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浅层反射地震方法是城市活断层探测常用的技术,但在基岩埋深比较浅的地区,往往只能识别出基岩顶面的反射波,而仅根据反射地震剖面上单个同相轴的变化很难准确判定断层是否存在.浅层地层的错断往往会引起速度的横向变化,利用高分辨折射地震方法采集的数据,应用层析成像方法获得的速度剖面,能够反映地下速度结构的变化,可以从另一方面揭示浅层断层存在的可能性.在四川某地,将这两种方法同时应用于活断层浅层地震勘探中.结果表明,两种方法联合应用可在一定程度上弥补浅层反射地震勘探方法在基岩埋深较浅地区的不足. 相似文献
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中国大陆下扬子及邻区地壳结构基本特征:深地震测深研究综述 总被引：1，自引：0，他引：1
系统回顾了20世纪70年代以来在中国大陆下扬子及其邻区开展的深地震测深工程,总结了相关宽角反射/折射地震资料的波组特征及地壳结构的基本特征。下扬子及邻区深地震测深资料普遍具有较清晰的初至震波Pg、上地壳底界面反射波P1、中地壳底界面反射波P3、莫霍界面反射波Pm及上地幔顶部首波Pn,震相连续,易追踪对比。受浅表沉积盖层或基岩等的影响,Pg波常出现局部延迟滞后或走时超前现象。尤其是大别造山带个别炮点的反射能量较弱或同相轴扭曲、波形紊乱等,均与地壳内界面和莫霍面的深度突变或破碎有关。该区域地壳结构大致分为上、中、下3层,但视资料情况中地壳和下地壳又可进一步划分为2个亚层。华北地台和扬子地台地壳厚度30~36km,莫霍界面形态变化较缓,存在局部隆起,下地壳平均速度6.7±0.3km/s。但大别造山带下方地壳厚度32~41km,莫霍界面下凹且出现4~7km垂向错断,下地壳平均速度6.8±0.2km/s。 相似文献
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通过对波动、振动和尾波的特征分析，提出以足够大的力冲击桩顶，在桩顶附近记录综合波列图，利用其振幅衰减、周期变化和反射波震相等判断桩身成型质量：波列周期均匀且较小，同时波列振幅衰减较快，而又未见明显反射波震相者桩身成型良好；而有缺陷如断裂、缩径等时波列振幅衰减变慢，反射波震相明显，且有大周期出现.它对桩的浅部（特别是桩顶下5米以内的）缺陷检测特别有效.另外利用动态PS曲线也可判断桩身成型质量：曲线较平滑者，桩身成型良好；曲线出现弯折者桩身存在缺陷，缺陷程度可参照承载力受影响大小确定. 相似文献
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用浅层折射和反射联合勘探方法在京－沪高速公路沂河桥址区进行隐伏断层和岩性垂直分带控测试验,试验是在宽约４００ｍ的水面上进行的。工作区第四系沉积层和下伏基岩对采用纵波速度作为探测物理量是敏感的,采用ＥＳ－２４０１高分辨率数字地震仪和“五小二高”的工作方法,全方位拾取折射和反射波信息,强化地质推断解释的可靠性,探测试验取得了良好的效果。 相似文献
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简要介绍了在青藏高原拉萨市附近刘吾 -大佛寺间断裂的浅层地震勘探工作 ,并进行了初步的地质解释。结果表明 ,刘吾 -大佛寺间断裂所在区域的速度模型为 5层结构。第 1层至第 4层的介质深度从 0m变化到 2 6 0m ,P波速度 80 0～ 2 0 0 0或 2 80 0m/s,介质为第四纪或第三纪覆盖层 ;第 5层的介质P波速度在 30 0 0～ 4 0 0 0m/s以上 ,其CDP图像分布零散、没有形成较强的反射界面 ,推测该区域为花岗岩类的基岩区。根据反射波组的连贯性、间断性及位置 ,判定在浅层地震勘探剖面 32 0m处存在着刘吾 -大佛寺间断裂 ,它是 1条逆断层 ,倾向NE ,倾角 80°左右 ,其上端点出现在深约 10 0m处 相似文献
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浅层地震勘探在沿海地区隐伏断层探测中的应用 总被引：16，自引：6，他引：16
中国沿海地区的第四系厚度变化较大,在大部分地区存在淤泥、黏土和砂层的多重互层情况,这种地层结构对地震波的传播十分不利,容易造成对高频信号能量的强烈耗散。沿海地区又具有人口密度大、工业干扰强烈的特点,地震波的激发、接收条件较差。文中给出了在粤东、天津和唐山覆盖层厚度变化较大的地区,利用浅层地震勘探开展隐伏断层探测的应用实例。较系统地介绍了野外工作、资料处理和解释方法。阐述了在强干扰环境下提高信噪比和分辨率的有效技术途径。所给实例中的反射波组能量强,隐伏断层的反应明显,经跨断点钻探验证,结果证实地震勘探确定的界面深度、断点位置和基岩错距等参数都是可靠的。所述技术方法对类似地区的城市活断层探测和工程物探工作都有较重要的参考价值 相似文献
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浅层地震勘探资料地质解释过程中值得重视的问题 总被引：5，自引：5，他引：5
浅层地震勘探是第四系覆盖区隐伏断层活动性研究常用的手段,叠加剖面上反射波组的分叉、合并、弯曲、中断、尖灭等被用作判断断层存在的重要标志。松花江北的吕刚屯、巨宝屯浅层地震叠加剖面上,T0为下更新统砂砾石层等松散堆积和白垩系砂岩、泥岩的分界面,反射波组清晰。T0-1波组为砂砾石层和黏土层、或砂砾石层和粉细砂层的反射界面,反射波组振幅大,能量强。根据地震反射剖面和测线上的钻孔资料,认为阿什河断层错断了下更新统下段,滨州断层错断了上更新统下段。而通过建立高精度的钻探联合地质剖面、地层年代测试和地层对比,确认阿什河断层没有错断第四系,滨州断层错断了下更新统下段。最后,从第四系的岩性、厚度变化等解释了浅层地震叠加剖面上反射波组的中断、弯曲并非断层活动的结果,而是由第四纪地层相变引起的 相似文献
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《Astronomy& Geophysics》2009,50(3):3.04-3.04
R esearch N otes
The prospect of advanced astrometric satellites raises the tantalizing possibility that we will be able to make astrometric measurements at such a precision as to place constraints on dark energy parameters. That is the premise outlined by Fiona Ding and Rupert Croft of Carnegie Mellon University, Pittsburgh, USA, in Monthly Notices of the Royal Astronomical Society , 相似文献
The prospect of advanced astrometric satellites raises the tantalizing possibility that we will be able to make astrometric measurements at such a precision as to place constraints on dark energy parameters. That is the premise outlined by Fiona Ding and Rupert Croft of Carnegie Mellon University, Pittsburgh, USA, in Monthly Notices of the Royal Astronomical Society , 相似文献
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John E. Stout 《地球表面变化过程与地形》2004,29(10):1195-1207
A basic feature of any wind‐eroding surface is its threshold – the wind speed at which sediment transport is initiated. A new method was developed and tested that allows for the rapid determination of threshold under natural wind conditions in the ?eld. A mathematical expression that relates saltation activity and relative wind strength was reformulated so that threshold may be calculated from measurements of saltation activity and the mean and standard deviation of wind speed. To test the new method and determine its usefulness, a ?eld experiment was performed within a region of low‐relief dunes on the Southern High Plains of West Texas. The experimental system consisted of a 2‐m meteorological tower and a piezoelectric saltation sensor. It was found that during periods of active aeolian activity, threshold values could be calculated every 5 minutes. This new method allows for routine monitoring of surface threshold conditions in the ?eld. Example threshold calculations are presented and they demonstrate that the method works well. Published in 2004 by John Wiley & Sons, Ltd. 相似文献
