion meter, ranged between 0.13 and 1.8 mm yr− 1 over the last year. Most active abrasion occurs in the upper part of the intertidal zone, but weathering is slowly destroying formerly abraded surfaces at lower elevations. These abandoned surfaces were abraded by materials supplied by erosion of fluvio-nival and periglacial slope deposits that covered, or partially covered, parts of the Galician coast during the middle and late Weichselian. During the Holocene, rising sea level and erosion of the slope deposits caused the abrasion zone to gradually migrate up to its present position near the high tidal level. The spatial and temporal role of abrasion on this coast is, therefore, closely associated with the exhumation and inheritance of ancient platform surfaces from beneath Weichselian deposits. 相似文献
5.
6.
Numerical simulation of aeolian dusty sand transport in a marginal desert region at the early entrainment stage 总被引：2，自引：0，他引：2
Aeolian dusty sand transport in the marginal region of a desert is described numerically from first suspension motion at the early entrainment stage to the unsteady state within a moderate range (1000 m long × 500 m high). A two-dimensional model is built for wind-blown dust flow, and the calculations are carried out using Fluent software. The simulation results describe an integrated picture of aeolian dusty sand transport including uplift, suspension, diffusion, deposition and its space–time concentration. According to the features of a sand–dust storm near the surface, a volume concentration expression of ejection grains is developed as a boundary condition in the simulation approach. The model is verified by comparing results with both experimental data from a wind tunnel and an analytic solution. Uniform dust sizes and R–R distributions are used in the simulation. Gas–solid two-phase flow patterns with these grains are obtained in the downwind space, including the turbulence intensity, gas phase stream functions and solid volume concentration distributions. The influence of wind velocities and grain sizes is analyzed. From the simulation results, spatial distributions of dust volume concentration in the early entrainment stage are described clearly. Different from coarse sands, there is a clear band of uniformly saturated dust concentration in the region directly above the surface. 相似文献
7.
Kenneth S. Edgett Rebecca M. E. Williams Michael C. Malin Bruce A. Cantor Peter C. Thomas 《Geomorphology》2003,52(3-4):289-297
Lithology and physical properties of strata exposed at the Earth's surface have direct influence on the erosion and geomorphic expression of landforms. While this is well known on our planet, examples on Mars are just coming to light among the tens of thousands of airphoto-quality images (resolutions 1.5–12 m/pixel) acquired since 1997 by the Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC). Specific examples occur among martian north polar layered materials, which MOC images reveal are divided into two distinct stratigraphic units: a lower, dark-toned layered unit and a younger, upper, lighter-toned layered unit. The lower unit is less resistant to wind erosion than the upper unit. The upper unit most likely consists of stratified dust and ice, while the lower unit contains abundant, poorly cemented sand. Sand is more easily mobilized by wind than dust; the lower resistance to erosion of the lower unit results from the presence of sand. Where wind erosion in polar troughs has penetrated to the lower unit, geomorphic change has proceeded more rapidly: sand has been liberated from the lower unit, and arcuate scarps have formed as the upper unit has been undermined. Wind erosion of the lower unit thus influences the geomorphology of the north polar region; this result likely explains the genesis of the large polar trough, Chasma Boreale, and the relations between dunes and arcuate scarps that have puzzled investigators for nearly three decades. The properties of the stratigraphic units suggest that the upper limit for the amount of water contained in the north polar layered materials may be 30–50% less than previously estimated. 相似文献
8.
Variable vegetation cover and episodic sand movement on longitudinal desert sand dunes 总被引：6，自引：0，他引：6
Longitudinal (linear) sand dunes of the Simpson and Strzelecki dunefields in eastern central Australia present a paradox. Low levels of activity today stand in contrast to luminescence dating which has repeatedly shown deep deposits of sand on dune crests dating to within the late Holocene. In order to investigate the nature of dune activity in the Simpson–Strzelecki dunefield, vegetation and sand mobility were investigated by detailed vegetation survey and measurement of rippled area and loose sand depth of dunes at three sites along a climatic gradient. The response of both vegetation and sand movement to inter-annual climate variability was examined by repeat surveys of two sites in drought and non-drought conditions. Projected plant cover and plant + crust cover were found to have inverse linear relationships with rippled area and the area of deep loose sand. No relationship was found between these measures of sand movement and the plant frontal area index. A negative exponential relationship between equivalent mobile sand depth on dune surfaces and both vascular plant cover and vascular + crust cover was also found. There is no simple threshold of vegetation cover below which sand transport begins. Dunes with low perennial plant cover may form small dunes with slip faces leading to a positive feedback inhibiting ephemeral plant growth in wet years and accelerating sand transport rates. The linear dunefields are largely within the zone in which plant cover is sufficient to enforce low sand transport rates, and in which there is a strong response of vegetation and sand transport to inter-annual variation in rainfall. Both ephemeral plants (mostly forbs) and crust were found to respond rapidly to large (> 20 mm/month) rainfall events. On millennial time-scales, the level of dune activity is controlled by vegetation cover and probably not by fluctuations of wind strength. Land use or extreme, decadal time-scale, drought may destabilise dunes by removing perennial plant cover, accelerating wind erosion. 相似文献
9.
