滇西北地区近年来应力场的数值模拟研究     

武永彩  李昂  唐红涛 《大地测量与地球动力学》2018,38(12):1238-1240

建立滇西北地区三维有限元地质模型，将2009~2016年GPS速度场数据作为数值模拟的位移边界条件，模拟获取该地区的构造应力场。结果表明，在楚雄至滇西北地区整体显示张性应力区；出现由“洱源鹤庆断裂-红河断裂-程海断裂”圈起的低值张性区，区域内部张性应力明显低于外部，这种张应力低值区尤其在区域四周断裂边界处，往往是地壳断裂活动的频发区；曲江断裂北端及元谋-绿汁江断裂南端出现张性应力集中区，是今后重点关注的断裂结点。  相似文献   

极地环境监测网的设计及其在南极普里兹湾的应用     

程文芳  朱建钢  吴荣荣  詹德川  陆大海  闫可  郑小罗 《海洋科学》2018,42(2):34-45

为了保护南极和北极的生态系统和环境,中国自20世纪90年代初开始推行和实施了极地环境监测计划,部署了各学科监测传感器阵列;采集了多学科数据,包括海洋、大气、冰冻圈、生物圈等主题;架构了"R/V雪龙号破冰船—极地考察站—国内基地"之间的快速数据传输网络;建立了海洋环境监测系统、太阳能地面空间监测系统、生态环境监测系统等系列监测系统。为了实现长期监测,达到预测和预警目标,本文针对国内外现状,在现有基础上设计了一套中国极地环境长期监测网(Polar Environment monitoring network of China,CPEMN)。该监测网集成各监测系统并在监测指标设计上覆盖我国极地所有常规监测/观测任务,且根据国际科研动态和长期监测规划拓展了预期监测范围。最后本文利用南极普里兹湾进行的破冰导航应用示范验证了CPEMN具有可执行性。  相似文献   

Accuracy assessment of NLCD 2011 percent impervious cover for selected USA metropolitan areas     

《International Journal of Applied Earth Observation and Geoinformation》2020

The emergence of high-resolution land cover data has created the opportunity to assess the accuracy of impervious cover (IC) provided by the National Land Cover Database (NLCD). We assessed the accuracy of the 900 m² NLCD2011 %IC for 18 metropolitan areas throughout the conterminous United States using reference data from 1 m² land cover data developed as part of the United States Environmental Protection Agency’s EnviroAtlas project. Agreement was assessed from two perspectives: 1) sensitivity to the size of the assessment unit used for the comparison, and 2) utility of NLCD %IC to serve as a proxy for high-resolution IC. The former perspective was considered because statistical relationships can be sensitive to assessment unit size and shape, and the latter perspective was considered because high resolution (reference) %IC data are not available nationwide. The utility of NLCD %IC as a proxy for the high resolution data was assessed for seven lattice (square) cell sizes ranging from 1 ha to 200 ha using four EnviroAtlas IC indicators: 1) %IC per 100 ha (1 km²); 2) %IC by Census block group; 3) %IC within a 15 m (radius) of the riparian zone, and; 4) %IC within a 50 m (radius) of the riparian zone. Agreement was quantified as per assessment unit deviation (NLCD %IC – reference %IC) and summarized as Mean Absolute Deviation (MAD) and Mean Deviation (MD) both within and across the 18 metropolitan areas. Ordinary least squares (OLS) regression (y = reference %IC and x = NLCD %IC) was also used to evaluate the quality of the NLCD %IC data. MAD was ≤ 5% for six of the seven lattice cell sizes. MAD was also ≤ 5% for Census block groups > 100 ha and for both riparian units. These results suggest that uncertainty attributable to the measurement of %IC was no greater than the uncertainty related to the effect of IC on aquatic resources that have been derived from studies of aquatic condition (e.g., benthic fauna) over a range of %IC. Overall, agreement was variable from one metropolitan area to the next. Agreement improved as assessment unit size increased and declined as the level of urbanization (NLCD %IC) increased. NLCD %IC tended to underestimate reference %IC overall, but NLCD %IC was sometimes greater than reference %IC in urbanized settings.  相似文献   

Turbulence Diffusion and Energy Spectrum Analysis of Large-scale Current Sheets in Flares     

