应用探地雷达探测活动断层

在浅覆盖区采用探地雷达探测地震活动断层。通过实验确定出最佳的采集参数和数据处理流程,在雷达剖面上,能够清晰地显示出断层上部的形态特征、上断点埋深和岩土分层。结合钻孔资料,利用雷达剖面上对第四系覆盖的分层结果和上断点所在的层位可以分析和评价断层的活动性。     

川滇地区地震(Ms≥5.0)破裂类型与前兆异常分布的关系

对川滇地区 31次 (组 ) 5 .0级以上地震与余震次数的关系进行了统计 ,结合“强地震分为走滑型地震和断错型地震”的理论 ,确定了各次 (组 )地震的破裂类型。从物理机制上对地震破裂类型与震前前兆异常分布关系进行了讨论 ,由此进一步探讨了 5 .0级以上地震震后趋势预测     

Presolar spinel grains from the Murray and Murchison carbonaceous chondrites

With a new type of ion microprobe, the NanoSIMS, we determined the oxygen isotopic compositions of small (<1μm) oxide grains in chemical separates from two CM2 carbonaceous meteorites, Murray and Murchison. Among 628 grains from Murray separate CF (mean diameter 0.15 μm) we discovered 15 presolar spinel and 3 presolar corundum grains, among 753 grains from Murray separate CG (mean diameter 0.45 μm) 9 presolar spinel grains, and among 473 grains from Murchison separate KIE (mean diameter 0.5 μm) 2 presolar spinel and 4 presolar corundum grains. The abundance of presolar spinel is highest (2.4%) in the smallest size fraction. The total abundance in the whole meteorite is at least 1 ppm, which makes spinel the third-most abundant presolar grain species after nanodiamonds (if indeed a significant fraction of them are presolar) and silicon carbide. The O-isotopic distribution of the spinel grains is very similar to that of presolar corundum, the only statistically significant difference being that there is a larger fraction of corundum grains with large ¹⁷O excesses (¹⁷O/¹⁶O > 1.5 × 10⁻³), which indicates parent stars with masses between 1.8 and 4.5 M_⊙.     

民乐、山丹6.1级地震异常及台站实现短临预报的思考

在综合分析了民乐-山丹6.1级地震前张掖中心台范围内震兆异常特征的基础上,总结了本次地震前该台的短临预报过程及存在的问题,对今后台站如何搞好地震短临预报工作进行了探讨.     

Image processing of 2D resistivity data for imaging faults

A methodology to locate automatically limits or boundaries between different geological bodies in 2D electrical tomography is proposed, using a crest line extraction process in gradient images. This method is applied on several synthetic models and on field data set acquired on three experimental sites during the European project PALEOSIS where trenches were dug. The results presented in this work are valid for electrical tomographies data collected with a Wenner-alpha array and computed with an l₁ norm (blocky inversion) as optimization method. For the synthetic cases, three geometric contexts are modelled: a vertical and a dipping fault juxtaposing two different geological formations and a step-like structure. A superficial layer can cover each geological structure. In these three situations, the method locates the synthetic faults and layer boundaries, and determines fault displacement but with several limitations. The estimated fault positions correlate exactly with the synthetic ones if a conductive (or no superficial) layer overlies the studied structure. When a resistive layer with a thickness of 6 m covers the model, faults are positioned with a maximum error of 1 m. Moreover, when a resistive and/or a thick top layer is present, the resolution significantly decreases for the fault displacement estimation (error up to 150%). The tests with the synthetic models for surveys using the Wenner-alpha array indicate that the proposed methodology is best suited to vertical and horizontal contacts. Application of the methodology to real data sets shows that a lateral resistivity contrast of 1:5–1:10 leads to exact faults location. A fault contact with a resistivity contrast of 1:0.75 and overlaid by a resistive layer with a thickness of 1 m gives an error location ranging from 1 to 3 m. Moreover, no result is obtained for a contact with very low contrasts (1:0.85) overlaid by a resistive soil. The method shows poor results when vertical gradients are greater than horizontal ones. This kind of image processing technique should be systematically used for improving the objectiveness of tomography interpretation when looking for limits between geological objects.     