沙粒的表面磨蚀效应是地表产尘、释尘的重要机制,针对干湖盆泥漠地表开展磨蚀释尘实验研究,对理解干湖盆地表风蚀过程及盐碱尘暴形成机理具有重要意义。对采自西居延海干涸湖盆泥漠地表土样进行室内磨蚀模拟实验,研究了不同粒级（细、中、粗）沙粒不同落沙角度（30°,45°,60°）的磨蚀效应。结果表明：（1）泥漠地表磨蚀实验中能够产生明显释尘效应的沙粒粒级阈值为中沙（0.25 mm<Md<0.50 mm）;（2）磨蚀粒径粒级相同时,磨蚀角度会对泥漠地表磨蚀释尘速率产生影响,磨蚀量的角度排序为60°>30°>45°,但同一粒级3种角度下的磨蚀释尘率差异不显著。（3）磨蚀角度为45°时,计算了泥漠地表的质量磨蚀率与能量磨蚀率,其中中沙为0.04 g·kg-1、0.43 g·J-1,粗沙为0.08 g·kg-1、0.74 g·J-1,极粗沙为0.26 g·kg-1、2.54 g·J-1;在磨蚀沙粒粒级倍增而磨蚀角度不变情况下,泥漠地表磨蚀释尘率与能量磨蚀率未发生正比例线性增长变化。 相似文献
10.
Calibration of the MDCO dust collector and of four versions of the inverted frisbee dust deposition sampler 总被引：2，自引：0，他引：2
Wind tunnel experiments were conducted to determine the efficiency of sediment samplers designed to measure the deposition of aeolian dust. Efficiency was ascertained relative to a water surface, which was considered the best alternative for simulating a perfectly absorbent surface. Two types of samplers were studied: the Marble Dust Collector (MDCO) and the inverted frisbee sampler. Four versions of the latter catcher were tested: an empty frisbee, an empty frisbee surrounded by an aerodynamic flow deflector ring, a frisbee filled with glass marbles, and a frisbee filled with glass marbles and surrounded by a flow deflector ring. Efficiency was ascertained for five wind velocities (range: 1–5 m s− 1) and eight grain size classes (range: 10–89 μm). The efficiency of dust deposition catchers diminishes rapidly as the wind speed increases. It also diminishes as the particles caught become coarser. Adding a flow deflector ring to a catcher substantially improves the catcher's efficiency, by up to 100% in some cases. The addition of glass marbles to a catcher, on the other hand, does not seem to increase the efficiency, at least not at wind velocities inferior to the deflation threshold. For higher velocities the marbles protect the settled particles from resuspension, keeping them in the catcher. The following five parameters determine the accumulation of aeolian dust in a catcher: the horizontal dust flux, the weight of the particles, atmospheric turbulence, resuspension, and the dust shadow effect created by the catcher. The final accumulation flux depends on the combination of these parameters. The catchers tested in this study belong to the best catchers currently in use in earth science and have been the subject of various aerodynamic studies to improve their efficiency. Nevertheless the catching efficiency remains low, in the order of 20–40% for wind speeds above 2 m s− 1. Other catchers suffer from the same low efficiencies. There is, thus, evidence to believe that dust deposition rates published in the aeolian literature and obtained by collecting the sediment in a catcher largely underestimate the true deposition. The errors are considerable, of the order of 100% and more. A reconsideration of the literature data on aeolian dust deposition measured by catchers is, therefore, required. 相似文献
11.
