On the relation of moderate-short term anomaly of earth resistivity to earthquake   总被引：1，自引：0，他引：1  

杜学彬  薛顺章  郝臻  张世中 《地震学报(英文版)》2000,13(4):393-403

IntroductionMany anomalies due to earthquake have been recorded in observation of earth-resistivity for30 years and over, which showed that there objectively existed the anomalies of each-resistivity.The crustal strUcture and medium conditions are quite complex, so the complexity of the temporal,spatial and intensive development of the anomalies is inevitable. Both of time and amplitUde ofanomalies among some stations near an epicenter are different (even among different observational directi…  相似文献   

混合含水介质压密作用下渗透系数的变化规律研究     

秦皓  牛萌萌  姚玉川  刘洋  谭静 《地下水》2018,(6):5-7

渗透系数是重要的水文地质参数,不同含水介质在不同条件下的渗透性不同。通过对中砂、细砂及其分别按1:1、2:1比例均匀混合的四种砂样进行压密实验,然后根据达西定律计算其在不同压密条件下的渗透系数,分析不同砂样的渗透系数呈现的线性关系,得出含水介质在不同压密作用下渗透系数的变化规律。结果表明,渗透系数随模拟含水介质压密的增大呈线性减小趋势,线性拟合决定系数为0.845 2～0.885 5;在单一砂样长时间实验下,由于重力影响所产生的细小颗粒运移,各砂样所测得的渗透系数均为前期快速下降,后期下降速度趋缓;含水介质透水能力主要取决于粒间空隙大小和多少等因素;混合砂中,随着粒径较小介质的比例增加,渗透系数在不同程度上更倾向于粒径较小的含水介质。  相似文献   

吐哈盆地台北凹陷柯柯亚构造中深层储层特征及成因          下载免费PDF全文

陈彬  钟建华  曲俊利  魏婷  徐杰 《沉积与特提斯地质》2015,35(3):27-34

通过薄片的镜下观察、扫描电镜、能谱分析和物性分析等手段的应用,对吐哈盆地北部斜坡柯柯亚构造中深层储层特征和成因进行了研究。结果表明,柯柯亚构造八道湾组储层几乎全部为碎屑岩,储层主要岩石类型为灰色、深灰色或灰黑色的中厚层状泥质粉砂岩、中-粗砂岩、含砾粗砂岩,普遍含大量碳屑。孔隙类型主要为粒内溶蚀孔和粒间剩余孔。成岩作用主要有压实作用、胶结作用和溶蚀作用。孔渗条件差,为特低孔特低渗类储层。沉积作用是特低孔特低渗储层发育的基础,成岩作用是中深层储层致密化的关键,粒度是储集性能的主控因素。  相似文献   

Wind tunnel experimental study on shed tunnels to prevent and control blowing snow on highways北大核心CSCD     