《Chinese Astronomy and Astrophysics》2021,45(4):470-493

Magnetic reconnection (MR) is one of the most important physical processes for many dynamical phenomena in the universe. Magnetohydrodynamical (MHD) simulation is an effective way to study the MR process and the physical pictures related to the MR. With different parameter setups, we investigate the influences of the Magnetic Reynolds number and spatial resolution on the reconnection rate, numerical dissipation, and energy spectrum distribution in the MHD simulation. We have found that the magnetic Reynolds number $R_m$ has definite impact on the reconnection rate and energy spectrum distribution. The characteristic time for entering into the non-linear phase will be earlier as the Reynolds number increases. When it comes to the tearing phase, the reconnection rate will increase rapidly. On the other hand, the magnetic Reynolds number affects significantly the Kolmogorov microscopic scale $l_{\mathit{ko}}$, which becomes smaller as $R_m$ increases. An extra dissipation is defined as the combined effect of the numerical diffusion and turbulence dissipation. It is shown that the extra dissipation is dominated by the numerical diffusion before the tearing mode instability takes place. After the instability develops, the extra dissipation rises vastly, which indicates that turbulence caused by the instability can enhance the diffusion obviously. Furthermore, the energy spectrum analysis indicates that $l_{\mathit{ko}}$ of the large-scale current sheet may appear at a macroscopic MHD scale very possibly.  相似文献   

Influence of length effect on embankment slope reliability in 3D          下载免费PDF全文

Michael A. Hicks  Yajun Li 《国际地质力学数值与分析法杂志》2018,42(7):891-915

Embankment slopes composed of spatially variable soils have a variety of different failure modes that are affected by the correlation distances of the material properties and the geometry and total length of the slope. This paper examines the reliability of soil slopes for embankments of different length and uses parallel computing to analyse very long embankments (up to 100 times the embankment height) for a clay soil characterised by a spatially varying undrained shear strength. Based on a series of analyses using the 3D random finite element method (RFEM), it is first shown that the reliability of slopes of various length can be efficiently computed by combining simple probability theory with a detailed 3D RFEM analysis of a representative shorter slope of length 10 times the slope height. RFEM predictions of reliability indices for longer slopes are then compared with results obtained using Vanmarcke's (1977a) simplified 3D method and Calle's (1985) extended 2D approach. It is shown that these methods can give significantly different results, depending on the horizontal scale of fluctuation relative to the slope length, with RFEM predicting a lower slope reliability than the Vanmarcke and Calle solutions in all cases. The differences in the solutions are evaluated and attributed to differences in the assumed and computed failure surface geometries.  相似文献   

大兴安岭西盆地群域构造与地球物理场综述          下载免费PDF全文

王典  李鹏  刘财  鹿琪  单玄龙  田有  于涵  杨宝俊 《地球物理学报》2019,62(3):1106-1128

中国东北地区大兴安岭西侧盆地群包括漠河盆地、根河盆地、拉布达林盆地、海拉尔盆地和二连盆地等,蕴藏着丰富的中、新生代油气资源.为研究该盆地群域古生代、中新生代构造演化,综合建立盆地群域地球动力学模型,补充东北亚构造演化理论,本文综述该盆地群域受控的区域构造与深部构造背景、盆地群构造特征与性质、主要控盆断裂特征、盆地群油气条件比较以及盆地群域已完成并取得重要结果的地球物理工作.归纳已有主要认识和研究结果:(1)对大兴安岭西侧的盆地群起构造控制作用的构造带包括蒙古—鄂霍茨克洋缝合带、西拉木伦河缝合带、黑河—贺根山缝合带、塔原—喜桂图缝合带、西太平洋板块俯冲带,以及额尔古纳—呼伦断裂和得尔布干断裂.(2)二连盆地、海拉尔盆地和漠河盆地的盆地构造轴向与蒙古—鄂霍茨克洋缝合带走向相关;而且三个盆地内的一级构造单元走向(隆起、坳陷和推覆带)也具有这类特点.(3)几个地学断面的综合地球物理研究表明,大兴安岭西侧盆地群岩石圈地幔厚度自北向南变厚,南部盆地基底与华北地台基底表现类似;盆地群基底电性结构因受到软流圈热物质作用可能在继续演化.(4)在盆地沉积地层方面,漠河盆地的下部是侏罗系陆相煤系地层,上部是白垩系火山岩地层;海拉尔盆地由下侏罗统的铜钵庙组、南屯组,上侏罗统的大磨拐河组和下白垩统的伊敏组共同组成扎赉诺尔群,厚约3000m;二连盆地中生代地层中,中下侏罗统主要为含煤建造,上侏罗统为火山岩建造,下白垩统主要为含油建造和含煤建造,上白垩统为砂砾岩建造.(5)盆地群整体勘探程度较低.基于上述研究结果,需要进一步研究的科学问题包括:由本研究区的地球物理、构造地质、石油地质等多学科的综合研究,解决研究区受控的区域构造应力场所包括的因素及其作用,以及在岩石圈尺度上三维空间的地球物理场表征;深部构造对盆地群域构造的作用;从晚古生代到中新生代研究区构造演化特点及其依据;从北至南约1650km长的盆地群域构造差异与依据;盆地群(域)油气条件与毗邻的松辽盆地在构造成因上的差异.  相似文献   