Velocity profile of a sand cloud blowing over a gravel surface 总被引：2，自引：0，他引：2
Particle dynamic analyzer (PDA) measurement technology was used to study the turbulent characteristics and the variation with height of the mean horizontal (in the downwind direction) and vertical (in the upward direction) particle velocity of a sand cloud blowing over a gravel surface. The results show that the mean horizontal particle velocity of the cloud increases with height, while the mean vertical velocity decreases with height. The variation of the mean horizontal velocity with height is, to some extent, similar to the wind profile that increases logarithmically with height in the turbulent boundary layer. The variation of the mean vertical velocity with height is much more complex than that of the mean horizontal velocity. The increase of the resultant mean velocity with height can be expressed by a modified power function. Particle turbulence in the downwind direction decreases with height, while that in the vertical direction is complex. For fine sands (0.2–0.3 mm and 0.3–0.4 mm), there is a tendency for the particle turbulence to increase with height. In the very near-surface layer (<4 mm), the movement of blown sand particles is very complex due to the rebound of particles on the bed and the interparticle collisions in the air. Wind starts to accelerate particle movement about 4 mm from the surface. The initial rebound on the bed and the interparticle collisions in the air have a profound effect on particle movement below that height, where particle concentration is very high and wind velocity is very low. 相似文献
12.
Origin and evolution of playas and blowouts in the semiarid zone of Tierra de Pinares (Duero Basin, Spain) 总被引：1，自引：0，他引：1
Mateo Gutirrez-Elorza Gloria Desir Francisco Gutirrez-Santolalla Cinta Marín 《Geomorphology》2005,72(1-4):177-192
A large number of blowouts and playas occur in the marginal sectors of the aeolian deposits located in the southern sector of the Duero Depression (Tierra de Pinares) in Spain. The blowouts are relict landforms that were developed on sand sheets by deflation during dry periods with lower vegetation cover and a deeper water table. The studied blowouts form complexes of NW–SE and NNW–SSE elongated hollows with accompanying dunes up to 4 km long in the leeward margins. Some hollows host lakes or swampy areas related to a shallow water table. The dunes formed by NE–ENE winds show steep windward slopes and gentle leeward slopes. The studied playas, with prevalent NNW–SSE orientations, result from the aeolian excavation of terrace deposits and the underlying marly bedrock. It is probable that the formation of these depressions in an initial stage was related to deflation processes affected preferentially NNW–SSE sandy channels perpendicular to the dominant wind direction. The precipitation of salts in the playas generates aggregates of clay particles (peloids) that are easily removed by the wind. Once the bottom reached the substratum, the deepening of the depressions progressed by the deflation of particles produced by weathering of the argillaceous bedrock. 相似文献
13.
Three experimental plots, covering the transition from the upper beach to the dune, on the North Sea coast of France were monitored at various intervals over a period of 18–24 months via high resolution terrain surveys in order to determine inter-site sand budget variability, as well as patterns and processes involved in sand exchanges between the upper beach and dune. The wind regime consists of a fairly balanced mix of moderate (80% of winds are below 8 m/s) onshore, offshore and shore-parallel winds. Sustained dune accretion over several years depends on the periodic local onshore welding of shoreface tidal banks that have developed in the storm- and tide-dominated setting of the southern North Sea. The only site where this has occurred in the recent past is Calais, where bank welding has created a wide accreting upper beach sand flat. At this site, significant sand supply from the subtidal sand bank reservoir to the upper beach flat occurred only once over the 18-month survey following a major storm. The bulk of the sand deposited over this large flat is not directly integrated into the adjacent embryo dunes by onshore winds but is progressively reworked in situ into developing dunes or transported alongshore by the balanced wind regime, thus resulting in alongshore stretching of the embryo dune system. The Leffrinckoucke site near Belgium shows moderate beach–dune mobility and accretion, while the Wissant site exhibits significant upper beach bedform mobility controlled by strong longshore currents that result in large beach budget fluctuations with little net budget change, to the detriment of the adjacent dunes. Accretion at these two sites, which are representative of the rest of the North Sea coast of France, is presently constrained by the absence of a shore-attached sand bank supply reservoir, while upper beach–dune sand exchanges are further limited by the narrow wave-affected upper beach, the intertidal morphology of bars and troughs which segments the aeolian fetch, and the moderate wind energy conditions. The balanced wind regime limits net sand mobilisation in favour of either the beach or the dune, and may explain the relatively narrow longshore morphology of the dune ridges bounding this coast. 相似文献
14.
