Application of surface-wave tomography to mineral exploration: a case study from Siilinjärvi,Finland     

Federico Da Col  Myrto Papadopoulou  Emilia Koivisto  Łukasz Sito  Mikko Savolainen  Laura Valentina Socco 《Geophysical Prospecting》2020,68(1):254-269

In order to assess the feasibility and validity of surface-wave tomography as a tool for mineral exploration, we present an active seismic three-dimensional case study from the Siilinjärvi mine in Eastern Finland. The aim of the survey is to identify the formation carrying the mineralization in an area south of the main pit, which will be mined in the future. Before acquiring the data, we performed an accurate survey design to maximize data coverage and minimize the time for deployment and recollection of the equipment. We extract path-averaged Rayleigh-wave phase-velocity dispersion curves by means of a two-station method. We invert them using a computationally efficient tomographic code which does not require the computation of phase-velocity maps and inverts directly for one-dimensional S-wave velocity models. The retrieved velocities are in good agreement with the data from a borehole in the vicinity, and the pseudo three–dimensional S-wave velocity volume allows us to identify the geological contact between the formation hosting most of the mineralization and the surrounding rock. We conclude that the proposed method is a valid tool, given the small amount of equipment used and the acceptable amount of time required to process the data.  相似文献   

冕洞与太阳风高速流关系的统计研究:到达时间、持续时间和峰值强度          下载免费PDF全文

卜萱  罗冰显  刘四清  龚建村  曹勇  王宏 《地球物理学报》2019,62(2):462-472

冕洞是太阳风高速流的源区.当冕洞出现在中低纬区域时,太阳风高速流会扫过地球并引发地球空间环境扰动,如地磁暴和高能电子暴等.在太阳活动周下降年和低年,这种类型的扰动占据主导地位.因此,冕洞高速流的到达时间、峰值时间、峰值强度和持续时间等,是空间天气预报的重要内容.本文基于2010年5月到2016年12月的SDO/AIA太阳极紫外图像以及1AU处ACE和WIND卫星的太阳风观测数据,确定了160个冕洞-太阳风高速流事件,定量计算了他们的特征参数,包括冕洞与太阳风高速流的开始时间、峰值时间、峰值强度和结束时间,分析了各个特征参数的分布规律,对冕洞-高速流之间的关系进行了统计研究,并提出了一种新的预报方法,为基于冕洞成像观测的太阳风高速流的精准预报提供了依据.  相似文献   

隐伏正断层错动致地表破裂变形特征的研究     

齐剑峰  郝文拯  王晓明  张江伟 《震灾防御技术》2019,14(3):628-639

通过建立三维计算模型，对隐伏正断层在均匀错动、倾斜错动和翘倾错动方式下地表土体的应力路径、破裂和变形特征进行了研究。根据地表破裂临界值，分析了工程建设“避让带”的宽度和起始位置的变化特征。根据行业规范，提出工程建设“关注带”的确定方法，分析了“关注带”的宽度和起始位置的变化特征，得到以下主要结论:①在断层错动过程中，位于两侧的地表土体应力路径变化明显不同，下盘一侧和上盘一侧分别以三轴拉伸和三轴压缩为主；②地表强变形带与地表破裂带的分布并不一致，需要综合考虑等效塑性应变和总位移比2个指标来评价同震地表错动对建筑物的影响；③当隐伏断层错动的垂直位移达到3m时，工程建设“避让带”的宽度在10—90m范围内变化，受上覆土体厚度和断层倾角的影响最大，而工程建设“关注带”的宽度在150—400m范围内变化，受上覆土体的性质影响最大。  相似文献   

面向目标的起伏地表组合震源延时参数计算方法          下载免费PDF全文

秦龙  尹成  崔永福  刘正文  张振  方兵  陶正武 《地球物理学报》2019,62(4):1492-1501

组合震源技术通过调节延迟激发时间和震源埋藏深度能够实现地震波场的定向传播,提高地震波的照明能量和地震数据信噪比.然而,目前国内外对基于特定目标的组合震源最佳聚焦方向的选取以及起伏地表组合震源定向理论的研究相对较少.在聚焦方向选取方面,目前基本是利用多种不同延时参数的组合震源分别进行试验,从而确定较好的组合震源延时参数.本文则利用爆炸反射面原理,在目的层界面上均匀布置震源同时激发地震波,能够产生垂直于地层界面传播的平面波,当初至波传播至地表时进行地表方向统计.根据互易性原理,以初至波传播方向的反方向为聚焦方向,激发产生的地震波主波束方向将垂直入射到目的层界面上,从而精确的计算出组合震源的最佳聚焦方向.在组合震源定向方面,目前主要是利用组合震源方向因子公式进行计算,但该方法要求震源布置在同一条直线上,并不能满足起伏地表的应用要求.本文以惠更斯-菲涅尔原理为理论基础,提出通过炮点向量在聚焦方向上的投影来确定组合震源传播至虚拟波前的走时,从而确定任意起伏地表组合震源的延迟激发时间.该方法不仅能够计算出沿给定地质模型的目的层界面垂直入射的组合震源聚焦方向,也能够确定任意起伏地表情况下形成沿该聚焦方向定向传播地震波场的组合震源延迟激发时间.因此,本文提出的面向目标的起伏地表组合震源延时参数计算方法对组合震源数据采集具有理论与实践意义.  相似文献   

Simplified modeling of catchment-scale evapotranspiration via boundary condition switching     

