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71.
初析静力触探判别液化对标准贯入试验的优越性 总被引:1,自引:0,他引:1
结合7个勘察场地的标准贯入和静力触探原位测试数据,应用数理统计原理和方法对二者进行比较分析,得出用静力触探试验判别地基土液化的均方差和变异系数等均优越于标准贯入试验。 相似文献
72.
73.
The Zoulang Nanshan Caledonian Subduct ion Complex in the Northern Qilian Mountains and Its Dynamics 总被引:1,自引:0,他引:1
Xu Zhiqin Xu Huifen Zhang Jianxin Li Haibing Zhu Zhizhi Qu Jingchuan Institute of Geology Chinese Academy of Geological Sciences BeijingChen Daizhang Chen Jinlu China University of Geosciences Beijingand Yang KaichunNo. Q ilian Geological Party Bureau of Geology Mineral Resources of Q inghai Province Q ilian County Q inghai 《《地质学报》英文版》1994,68(3)
The front of the Zoulang Nanshan Caledonian volcanic island arc zone in the northern Qilian Mountains is a forearc accretionary terrane, composed of multiple accretionary volcanic island arcs, flysch accretionary wedges,high-pressure metamorphosed detachment zones and remnants of ophiolites. It resulted from the northeastward subduction of the Early Palaeozoic Qilan oceanic crust beneath the Alxa block. High-pressure metamorphism, which occurred during the subduction, progressed through three stages: the initial stage of medium T-high P,the main stage of temperature decrease and pressure increase, and the lag stage of pressure decrease and temperature increase. Finally the paper presents a retrotrench subduction dynamic model indicative of northward subduction of the central Qilian block and southward accretion of the Alxa block during the period of 450-500 Ma. 相似文献
74.
朱杏芬 《中国天文和天体物理学报》1986,(1)
以Savage-Bolton的两个5°×5°天区的光学类星体巡天为样品,本文系统地分析了成线排列的类星体数目,并与由Monte Carlo方法产生的随机样品进行了比较。统计结果表明,类星体成线排列现象至少在这组样品中不明显。 相似文献
75.
P. Pravec P. Scheirich L. Šarounová G. Hahn G. Esquerdo Z. Krzeminski B.D. Warner M.C. Nolan L.A.M. Benner A. Galád W. Holliday Yu.N. Krugly R. Whiteley D.R. DeGraff S. Larson W.R. Cooney Jr. J. Zhu R. Dyvig V. Reddy Š. Gajdoš G. Masi D. Higgins B. Knight R. Behrend G. Burki C. Demeautis N. Waelchli A. Klotz M. Rieugné V. Cotrez G. Kober 《Icarus》2006,181(1):63-93
Photometric data on 17 binary near-Earth asteroids (15 of them are certain detections, two are probables) were analysed and characteristic properties of the near-Earth asteroid (NEA) binary population were inferred. We have found that binary systems with a secondary-to-primary mean diameter ratio Ds/Dp?0.18 concentrate among NEAs smaller than 2 km in diameter; the abundance of such binaries decreases significantly among larger NEAs. Secondaries show an upper size limit of Ds=0.5-1 km. Systems with Ds/Dp?0.5 are abundant but larger satellites are significantly less common. Primaries have spheroidal shapes and they rotate rapidly, with periods concentrating between 2.2 to 2.8 h and with a tail of the distribution up to ∼4 h. The fast rotators are close to the critical spin for rubble piles with bulk densities about 2 g/cm3. Orbital periods show an apparent cut-off at Porb∼11 h; closer systems with shorter orbital periods have not been discovered, which is consistent with the Roche limit for strengthless bodies. Secondaries are more elongated on average than primaries. Most, but not all, of their rotations appear to be synchronized with the orbital motion; nonsynchronous secondary rotations may occur especially among wider systems with Porb>20 h. The specific total angular momentum of most of the binary systems is similar to within ±20% and close to the angular momentum of a sphere with the same total mass and density, rotating at the disruption limit; this suggests that the binaries were created by mechanism(s) related to rotation near the critical limit and that they neither gained nor lost significant amounts of angular momentum during or since formation. A comparison with six small asynchronous binaries detected in the main belt of asteroids suggests that the population extends beyond the region of terrestrial planets, but with characteristics shifted to larger sizes and longer periods. The estimated mean proportion of binaries with Ds/Dp?0.18 among NEAs larger than 0.3 km is 15±4%. Among fastest rotating NEAs larger than 0.3 km with periods between 2.2 and 2.8 h, the mean proportion of such binaries is (66+10−12)%. 相似文献
76.