内蒙古中部构造混杂带晚古生代-早中生代变质基性岩的地球化学特征及其大地构造意义

内蒙古中部构造混杂带中的变质基性岩可分为南、北两带:南带位于乌兰沟-图林凯地区,被划分至温都尔庙群下部的桑达来因组,主要为一套变质玄武岩和辉长岩、辉绿岩,局部含有超基性岩和碳酸岩透镜体,其中变质基性火山岩以绿片岩相变质为主,局部保留枕状构造或发育蓝片岩,已有的锆石U-Pb年代学数据表明南带变质基性火山岩形成于晚古生代到早中生代;北带位于芒和特-二道井-红格尔一线,主要呈岩块状保存在由绢云绿泥石英片岩、硅质岩、含铁石英岩和少量的大理岩组成的基质中,岩石类型包括蓝片岩、冻蓝闪石片岩、阳起片岩、绿帘角闪片岩等。地球化学研究显示南、北两带的变质基性岩相对低Al(Al2O3=10.66%~14.97%)、低Ti(TiO2=1.27%~1.96%)、高Na(Na2O=1.02%~4.20%)、贫K(K2O=0.02%~0.71%),具有拉斑玄武岩到碱性玄武岩系列的过渡特征,高的Na2O/K2O比值(6.89~454)暗示这些基性岩在变质作用前发生了细碧角斑岩化。不活动元素Zr与其他高场强元素(HSFE;Th、Nb、Hf、Ti)和稀土元素(REE)显示良好的线性关系,表明在变质过程中,高场强元素和稀土元素基本保持稳定,可以反映原岩的性质。根据稀土、微量元素配分型式和相关比值可以将内蒙中部构造混杂带中的变质基性岩分为两类:一类稀土含量相对较低(∑REE=46.00×10-6~78.08×10-6)、轻重稀土分异不明显((La/Yb)N=0.50~1.04),无明显Eu负异常,Hf/Ta=6.82~15.18,具有正常的大洋中脊玄武岩(NMORB)特征;另一类稀土含量相对较高(∑REE=58.66×10-6~151.3×10-6)、轻重稀土分异明显((La/Yb)N=2.28~4.68),无明显Eu负异常,Hf/Ta=2.06~4.70,与富集型洋中脊玄武岩(E-MORB)相似。部分变质基性岩样品轻微富集大离子亲石元素Rb和Ba,可能暗示原岩在就位过程中遭受了微弱的陆壳混染。以上地球化学特征表明这些变质基性岩的原岩可能形成于一个扩张规模有限的陆内洋盆环境。已有的古生物地理学研究表明古亚洲洋闭合后,到晚古生代早期,内蒙古中部地区成为佳-蒙地块的一部分。石炭纪期间整个内蒙古中部发育稳定的浅海相沉积,局部为造山后隆起环境,发育加里东I型花岗岩和花岗闪长岩。从晚石炭世-早二叠世起,内蒙中部开始处于伸展环境:二连浩特到东乌珠穆沁旗一带发育大量的碱性岩;华北克拉通北缘发育很多高钾钙碱性-碱性的花岗岩;内蒙中部地区广泛发育二叠纪大石寨组双峰式火山岩。到中二叠世开始裂解形成若干近东西向分布的海盆,发育哲斯组、林西组浅海相、泻湖相沉积。持续的伸展形成了有限洋盆,发育以温都尔庙群为代表的含铁硅质岩以及晚古生代-早中生代基性岩。由于早中三叠世华北板块与扬子板块全面碰撞和陆内造山过程的影响,有限洋盆最终在早中生代之后发生被动闭合,形成南、北构造混杂带,并导致该基性岩乃至整个内蒙中部的晚古生代沉积发生广泛绿片岩相变质作用,而局部蓝片岩的形成可能与有限洋盆的俯冲作用有关。     

西藏冈底斯带阿索构造混杂岩南侧亚布努马花岗斑岩地球化学特征及锆石U-Pb年龄

西藏中冈底斯北部尼玛县阿索乡亚布努马地区东侧出露一处花岗斑岩岩脉,LA-ICP-MS锆石U-Pb测年结果显示,该花岗斑岩的形成时代为晚侏罗世(161.2±5.9Ma)。全岩地球化学数据显示其高硅、富碱、富铝的特征,属于碱性准铝质花岗斑岩;富集轻稀土元素,轻、重稀土元素分异明显,具有明显的负Eu异常,富集Rb、Pb等大离子亲石元素,亏损Ba、Sr元素及Nb、Ta、Ti、U等高场强元素,形成于岛弧环境。其源区可能为来自俯冲带增厚下地壳的深熔作用,结合区域上同时代的岩浆事件,亚布努马花岗斑岩应该形成于以班公湖-怒江洋南向俯冲为动力背景的陆缘弧环境。     

混凝土单桩对瑞利波的阻隔机理试验研究

通过室外试验的方法绘制相对加速度的二维等值线图,并依据桩周土体的振动情况进行区域划分,进一步研究单桩几何尺寸变化时其周围土体振动区域的变化情况.结果表明:单桩桩前、桩两侧存在振动加强区,桩前的振动加强现象更强,以桩角处尤为明显;当桩长与波长的比值在0.109～0.840时,隔振区、反射区的面积增长幅度较大,而绕射区的面...     

TBM机施工隧道瞬变电磁超前探测研究

在隧道掘进机(TBM)施工隧道内,传统瞬变电磁的装置形式受到了TBM机械的限制,TBM自身的金属构件对二次场衰减电压的采集产生了强烈的电磁干扰.为了克服瞬变电磁法在TBM施工隧道内遇到的困难,在前人工作的基础上,尝试提出了一种基于电性源激发、电场分量采集的施工隧道瞬变电磁超前探测装置形式.针对钻爆法与TBM施工隧道各自不同的工况,利用三维时域有限差分法对单个电性源激励下隧道前方瞬变电磁场的分布规律与响应特征进行了正演模拟.通过对瞬变电磁场的分布规律以及响应特征进行分析,认为所述的电性源发射装置不仅可以在钻爆法施工隧道内使用,并且具有在TBM施工隧道内进行隧道超前预报的能力.