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991.
992.
针对地下水埋深较浅地区,由高层建筑荷载引起的土体变形问题,以比奥固结理论为基础,结合土体非线性流变理论,将土体本构关系推广到黏弹塑性;同时考虑土体力学参数及水力参数的动态变化关系,建立了高层建筑荷载引发地面沉降与隆起变形的三维有限元数值模型,详细研究了高层建筑荷载影响下的土体变形特征及此过程中土体力学参数及水力学参数的变化特征。结果表明:由高层建筑荷载引起的地面沉降呈现漏斗状,以建筑物中心为漏斗中心,高层建筑荷载施加初期,高层建筑周围出现隆起,到达最大值后隆起逐渐消失;高层建筑底部浅层土体孔隙度、渗透系数及泊松比均呈现缓慢减小趋势,弹性模量呈现缓慢增大趋势;而高层建筑周围浅层土体的孔隙度、渗透系数及泊松比呈现先增大后减小的变化趋势,弹性模量则呈现先减小后增大的变化趋势;高层建筑影响区域浅部土体参数的变化趋势与土体的回弹及压缩有关。  相似文献   
993.
基于自动站观测资料的深圳城市热岛研究   总被引:7,自引:2,他引:5  
利用103个自动站气温观测资料,对深圳的城市热岛现象进行了研究.分析表明:1)高速的城市化进程造成自动站周边下垫面属性的变化,对气温造成了显著影响,这种影响即使是在仅仅10年内也表现得较为明显.2)由于深圳地处海滨,深圳的近地层气温分布是海陆作用叠加城市热岛效应形成的结果.按照传统定义的深圳城市热岛,其空间分布在不同季...  相似文献   
994.
The present study combined remote sensing with geographical information system (GIS) technology to interpret Landsat TM images from 1996 to 2000 and establish a land cover database for the Hexi Corridor of China’s Gansu Province. The areas of sand and dust emission and trends in their change were extracted by analyzing the database, with the following results: In 2000, the source area for sand and dust storms totaled nearly 170,000 km2, accounting for 75.1% of the study region. The emission area decreases from as much as 70,000 km2 in winter and spring to around 58,000 km2 in summer and autumn, accounting for 41.1 and 34.1% of the source area, respectively. During the 4 years of the study period, the emission area decreased by nearly 57 km2 in winter and spring (a 0.1% change); however, the vulnerability of the land surface to wind erosion increased in ca. 190 km2 and decreased in ca. 102 km2. Although the area of dust emission decreased from 1996 to 2000, the area vulnerable to wind erosion increased by ca. 87 km2, and the increased number of sand and dust storm days in the region between 2000 and 2003 appears to be correlated with this increase.  相似文献   
995.
The study investigates the groundwater evolution and its residence time in the Ejina Basin, northwest China according to isotope and hydrochemical analyses results. The groundwater chemistry is mainly controlled by the dissolution of halite, Glauber’s salt, gypsum, dolomite and calcite, also influenced by other processes such as evaporation, ion exchange, and deposition. Based on tritium content in atmospheric precipitation and by adopting a model with exponential time distribution function, the mean residence time of the unconfined aquifer groundwater with fairly high tritium activities (21–49 TU) is evaluated. The results show that these groundwaters have low residence time (5–120 years) and are renewable. In contrast, the deep confined groundwaters are tritium-free and radiocarbon values range from 18.3 to 26.7 pmc. According to the most commonly used 14C correction models, the radiocarbon groundwater ages were calculated which yield ages of approximately 4,087–9,364 years BP. Isotopic signatures indicate formation of deep confined groundwaters in a colder and wetter climate during the late Pleistocene and Holocene. It is suggested that long-term, rational water usage guide should be set up for the Heihe River Basin as a whole to permit a considerable discharge to the Ejina Basin.  相似文献   
996.
