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891.
Characteristics of particle size for creeping and saltating sand grains in aeolian transport 下载免费PDF全文
Hong Cheng Jiajia He Xueyong Zou Jifeng Li Chenchen Liu Bo Liu Chunlai Zhang Yongqiu Wu Liqiang Kang 《Sedimentology》2015,62(5):1497-1511
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
892.
893.
藏北青南高原长期受风蚀影响,地表粗化现象明显。本研究系统采集该区东西向调查样带内表层(0~1 cm)与浅层(1~10 cm)土壤样品,通过粒度测定、构建能够表征土壤风蚀粗化程度的风蚀粗化指数(WECI),分析该区地表风蚀粗化特征。结果表明:藏北青南高原土壤中砾石、极粗砂、粗砂等粗颗粒组分在表层土壤中含量较浅层土壤有所增加,自西向东逐渐减少;黏土与粉砂等细颗粒组分相反,表层较浅层土壤中含量明显下降,自西向东逐渐增加。从样带东部的高寒草甸区到中部高寒草原区和西部高寒草原与荒漠草原过渡区,表层土壤环境敏感组分逐渐变粗,各区域平均风蚀粗化指数依次为1.05、1.47和1.77,地表风蚀粗化趋于加剧。现有文献常用的土壤粒度分形维数与土壤质地粗化度是刻画土壤质地粗细程度的静态指标,无法衡量风蚀导致的地表颗粒组成变化,本文构建的风蚀粗化指数克服了上述不足,且具有风蚀动力学依据。 相似文献
894.
风沙过渡区土地利用变化及生态效应图谱——以陕北榆阳区为例 总被引:7,自引:4,他引:3
以遥感影像资料为依据,运用地学信息图谱研究方法,在RS和GIS的支持下分析榆阳区1985~2000年土地利用及其生态服务价值的时空变化特征。结果表明:该区研究期内最主要的土地利用动态是未利用地向草地的转化,其变化占全区总变动量91.14%;土地利用变化使生态系统的生态服务价值增加了158.59×106元,增幅为8.23%,其中,风沙区占总增量的85.99%,增幅10.88%,黄土丘陵沟壑区占总增量14.01%,增幅3.29%。经过实证分析,利用地学信息图谱进行土地利用变化和生态效应定量研究是一种十分有效的方法。 相似文献
895.
本文首次利用完全相同两颗卫星(CLUSTER C1和C3)的数据对地球激波前兆区太阳风的减速和偏转特性进行了统计研究.结果表明,在激波前兆坐标系中,太阳风减小的速度随观测点到激波的距离DBS增大而减小,随行星际磁场与激波法向夹角θBN增大也减小,在ULF波动区深度DWS小于6Re(Re为地球半径)的范围内最为显著;伴随着太阳风减速的另外一个现象——太阳风的偏转,也存在相似的规律.其最大减速和最大偏转角度分别为10 km/s和3°.太阳风减速和偏转,以及随之变化的太阳风动压,可能会引起地球磁层顶位置和形状发生改变,同时也为激波前兆区弥散(diffuse)离子的起源及加热提供了一种可能的机制. 相似文献
896.
本文根据搭载于Cluster卫星的CIS/CODIF和RAPID仪器的观测数据,统计研究了等离子体片中的H+、O+离子在磁暴期间的时间变化特性,及其对太阳风条件的响应.观测结果表明:(1) 磁暴开始前,O+离子(0~40 keV)数密度保持在较低水平.随着磁暴的发展,O+数密度缓慢上升,其峰值出现在Dst极小值附近;H+离子(0~40 keV)数密度在磁暴开始之前的较短时间迅速增加并达到峰值,在磁暴开始之后迅速降低,并在整个主相和恢复相期间保持在相对较低水平.更高能量的离子则在磁暴开始后迅速增多,并在低能O+离子达到峰值之前达到峰值.因此我们推测磁暴初期从等离子体片注入环电流的主要是H+离子,主相后期O+离子可能扮演更为重要的角色.(2)在地磁活动时期,太阳风密度和动压强与等离子体片中的H+、O+数密度存在一定相关性.等离子体片中的H+离子对北向IMF Bz较为敏感,而IMF Bz南向条件下更有利于太阳风参数对等离子体片中O+数密度的影响.在地磁活动平静期,太阳风条件对等离子体片中的离子没有明显影响. 相似文献
897.