马磊  刘健  冉武平  胡智轩  李在蓝  俞祥祥 《冰川冻土》2022,44(2):726-734

There is a severe phenomenon of blowing snow by wind in winter in Mayitas area of Xinjiang. Road traffic interruptions and casualties caused by wind and snow disasters often occur. The existing engineering measures can alleviate the problems of low visibility and problems with accumulating snow on pavement caused by wind and snow to a certain extent, but cannot completely eliminate the impact. Aiming at the problem that the blowing snow disaster difficult to be completely cured under strong wind conditions, a shed tunnel engineering treatment scheme is proposed, and a wind tunnel simulation experiment is carried out on the shed tunnel form and snow prevention scheme at the entrance of the tunnel. The wind tunnel experimental section is 8 m long, 1. 3 m horizontally wide and 1 m high. The shed tunnel model is made by 1:60 scale 3D printing method, the snow barrier model is made of wooden strips, and the simulation medium is made of fine sand, refined salt and sawdust. Firstly, three kinds of shed structures, including fully enclosed, overhanging and ventilated, were simulated under the condition of 90° wind direction, and compared with the form of blowing snow stacking. Three parameters for similarity were used:density, particle size and stacking shape. The similarity is determined by weighted Euclidean distance between simulation medium and blowing snow, the similarity of the slump angle of the predecessors is verified, and the most suitable medium for simulating blowing snow is deduced. According to the experimental results, combined with the actual situation of wind blowing and snow disasters in Mayitas, flow field of the closed shed tunnel by a wind direction angle of 30° has been separately conducted with or without protective measures. The results show that when the wind tunnel stacking experiment is used to study the deposition state of blowing snow under non-low temperature conditions, the sawdust has good similarity with the blowing snow in the process of wind and snow movement. A large amount of medium was poured into the ventilated shed during the experiment, which proved that its anti-wind and snow performance was not ideal. By contrast, the closed shed and the overhanging shed have better wind and snow prevention effects. The snow barrier has a good blowing snow inhibition function at the entrance. From the stacking experiment, in the comparison with and without snow barrier, volume of the medium in the shed is very different, which proves that the snow barrier can effectively prevent the blowing snow from entering the shed. Among them, the difference in wind speed inside and outside the shed is obvious, which proves that snow barrier can significantly reduce the wind speed outside the shed and has the function of inhibiting the formation of weak wind areas inside the shed. The study has confirmed that the shed tunnel project with suitable snow barrier layout plan for tunnel entrance protection is an effective means to control wind and snow disasters. For highway traffic in Xinjiang, it is a feasible solution to use shed tunnel engineering to control blowing snow disasters. After dealing with the snow deposition at the entrance of shed tunnel, the shed tunnel engineering form of low-cost environment integration and the vehicle operation safety guarantee measures of long-distance shed tunnel are the problems that need to be solved in the future. © 2022 Tianjin Press of Chinese Herbal Medicines. All rights reserved.  相似文献   

浅埋管道水平横向作用下砂土极限承载力研究     

钟紫蓝  韩春堂  李锦强  赵鑫  缪惠全 《岩土力学》2022,43(Z2):95-103

断层、滑坡、液化等地质灾害引起的场地大变形对埋地管道结构安全产生严重的威胁。开展了中密砂中埋地管道−砂土水平横向相互作用的系列三维数值模拟,根据数值模拟的结果探讨了不同深径比下管−砂土横向相互作用时土体的破坏模式,研究了深径比对砂土极限承载力的影响。基于管周土体的破坏模式建立了简化计算模型,根据极限平衡理论推导了管道水平横向运动时砂土极限承载力计算公式。研究结果表明：极限状态下,浅埋管道周围土体形成延伸到地表的破裂面,轮廓线近似对数螺线;砂土的极限承载力随着深径比增加,最终在临界深径比处达到稳定;随着深径比的增加,土体发生剪切滑动破坏所需的管道位移也逐渐增大;由于横向承载力系数取值依据不同,国内外规范计算所得土体极限承载力差异较大;得到的解析解能够较好地预测中密砂土中浅埋管道水平横向运动时土体的极限承载力。  相似文献   

TerraSAR-X卫星影像中大比例尺测图应用研究     

刘美娟  谢金华  邱振戈  张春玲 《测绘科学》2015,(9):143-148

为了研究TerraSAR-X卫星的中大比例尺测图可行性,文章利用成都都江堰市3m、1m分辨率的TerraSAR-X影像、控制点及可见光卫星影像,对TerraSAR-X影像在多云多雨地区的中、大比例尺测图展开了研究和分析。实验表明利用TerraSAR-X影像能够符合中大比例尺基础地图测图或修测的精度要求,可用于困难地区1∶50 000~1∶10 000比例尺的基础测图生产和更新。  相似文献   