谭明 《第四纪研究》2009,29(5):851-862
根据最近的研究结果,中国季风区同一洞穴或同一区域的晚全新世石笋氧同位素序列具有较好的重复性,表明中国季风区的石笋氧同位素短尺度(10~100年尺度,后同)变率所具有的信号强于噪音。通过进一步比较分析发现,一些石笋氧同位素记录虽然来自距离上千公里之遥的不同区域,但它们的波动形式在年代际至世纪尺度极其相似,说明它们是一致的大区域信号,但多数石笋氧同位素序列未能校准到本区器测的降水或温度记录上。通过与中国气候学家建立的各类季风指数比较,发现这些具有一致大区信号的中国石笋氧同位素序列与海平面气压差指数或海陆温差指数关系最好。再通过与印度洋-太平洋海域海平面气压差、以及许多海、气环流观测记录对比,发现中国季风区石笋氧同位素序列记录了20世纪后期最强的一次全球海、气环流年代际均值突变,由此初步确认了中国季风区石笋氧同位素短尺度变化的环流意义: 当印度洋海水和中东太平洋海水温度偏低时,西太平洋副热带高压偏北东缩而弱,中国季风区内来自印度洋的水汽份额增大,由于这些水汽的输送路程很远,导致中国季风区的雨水氧同位素及石笋氧同位素较轻; 而当印度洋海水和中东太平洋海水温度偏高时,西太平洋副热带高压偏南西伸而强,中国季风区内来自印度洋的远源水汽份额减少,而来自西太平洋的水汽份额增大,由于后者输送路程较近,导致中国季风区的雨水氧同位素及石笋氧同位素较重。由此命名瑞利分馏原理所决定、反映印度洋/太平洋海、气环流转变且大区域一致的中国季风区石笋氧同位素10~100年尺度变化为“环流效应”。  相似文献   
997.
Laboratory experiments on longitudinal dispersion in clear-water and sediment-laden open channel flows are reported. Data from these experiments and those available from previous studies indicate that the suspended sediment present in the flow affects the longitudinal dispersion process. The observed velocity distributions over the depth of sediment-laden flows indicate that the velocity deviates from the mean velocity more in sediment-laden flows than in clear-water flows. The velocity distributions over the cross section and secondary flow in the channel are also expected to be altereddue to the presence of suspended sediments in the flow. For these reasons, more dispersion is found in sediment-laden flows than in corresponding clear-water flows. A predictor for the dispersion coefficient in sediment-laden flows is proposed.  相似文献   
998.
Monitoring of the active galaxy nucleus 3C 66A in the VHE γ-ray and analysis of data in X-rays and optical ranges over the period 1996–2009 were carried out. The nature of processes responsible for one or another type of radiation appeared to be very complicated since, at certain periods of time, an either positive or negative correlation may be observed between different types of radiation. Period of radiation P = 365 days in the X-ray range was found.  相似文献   
999.
SWAN, the all-sky hydrogen Lyman-alpha camera on the SOHO spacecraft, designed primarily to image the interplanetary neutral hydrogen around the Sun, also observes comets continuously over large portions of their apparitions to the north and south of the ecliptic and at small solar elongation angles. Because of SOHO’s location at the L1 Lagrange point, analysis of SWAN images provides excellent temporal coverage of water production. We report here our results of observations of some interesting target comets selected from the extensive SWAN archive. These include three Oort Cloud Comets C/2002 V1 (NEAT), C/2002 X5 (Kudo–Fujikawa), C/2006 P1 (McNaught) and three apparitions of atypical short-period Comet 96P/Machholz 1. The common aspect of these four comets is their small perihelion distances, which are 0.19, 0.09, 0.17, and 0.12 AU, respectively. Their water production rates over their whole apparitions can be approximated by power laws in heliocentric distance (r in AU) as follows: 1.3 × 1029 r−2.1 s−1 for C/2002 V1 (NEAT), 7.5 × 1028 r−2.0 s−1 for C/2002 X5 (Kudo–Fujikawa), 5.4 × 1029 r−2.4 s−1 for C/2006 (P1 McNaught) and 4.6 × 1027 r−2.1 s−1 for 96P/Machholz 1. We also present daily-average water production rates for the long-period comets over long continuous time periods. We examine these results in light of our growing survey of comets that is yielding some interesting comparisons of water production rate variations with heliocentric distance and taxonomic classes.  相似文献   
1000.
In this paper, we introduce a simplified model for explaining the observations of optical intra-day variability (IDV) of the BL Lac Objects. We assume that the source of the IDV are the stochastic oscillations of an accretion disk around a supermassive black hole. The stochastic fluctuations on the vertical direction of the accretion disk are described by using a Langevin type equation with a damping term and a random, white noise type force. Furthermore, preliminary numerical simulation results are presented, which are based on the numerical analysis of the Langevin stochastic differential equation.  相似文献   
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