利用海洋重力场变化分析洋底板块运动          下载免费PDF全文

李倩倩  鲍李峰  C. K. Shum 《地球物理学报》2020,63(7):2506-2515

洋底板块运动是地球动力学和全球变化研究的重要内容.本文根据质量迁移与地球外部重力场变化的对应关系,利用不同时期测高资料推算的1995—2019全球海洋重力场变化结果,反演分析全球洋底板块运动特征.研究表明,板块汇聚边界、板块内无震海岭、海山群、断裂带等区域重力异常变化显著,而在板块离散边界无明显变化趋势;西南印度洋中脊、大西洋中脊、中印度洋中脊等地区重力异常垂直梯度变化显著,且在西太平洋俯冲带、部分海岭区域也存在明显变化,其空间分布与地形基本吻合.海洋重力场变化整体上准确反映了全球洋底板块构造运动.相较于重力异常变化反演结果,重力垂直梯度的变化能够更为准确地反映洋底板块运动特征,特别是在洋中脊区域,扩张速率越小,垂直重力梯度变化越显著.此外,详细讨论了测高海洋重力场不确定因素对洋底板块运动分析结果的影响,海面坡度改正是主要因素之一.  相似文献   

电性源地-井瞬变电磁法全分量响应特性与探测能力分析   总被引：1，自引：0，他引：1       下载免费PDF全文

陈卫营  韩思旭  薛国强 《地球物理学报》2019,62(5):1969-1980

结合地面电性源瞬变电磁法（TEM）探测深度大和地-井TEM探测精度高的优点，本文提出对电性源地-井TEM进行研究.基于一维正演理论，本文对电性源在地下激发的六个电磁场分量的扩散、分布特性和探测能力进行分析研究.研究结果表明地下瞬变场各分量的分布特征与地面情况类似，但是对地层的探测能力与地面情况存在较大差别.各分量的探测能力与它们的扩散特性有关，其中受积累电荷作用，垂直电场E_z和水平磁场Ḣ_x分量对目标层的反映最为明显，E_x和Ḣ_y分量在地下扩散时受"返回电流"的影响会出现变号现象，使得异常体带来的影响被掩盖，不易被分辨.本文研究结果为发展电性源地-井TEM的施工技术、数据处理与解释，建立了相应的理论基础，获得了对该方法的初步认识.  相似文献   

汕头试验井地面与井下环境地噪声对比测试分析     

郭德顺  陈建涛  谢剑波  叶春明 《华南地震》2014,(3):57-64

试验井位于汕头市衡山路,观测系统为井下宽频地震计TBG-60B和地面宽频带地震计TDV-60B,频带为60S~50 Hz,选取的地面观测数据与对应的井下观测数据都是同一时间的,使用童汪练研究员的地噪声分析软件和MATLAB绘图工具,研究台站环境地噪声随观测井深度的变化特征,得到井深与观测地噪声之间的对比关系,为井下地震台站勘选和工程建设提供基础数据。发现地噪声水平从覆盖层进入到基岩有很大变化,从强风化层进入到中微风化层也有明显变化,考虑钻井建设成本和台站建设地噪声水平要求之间的综合效益,在粤东地区典型的地质结构条件,较佳的平衡点应该是至少需要进入完整中微风化层基岩10 m。  相似文献   

Chemical spots on the surface of the strongly magnetic Herbig Ae star HD 101412     

S. P. Jrvinen  S. Hubrig  M. Schller  I. Ilyin  T. A. Carroll  H. Korhonen 《Astronomische Nachrichten》2016,337(3):329-338

Due to the knowledge of the rotation period and the presence of a rather strong surface magnetic field, the sharp‐lined young Herbig Ae star HD 101412 with a rotation period of 42 d has become one of the most well‐studied targets among the Herbig Ae stars. High‐resolution HARPS polarimetric spectra of HD 101412 were recently obtained on seven different epochs. Our study of the spectral variability over the part of the rotation cycle covered by HARPS observations reveals that the line profiles of the elements Mg, Si, Ca, Ti, Cr, Mn, Fe, and Sr are clearly variable while He exhibits variability that is opposite to the behaviour of the other elements studied. Since classical Ap stars usually show a relationship between the magnetic field geometry and the distribution of element spots, we used in our magnetic field measurements different line samples belonging to the three elements with the most numerous spectral lines, Ti, Cr, and Fe. Over the time interval covered by the available spectra, the longitudinal magnetic field changes sign from negative to positive polarity. The distribution of field values obtained using Ti, Cr, and Fe lines is, however, completely different compared to the magnetic field values determined in previous low‐resolution FORS 2 measurements, where hydrogen Balmer lines are the main contributors to the magnetic field measurements, indicating the presence of concentration of the studied iron‐peak elements in the region of the magnetic equator. Further, we discuss the potential role of contamination by the surrounding warm circumstellar matter in the appearance of Zeeman features obtained using Ti lines. (© 2016 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献