《Advances in water resources》2014

  相似文献   

Distribution and source of heavy metals in the surface sediments from the near-shore area,north Jiangsu Province,China   总被引：1，自引：0，他引：1  

Gang Xu  Jian Liu  Shaofeng Pei  Xianghuai Kong  Gang Hu 《Marine pollution bulletin》2014

Samples of surface sediment and vibrocore were collected in the near-shore area of north Jiangsu Province for grain size, elements, ²¹⁰Pb_excess and ¹³⁷Cs analyses. In our study area, the diversity of metal concentration was controlled not by the grain size, but by the source. The element content of the old Yellow River Delta was used as baseline for our study area. Geoaccumulation indexes indicate that no station was polluted by Cu, Pb, Zn and As, but the I_geo values of As were close to zero in some stations. Slight pollution caused by Cd was observed in some stations. Correlation and enrichment factors suggest that Cu, Pb and Zn are lithogenic in origin, while As and Cd are mixed in origin. Especially, in some polluted stations Cd was obviously anthropogenic in origin.  相似文献   

Meridional circulation from differential rotation in an adiabatically stratified solar/stellar convection zone     

M. Dikpati 《地球物理与天体物理流体动力学》2014,108(2):222-235

Meridional circulation in stellar convection zones is not generally well observed, but may be critical for the workings of MHD dynamos operating in these domains. Coriolis forces from differential rotation play a large role in determining what the meridional circulation is. Here, we consider the question of whether a stellar differential rotation that is constant on cylinders concentric with the rotation axis can drive a meridional circulation. Conventional wisdom says that it can not. Using two related forms of the governing equations that respectively estimate the longitudinal components of the curl of the meridional mass flux and the vorticity, we show that such differential rotation will drive a meridional flow. This is because to satisfy anelastic mass conservation, non-spherically symmetric pressure contours must be present for all differential rotations, not just ones that depart from constancy on cylinders concentric with the rotation axis. Therefore, the fluid is always baroclinic if differential rotation is present. This is because, in anelastic systems, the perturbation pressure must satisfy a Poisson type equation, as well as an equation of state and a thermodynamic equation. We support our qualitative reasoning with numerical examples, and show that meridional circulation is sensitive to the magnitude and form of departures from rotation constant on cylinders. The effect should be present in 3D global anelastic convection simulations, particularly those for which the differential rotation driven by global convection is nearly cylindrical in profile. For solar-like differential rotation, Coriolis forces generally drive a two-celled circulation in each hemisphere, with a second, reversed flow at high latitudes. For solar like turbulent viscosities, the meridional circulation produced by Coriolis forces is much larger than observed on the Sun. Therefore, there must be at least one additional force, probably a buoyancy force, which opposes the meridional flow to bring its amplitude down to observed values.  相似文献   

On effective characteristic of Rayleigh surface wave propagation in porous fluid-saturated media at low frequencies     

《Soil Dynamics and Earthquake Engineering》2014

  相似文献   

ASO-S卫星工程科学应用系统的数据库设计          下载免费PDF全文

葛蕴翊  黎辉  黄宇  李敬伟  雷仕俊  藏京京  苏杨  封莉  李友平  李瑛  徐遵磊  李翔 《天文学报》2020,61(4):46

先进天基太阳天文台(Advanced Space-based Solar Observatory, ASO-S)卫星是我国首颗太阳观测卫星, 主要观测太阳耀斑和日冕物质抛射以及产生它们的磁场结构. ASO-S卫星的科学应用系统是科学卫星工程的6大系统之一, 它连接科学用户和卫星数据, 为将卫星的科学数据转化为科学成果提供保障. 科学应用系统的数据库是连接软件与海量数据的枢纽, 为科学数据生产和用户服务及运行提供数据层的支撑. 介绍了科学应用系统的数据库架构设计、数据库的选择以及数据库性能优化和表样例. 这里的数据库包括观测计划、工程参数、运维日志、科学数据、定标数据和特征事件识别等数据库. 这些数据库的建设将为ASO-S卫星工程科学应用系统的顺利运行提供数据支撑, 也可以为未来其他科学卫星类似数据库的搭建提供参考和借鉴.  相似文献   

火星电离层电子浓度昼夜变化特性研究          下载免费PDF全文

张学习  雷久侯  万卫星  钟嘉豪 《地球物理学报》2018,61(8):3113-3123

本文利用MAVEN卫星Langmuir Probe and Waves（LPW）仪器的在轨电子浓度探测数据，研究了火星电离层电子浓度随太阳天顶角（Solar Zenith Angle，SZA）的变化以及昼夜电子浓度变化的异同.基于2014年至2017年期间MAVEN的电子浓度数据，我们发现：在200 km以下，白天电离层电子浓度主要受光化学平衡控制，由于白天光电离过程使得昼夜电子浓度差异较大，此时电离层昼夜传输能影响到的最大范围约在SZA=110°；而在200 km以上，白天电离层受输运过程控制，此时昼夜电子浓度差别较小，电离层昼夜间电子浓度变化较为缓慢.通过研究MAVEN在deep-dip（低高度深入探测）期间的电子浓度数据，我们发现火星磁场会显著影响夜间200 km以下的电子浓度分布结构，强磁场中闭合磁力线对电子沉降过程的阻碍作用使得在夜间该区域的电子浓度小于相邻区域.同时，通过比较deep-dip期间昼夜电子浓度随高度的变化，发现夜间电子沉降作用的影响可能主要集中在160 km以下.  相似文献