戈壁砾石覆盖度与风蚀强度关系实验研究 总被引：3，自引：1，他引：2
戈壁表面的砾石覆盖度对风沙物质的运移有不可忽略的影响,在极端干旱区砾石覆盖是防沙治沙的重要手段。通过风洞实验模拟了阿拉善戈壁区砾石覆盖度与风蚀强度的关系。结果表明,当因地表风化作用等产生的松散颗粒物被吹蚀后,不同地点、不同样品之间风蚀强度有明显的差异,因而砾石覆盖度与风蚀强度之间的相关关系并不显著;但数据标准化后则表明,当砾石覆盖度在40%以下时,随砾石覆盖度的增加风蚀强度也有所增大。戈壁地区的风沙运动中,在砾石覆盖度小于40%条件下,不同风速下风蚀强度的变异系数是不同砾石覆盖度下的风蚀强度的变异系数的2倍左右。在极端干旱的戈壁区,影响风蚀强度的因素十分复杂,砾石覆盖度增大不仅不能控制风蚀现象的发生,反而增强气流对地表的风蚀能力,这一因素可能是阿拉善高原戈壁区成为中亚强沙尘暴主要源地的重要原因之一。 相似文献
15.
沙漠地区春季近地层气象要素分布规律的观测研究 总被引：7，自引：2，他引：5
利用2005年1月至2006年4月朱日和地区20 m气象塔的风向、风速、气温、相对湿度的观测资料,分析沙漠地区春季近地层气象要素的分布规律。结果表明: 春季温度回升,风速最大,相对湿度最小,利于起沙,故沙尘天气频繁。风速满足幂指数率分布规律,并且幂指数m能够很好的反映出风速梯度的变化情况;在沙尘暴、扬沙、背景、浮尘的天气条件下,春季近地面层风速梯度依次增大,湍流动量、热量交换系数依次减小;风向以西南为主。浮尘、扬沙天气各气层平均增温率分别大于或小于同时段的背景大气;沙尘暴期间温度下降,平均降温率为0.61 ℃\5h-1。春季相对湿度的平均递减率(递增率)与平均增温率(降温率)的大小正相关。浮尘天气相对湿度的平均递减率大于同时段的背景大气;扬沙天气相对湿度的平均递减率小于同时段的背景大气;沙尘暴天气相对湿度增大,平均增大率为2.80%\5h-1。 相似文献
16.
Aeolian processes are probably the dominant ongoing surface process on Mars; Large Dark Dunes (LDDs), particularly common aeolian landforms, were first recognized in the early 1970s. Recent, higher resolution images have revealed another, morphologically distinct, large population of smaller, ripple-like aeolian bedforms that have been termed “Transverse Aeolian Ridges” (TARs) as it is unknown whether they formed as large ripples or small dunes. We have begun a new study of TARs that examines their distribution, orientation, and morphology using > 10,000 high-resolution Mars Orbiter Camera (1.5 to 8 m/pixel resolution) images in a 45° longitude wide, pole-to-pole survey. The aim of this study is to assess whether TARs are active, to identify possible sediment sources and pathways, and to determine the volumes of sediment that they comprise. We present results from the first half of this study, in which we examine the northern hemisphere, and describe a new three-part classification scheme used to aid the survey.Our results show that TARs are abundant but not ubiquitous: preferentially forming proximal to friable, layered terrains such as those found in Terra Meridiani — the location of the ongoing Mars Exploration Rover “Opportunity” mission. TAR distribution in the northern hemisphere shows a strong latitudinal dependence with very few TARs being found north of 30° N. We also find that in most cases TARs are less mobile than LDDs, a conclusion possibly explained by Mars Exploration Rover Opportunity observations that show TAR-like ripples to have a core of fine material armored by a monolayer of granule-sized particles. This could disallow significant bedform movement under the current wind regime. That TARs are essentially inactive is confirmed by superposition relations with slope streaks and LDDs and by observations of superposed impact craters. We suggest that observations made by the Opportunity Rover in Terra Meridiani indicate that the small aeolian bedforms common here are ripples and not small dunes. Farther south, these bedforms transition into larger features indistinguishable from TARs, suggesting that TARs (in the Meridiani area at least) are ripples and not dunes. 相似文献
17.
新月形沙丘与线性沙丘共存区域风况特征 总被引：2，自引：2，他引：0
与火星类似,柴达木盆地的新月形沙丘和线性沙丘共存现象引起了众多学者的关注。为探究该现象的发育环境和形成条件,以全球典型新月形沙丘和线性沙丘共存区域为研究对象,选取研究区域附近气象站点3a风速、风向数据,分析这些典型区的风况特征。结果表明:不同的新月形沙丘与线性沙丘共存区域,风速存在明显差异,柴达木盆地和塔克拉玛干沙漠共存区域年平均风速和最大风速均小于沙特阿拉伯沙漠和撒哈拉沙漠;起沙风风向控制沙丘走向,多数共存区域全年起沙风风向较单一,部分区域存在明显的主次风,且主次风风向夹角为锐角;新月形沙丘和线性沙丘可共存于在高、中、低风能环境,中、低风向变率锐双峰或宽单峰风况,沙丘发育受风能环境影响较小,可能受风向变率、下垫面和沙源供应影响大;合成输沙势方向与沙丘走向一致且季节变化小,输沙方向稳定。部分气象站点距离研究区较远,对于研究区的风况指示意义有限。 相似文献
18.