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Analytic expressions for the velocity sensitivity to the elastic moduli for the most general anisotropic media 总被引：1，自引：0，他引：1
For non‐linear kinematic inversion of elastic anisotropy parameters and related investigations of the sensitivity of seismic data, the derivatives of the wavespeed (phase velocity and group velocity) with respect to the individual elastic moduli are required. This paper presents two analytic methods, called the eigenvalue and eigenvector methods, to compute the derivatives of the wavespeeds for wave propagation in a general anisotropic medium, which may be defined by up to 21 density‐normalized elastic moduli. The first method employs a simple and compact form of the eigenvalue (phase velocity) and a general form of the group velocity, and directly yields general expressions of the derivatives for the three wave modes (qP, qS1, qS2). The second method applies simple eigenvector solutions of the three wave modes and leads to other general forms of the derivatives. These analytic formulae show that the derivatives are, in general, functions of the 21 elastic moduli as well as the wave propagation direction, and they reflect the sensitivity of the wavespeeds to the individual elastic moduli. Meanwhile, we give results of numerical investigations with some examples for particular simplified forms of anisotropy. They show that the eigenvalue method is suitable for the qP‐, qS1‐ and qS2‐wave computations and mitigates the singularity problem for the two quasi‐shear waves. The eigenvector method is preferable to the eigenvalue method for the group velocity and the derivative of the phase velocity because it involves simpler expressions and independent computations, but for the derivative of the group velocity the derivative of the eigenvector is required. Both methods tackle the singularity problem and are applicable to any degree of seismic anisotropy for all three wave modes. 相似文献
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Ruth Bamford, Robert Bingham and Mike Hapgood discuss the physics behind shielding spacecraft from solar and cosmic radiation with mini-magnetospheres. 相似文献
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C.R. Brewitt-Taylor 《Physics of the Earth and Planetary Interiors》1975,10(2):151-158
A model for the coast-effect of geomagnetism is presented, in which the horizontal magnetic field induces currents in a circuit including a thin finite ocean. The currents flow horizontally across the ocean, vertically down into the earth, back through the deep interior of the earth, and vertically up to the ocean to complete the current loop. The upper layers of the earth are given non-zero conductivity, allowing the possibility of such current loops.A two-dimensional model involving such currents has been worked out analytically, and it is found that a significant induced magnetic field at the seafloor can be obtained with a reasonable conductivity in the earth's upper layers. A three-dimensional model has also been worked out numerically. It is found that the induced vertical component of magnetic field is of comparable magnitude to the horizontal component induced normal to the coast, whereas the horizontal component parallel to the coast is small. These relations are required to explain the observation of Parkinson arrows. 相似文献
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Projects to drill into and recover samples from active faults are progressing in two widely separated locations: off the coast of Japan and in California. 相似文献