M. R. Phillips 《地球表面变化过程与地形》2008,33(13):2094-2107
In 1997–98, unique critical beach erosion led to structural failure along the Penarth, South Wales, UK coastline and anthropogenic activities, such as the construction of the Cardiff Bay Barrage and offshore marine aggregate dredging, were suggested as causes. The time‐frame of significant erosion was between 1995 and 1997 and forcing agents (extreme sea level and wind direction) and shoreline indicators (mean beach level and MHW) were analysed in order to assess change. Water level analysis showed that although there was no significant difference between actual and predicted mean sea levels, extreme sea levels at that time were significantly higher (t = 3·305; d.f. = 8; p < 0·05). Three wind direction analyses (annual mean, mean annual maximum gust and mean annual maximum gust ≥28 kn) between 1995 and 1997 also showed significant differences (p < 0·05). All comprised more easterly components which meant they approached the beach from the sea. Furthermore, gusts ≥28 kn from the northeast quadrant, that is, 0° to 90° true, were significantly more frequent during these years (t = 3·674; d.f. = 8; p < 0·01). Justification of statistical significances was established and there was supporting evidence of unusual meteorological conditions at that time. Relationships showed correlation between forcing agents (extreme sea level and wind direction) and shoreline indicators (mean beach level and Mean High Water). Furthermore, regression analysis showed winds from the northeast quadrant resulted in steeper longshore gradients, as a consequence of beach material loss. Therefore, it was concluded that the critical erosion of Penarth beach between 1995 and 1997 was caused by increased wave attack from the northeast and southeast quadrants, generated by unique significant changes in wind direction and extreme sea levels. Copyright © 2008 John Wiley & Sons, Ltd. 相似文献
898.
Jiang YuJun Liu HuiZhi Zhang BoYin Zhu FengRong Liang Bin Sang JianGuo 《中国科学D辑(英文版)》2008,51(1):103-113
Flow structure and wind pressure distribution caused by obtuse obstacles are usually the focuses in Computational Wind Engineer researches (CWE). By solving the non-hydrostatical dynamic equations, PUMA model (Peking University Model of Atmospheric Environment) was developed and applied to simulating the flow structure and wind pressure distribution around a tower-shaped building. Evaluation about the wind environment and wind loads around the building was obtained through the analysis of the numerical simulation results and wind tunnel data. Comparisons between the simulation and wind tunnel study indicate that numerical simulation results agree well in the flow field and wind pressure distribution around the tower-shaped building. On the other hand, the horizontal grid interval of 2 m and the vertical grid of 3 m were still too crude to simulate the flow structure and wind pressure distribution on the building surface more exactly in detail; and the absence of suitable pressure perturbation parameterization scheme between the solid and the adjacent space also limits the accuracy of the numerical simulation. The numerical simulation model can be used to evaluate the wind environment and wind load around high buildings. 相似文献
899.
In the surface wind drift layer with constant momentum flux, two sets of the consistent surface eleva- tion expressions with breaking and occurrence conditions for breaking are deduced from the first in- tegrals of the energy and vortex variations and the kinetic and mathematic breaking criterions, then the expression of the surface elevation with wave breaking is established by using the Heaviside function. On the basis of the form of the sea surface elevation with wave breaking and the understanding of small slope sea waves, a triple composite function of real sea waves is presented including the func- tions for the breaking, weak-nonlinear and basic waves. The expression of the triple composite func- tion and the normal distribution of basic waves are the expected theoretical model for surface elevation statistics. 相似文献
900.
岩爆破坏过程能量释放的数值模拟 总被引:1,自引:0,他引:1
岩爆是地下岩石开挖中的一种工程灾害现象,是岩体结构发生破坏时,由于内部储存的弹性能释放并转换为动能而造成动力形式的破坏。岩爆破坏过程中的能量释放与岩体在应力峰值前后的应力-应变特性紧密相关。另外,施工中开挖速度引起的加载速率的变化也会对岩爆的产生有明显影响。以岩体全过程应力-应变曲线试验为基础分析岩爆破坏过程。分析中采用的模型考虑了岩石峰值后应力-应变特性及加载速率的影响。运用数值方法对岩石洞室的开挖过程进行了模拟,在模拟中对岩体破坏的发生及弹性能释放过程进行了分析。数值分析结果显示,岩体洞室开挖过程中岩石破坏由岩体表面向岩体内部发展,岩石的弹性能释放率也随着破坏的发展而不断增加。分析结果还显示,岩体破坏时的弹性能释放速率会随着开挖速率的提高而明显增加。 相似文献