Based on the sand dust storms data and climatic data in 12 meteorological stations around sand dust storm originating areas of the Taklimakan Desert, we analyzed the trends of the number of dust storm days from 1960 to 2005 as well as their correlations with temperature, precipitation, wind speed and the number of days with mean wind speed ≥ 5 m/s. The results show that the frequency of dust storm events in the Taklimakan region decreased with the elapse of time. Except Ruoqiang and Minfeng, in the other 10 meteorological stations, the frequency of dust storm events reduces, and in 4 meteorological stations of Kuqa, Korla, Kalpin and Hotan, the frequency of dust storm events distinctly decreases. The temperature has an increasing trend, while the average wind speed and the number of days with mean wind speed ≥ 5 m/s have decreasing trends. The correlation analysis between the number of days of dust storms and climatic parameters demonstrates that wind speed and the number of days with mean wind speed ≥ 5 m/s have strong positive correlation with the number of days of dust storms, with the correlations coefficients being 0.743 and 0.720 (p<0.01), respectively, which indicates that strong wind is the direct factor resulting in sand dust storms. Whereas precipitation has significant negative correlation with the number of days of dust storms (p<0.01), and the prior annual precipitation has also negative correlation, which indicates that the prior precipitation restrains the occurrence of sand dust storms, but this restraining action is weaker than the same year’s precipitation. Temperature has negative correlation with the number of dust storm days, with a correlations coefficient of –0.433 (p<0.01), which means that temperature change also has impacts on the occurrence of dust storm events in the Taklimakan region. 相似文献
19.
对策勒2011年1—12月4个不同下垫面的风速、温度、湿度、光合有效辐射的月差异进行分析,同时选取夏季晴天天气作为背景,比较沙尘暴、扬沙、浮尘、阴雨天时4个下垫面气象要素的差异。结果标明:与流沙地相比,绿洲-沙漠过渡带半固定沙地、固定沙地、绿洲内部2.0 m高处的6月平均风速依次减少了25.22%、27.93%、65.27%,12月绿洲内部0.5 m高处平均气温分别高于流沙地、半固定沙地、固定沙地1.39 ℃、1.21 ℃、2.70 ℃。5—10月4个下垫面之间温、湿度差异较春、冬季显著,7月流沙前沿2.0 m高处平均气温分别比半固定沙地、固定沙地、绿洲内部高0.35 ℃、1.61 ℃、3.75 ℃。沙尘暴天气下4个下垫面之间的风速差值依次小于扬沙、浮尘、阴雨、晴天天气下;在浮尘和晴天天气下,气温从流沙前沿到绿洲内部逐渐减低,相对湿度逐渐增加;沙尘暴和阴雨天气下各下垫面的气温和相对湿度无明显差异,扬沙天气下各下垫面之间温、湿度差异大于阴天天气,但小于浮尘和晴天天气;4个下垫面之间的光合有效辐射（PAR）在沙尘暴天气下差异最为明显,浮尘和阴雨天气下4个下垫面之间的PAR接近,晴天天气下各点PAR明显大于扬沙天气下,且各下垫面之间差异大于扬沙天气下的差异。 相似文献
20.
Ambient air particulate matter concentrations were measured at three locations in semi-arid SE Spain during 2005-2007. Sites representative of urban and rural background levels, as well as one representative of a rural area influenced by local mineral industry, were selected.The contribution of coarse particle resuspension (mainly crustal) in the area was assessed by studying the influence of wind speed, human activity and African dust outbreaks on the daily mass concentration and the aerosol number size distribution. Wind and soil characteristics in the area, typical of many semi-arid environments, are not conducive to major dust entrainment events.Twenty-four hour PM10 mass concentrations, subjected to air quality regulation, present a net decrease as wind speeds increase at the three study sites. Size-resolved measurements in the diameter range 0.25-32 μm with higher temporal resolution, however, show a net increase in the coarse particle concentrations with increasing wind speed, while the smallest particles are diluted. Although suspension is found to occur at all wind speeds, threshold values for an increase in particulate concentration can be identified and show some dependence on the particle size.African dust outbreaks, human activity and wind speed are (in this order) the main contributors for increasing particle sizes. 相似文献