2015年6—8月T639、ECMWF及日本模式中期预报性能检验   总被引：1，自引：1，他引：0  

尹姗 《气象》2015,41(11):1417-1424

对2015年6—8月T639、ECMWF及日本（文中简称EC和JP）数值模式的中期预报产品进行了对比分析和检验,结果表明：三个模式对亚洲中高纬环流形势的调整和演变具有较好的预报性能,其中EC模式的预报效果最好。EC模式对西太平洋副热带高压的预报较为准确,T639模式的预报与实况存在一定偏差。三个模式均能较好地预报出2015年7月新疆持续性高温天气,且对北方地区850 hPa温度的预报较零场均偏高。在南方地区,三个模式预报的温度偏差比北方地区小,EC模式的预报效果优于T639和JP模式。对于1513号台风苏迪罗,T639模式较好地预报了台风的登陆位置和路径变化,强度预报略偏强,而EC模式预报的台风登陆时间偏早。  相似文献   

Interaction of the supernova remnant HB3 with the ambient interstellar gas     

I. V. Gosachinskii 《Astronomy Letters》2005,31(3):179-185

The well-known shell supernova remnant (SNR) HB3 is part of a feature-rich star-forming region together with the nebulae W3, W4, and W5. We study the HI structure around this SNR using five RATAN-600 drift curves obtained at a wavelength of 21 cm with an angular resolution of 2′ in one coordinate over the radial-velocity range ?183 to +60 km s^?1 in a wider region of the sky and with a higher sensitivity than in previous works by other authors. The spatial-kinematic distribution of HI features around the SNR clearly shows two concentric expanding shells of gas that surround the SNR and coincide with it in all three coordinates (α, δ, and V). The outer shell has a radius of 133 pc, a thickness of 24 pc, and an expansion velocity of 48 km s^?1. The mass of the gas in it is ≈2.3 × 10⁵M_⊙. For the inner shell, these parameters are 78 pc, 36 pc, 24 km s^{? 1}, and 0.9 × 10⁵M_⊙, respectively. The inner shell is immediately adjacent to the SNR. Assuming that the outer shell was produced by the stellar wind and the inner shell arose from the shock wave of the SNR proper, we estimated the age of the outer shell, ≈1.7 × 10⁶ yr, and the mechanical luminosity of the stellar wind, 1.5 × 10³⁸ erg s^?1. The inner shell has an age of ≈10⁶ yr and corresponds to a total supernova explosion energy of ≈10⁵² erg.  相似文献   

亚甲基蓝对南美白对虾(Pemaeus vannamei Boon)幼体的毒性研究   总被引：6，自引：0，他引：6  

刘建勇  彭树锋 《海洋湖沼通报》2005,(1):49-53

研究了亚甲基蓝对南美白对虾蚤状幼体、糠虾幼体及仔虾的急性毒性。结果表明,不同发育期的幼体,仔虾对此种消毒剂的耐受力不同。亚甲基蓝对南美白对虾蚤状幼体(Z)的24hLC50、48hLC50和安全浓度分别为:2.88×10-6,0.89×10-6,0.025×10-6;对糠虾幼体(M)的24hLC50、48hLC50和安全浓度分别为:3.39×10-6,1.04×10-6,0.029×10-6;对仔虾(P)的24hLC50、48hLC50和安全浓度分别为:6.76×10-6,2.24×10-6,0.073×10-6。  相似文献   

从南海与大洋磁异常的相关性探讨南海的成因   总被引：1，自引：0，他引：1  

霍明远  吴廷芳  杨华 《热带海洋学报》1995,(1)

对南海与大洋盆地条带状磁异常的相关分析表明，相关系数为０．１１—０．６５９，存在弱线性关系。这从一个侧面反映出边缘海洋壳与大洋壳本质上的差异。边缘海洋壳是玄武岩浆侵入并吞蚀破碎的大陆边缘地壳后形成的不同于大洋壳的新型洋壳。南海盆地磁异常显示其洋壳是新老不一、厚薄不匀的新洋壳的拼合叠覆体。  相似文献