浙江近海夜光藻的分布及其生态学特点 总被引:4,自引:1,他引:4
本文利用历次夜光藻调查资料,阐述了其在浙江近岸海域的分布特点,丰度高峰主要出现在春秋季,夏季亦存在暴发性增殖的可能性,冬季则基本见不到夜光藻的踪迹。杭州湾口等水体浑浊区是夜光藻的低丰度区,仅在春夏季有零星出现,这与水体透明度低、悬浮泥沙含量高及强烈的水动力因子等密切相关。在时间尺度上,夜光藻丰度呈上升趋势,根本原因是海域富营养化加剧的结果。 相似文献
77.
深潜器的使命和一般的潜水艇不同,它在操纵性方面的特点与战斗潜艇相比有很大的差异,操纵要求和操纵手段均有不同.它不仅要求和普通潜艇一样在水平面和垂直面内有良好的操纵性,而且由于水下作业和潜艇救生等的需要,还要求艇能在水中完成停悬、横向平移、原地回转、纵摇、滚转以及水下对接等特殊的操作. 相似文献
78.
对类比路段进行连续模拟试验,进行现场调查,给出汽车尾气主要污染物的排污强度,预测了汽车尾气中CO、C_nH_m和NO_x的扩散范围。 相似文献
79.
海洋颗粒有机碳(POC)是海洋固碳的一个关键参数。为了研究南海北部陆架及海盆表层POC浓度的时空分布特征以及变化趋势,本文利用2009-2011年4个季节的实测数据,对NASA发布的MODIS/AQUA卫星月平均POC遥感产品,进行了验证和校正;并利用校正后的遥感数据分析了2003-2014年POC的时空分布特征和变化趋势。发现POC遥感产品与南海北部实测数据具有较好的线性关系(R2=0.72),但存在系统性偏高,需利用实测数据对遥感数据进行区域性校正。分析校正后的遥感数据发现,南海北部陆架POC浓度较高,平均为(33.34±8.02)mg/m3;吕宋海峡西南海域浓度较低,平均为(29.25±6.20)mg/m3;中央海盆区浓度最低,平均为(27.02±4.84)mg/m3。春夏季POC浓度较低,最低值一般出现在5月,冬季(12月至翌年1月)POC浓度达到最高。利用2003-2014年的长时间序列遥感叶绿素(Chl a)和海表温度(SST)、混合层深度(MLD)模式数据,以及实测数据对南海北部POC浓度的影响机制进行了分析。发现POC与Chl a在秋冬呈现较好的相关关系(R2=0.51),但在春夏季较离散,表明秋冬季生物作用对POC影响较大。2003-2014年期间,POC与Chl a、MLD及SST存在明显的年际变化,但并没有显著的上升或下降趋势。 相似文献
80.
A numerical modeling study of the influence of the lateral flow on the estuarine exchange flow was conducted in the north passage of the Changjiang estuary. The lateral flows show substantial variabilities within a flood-ebb tidal cycle. The strong lateral flow occurring during flood tide is caused primarily by the unique cross-shoal flow that induces a strong northward (looking upstream) barotropic force near the surface and advects saltier water toward the northern part of the channel, resulting in a southward baroclinic force caused by the lateral density gradient. Thus, a two-layer structure of lateral flows is produced during the flood tide. The lateral flows are vigorous near the flood slack and the magnitude can exceed that of the along-channel tidal flow during that period. The strong vertical shear of the lateral flows and the salinity gradient in lateral direction generate lateral tidal straining, which are out of phase with the along-channel tidal straining. Consequently, stratification is enhanced at the early stage of the ebb tide. In contrast, strong along-channel straining is apparent during the late ebb tide. The vertical mixing disrupts the vertical density gradient, thus suppressing stratification. The impact of lateral straining on stratification during spring tide is more pronounced than that of along-channel straining during late flood and early ebb tides. The momentum balance along the estuary suggests that lateral flow can augment the residual exchange flow. The advection of lateral flows brings low-energy water from the shoal to the deep channel during the flood tide, whereas the energetic water is moved to the shoal via lateral advection during the ebb tide. The impact of lateral flow on estuarine circulation of this multiple-channel estuary is different from single-channel estuary. A model simulation by blocking the cross-shoal flow shows that the magnitudes of lateral flows and tidal straining are reduced. Moreover, the reduced lateral tidal straining results in a decrease in vertical stratification from the late flood to early ebb tides during the spring tide. By contrast, the along-channel tidal straining becomes dominant. The model results illustrate the important dynamic linkage between lateral flows and estuarine dynamics in the Changjiang estuary. 相似文献