非饱和土地基中复合多层波阻板对S波的隔离效应     

舒进辉  马强  常立君 《岩土力学》2023,44(1):217-231

基于弹性波在非饱和多孔介质与单相弹性介质中的传播理论,考虑在非饱和土地基中设置一定厚度的复合多层波阻板（复合多层波阻板以3层为例）,利用Helmholtz矢量分解定理,推导了非饱和土地基中S波通过复合多层波阻板的透射、反射振幅比的解析解。通过数值算例,分析了层间波阻板剪切模量和密度等物理力学参数对非饱和土地基中S波通过复合多层波阻板时传播特性的影响规律。结果表明：复合多层波阻板中层间波阻板材料的剪切模量和密度对透反射系数影响显著。复合多层波阻板是一种有效的隔振屏障,严格控制层间波阻板的剪切模量和密度可以获得最佳隔振效果,这为复合多层波阻板在地基振动控制领域中的应用提供理论指导。  相似文献   

基于A- CGAN的深反射地震数据随机噪声压制方法研究     

韩建光  王卿  许媛  刘志伟 《地质论评》2023,69(4):2023040015-2023040015

基于深度学习的地震数据噪声压制方法是当前地震数据去噪处理的重要方向。深度学习方法突破了传统滤波处理的局限,在对常规地震数据的噪声压制中表现出效率高、信噪分离效果好的特点。但针对深部弱有效反射数据,当前的深度学习方法特征提取能力有限,难以取得较好的去噪效果。笔者等结合深反射地震数据特点,针对当前深度学习噪声压制方法在特征提取及对数据集依赖上的局限,提出了基于注意力循环生成对抗网络(Attention Cycle- Consistent Generative Adversarial Networks,A- CGAN)的深反射地震数据随机噪声压制方法。借助循环一致生成对抗网络(Cycle- Consistent Generative Adversarial Networks,Cycle- GAN)的域映射思想,降低对数据集的要求。为了构建适用于深反射地震数据的去噪网络,从3个方面对Cycle- GAN进行改进：在Cycle- GAN的生成器（去噪器）中加入残差结构和注意力机制,用于加深网络深度和提高其特征提取能力;在Cycle- GAN的鉴别器中使用块判决,提高鉴别精度和准确度;在损失函数部分加入感知一致性损失函数,提升网络模型恢复纹理细节信息的能力。通过合成地震数据和实际深反射地震数据测试,验证了优化算法的有效性,体现了良好的应用价值。  相似文献   

开封断裂第四纪活动特征     

孙杰  张予川  徐婉君  李涛  张扬 《震灾防御技术》2022,17(2):234-241

开封断裂是郑州-开封断裂带的重要组成部分,也是黄河中下游平原的一条重要控制性断裂。利用浅层地震勘探发现,开封断裂为总体走向EW,倾向N的正断层;断裂分为东、西2支,断裂活动性具有明显的分段特征,东支活动性较西支强。钻孔联合剖面揭示开封断裂东支断裂上断点埋深27～35 m,根据地层年代学结果,其最新活动时间为晚更新世。研究成果为开封市城乡规划、重大工程选址和地震区划工作提供了重要的基础数据。  相似文献   

基于反射地震资料探讨泥河湾盆地的新生代和中生代地层     

朱小三  钱荣毅  王永  董进  迟振卿  姚培毅 《地质学报》2015,89(12):2236-2249

查明泥河湾盆地新生界及中生界地层序列及基底的分布与赋存形态是研究泥河湾盆地形成机制的基础性工作。本研究在泥河湾盆地桑干河与壶流河交接处附近采集了四条测线的反射地震数据,通过对精细处理后的地震剖面进行详细分析,在剖面上厘定了三个具有明显强反射标志的地层,即古近系的玄武岩、侏罗系上统的含煤地层和侏罗系下统的含煤地层;其中,新近系沉积层与古近系玄武岩界面在地震剖面上出现的双程旅行时为0.3~0.6s,深度范围为300~500m,而第四系泥河湾组底界由南西到北东逐渐加深,其界面深度为200~300m;侏罗系上统含煤地层在地震剖面上出现的双程旅行时在0.8s上下波动,其深度约为1200m,探测出侏罗系上统顶界面的深度范围为800~1100m;侏罗系下统含煤地层在地震剖面上出现的双程旅行时为1.0~1.4s,深度范围为1800~2000m,由此推测出中生界侏罗系与古生界寒武系地层分界线的深度为2000m左右;根据地震反射波阻抗差别推测出新元古界和太古界地层的分界面在地震剖面上出现的时间约为2.5s,其深度为4000m左右。本研究通过四条反射地震测线的数据基本上查明了泥河湾盆地位于探测区处第四系泥河湾组底界面的深度分布范围及起伏形态、侏罗系上统顶界面和下统底界面的大致埋深,为查明泥河湾盆地新生界及中生界地层序列提供了基础性的参考信息。  相似文献   

Reflection effect in close binaries. IV. Limb darkening of the reflected radiation incident from an extended surface of the secondary     

A. Peraiah  M. Srinivasa Rao 《Journal of Astrophysics and Astronomy》1983,4(3):175-182

The law of limb darkening has been calculated when the atmosphere of the primary component is illuminated by the extended surface of the secondary component in a binary system. The specific intensities calculated at infinity show marked changes when the plane-parallel approximation is replaced by the assumption of spherical symmetry. The middle portions of the illuminated surface reflect maximum radiation while the innermost and outermost layers show lesser amount of reflected radiation.  相似文献   

Emission line widths of an asymmetric bowshock inside a cloud of dust     

W. J. Henney 《Astrophysics and Space Science》1995,224(1-2):481-482

A model is presented that explains the anomalous emission line widths in the Herbig-Haro object HH 1 in terms of emission from a lop-sided bowshock and scattering by surrounding dust.  相似文献   

Common reflecting elements (CRE) ray tracing for the calculation of the global multi-offset time field     

Z. Koren  B. Gelchinsky 《Geophysical Journal International》1989,99(2):391-400

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High velocities and seismic anisotropy in Pleistocene turbidites off Western Canada     

Earl E. Davis  Ron M. Clowes 《Geophysical Journal International》1986,84(2):381-399

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Reflection effect in close binaries. II. Distribution of emergent radiation from the irradiated component along the line of sight     

A. Peraiah 《Journal of Astrophysics and Astronomy》1983,4(1):11-17

We have calculated the effects of irradiation from a point source observed at infinity. Plane-parallel approximation and spherically-symmetric approximations are employed in calculating the self-radiation field for the sake of comparison. It is found that there are considerable changes in the radiation received at infinity between the approximation of plane-parallel stratification and spherical symmetry.  相似文献   

Constraining models of the tectonic setting of the giant Olympic Dam iron oxide–copper–gold deposit, South Australia, using deep seismic reflection data     

Barry Drummond  Patrick Lyons  Bruce Goleby  Leonie Jones 《Tectonophysics》2006,420(1-2):91

In the Gawler Craton, the completeness of cover concealing the crystalline basement in the region of the giant Olympic Dam Cu–Au deposit has impeded any sufficient understanding of the crustal architecture and tectonic setting of its IOCG mineral-system. To circumvent this problem, deep seismic reflection data were recently acquired from  250 line-km of two intersecting traverses, centered on the Olympic Dam deposit. The data were recorded to 18 s TWT ( 55 km). The crust consists of Neoproterozoic cover, in places more than 5 km thick, over crystalline basement with the Moho at depths of 13–14 s TWT ( 40–42 km). The Olympic Dam deposit lies on the boundary between two distinct pieces of crust, one interpreted as the Archean–Paleoproterozoic core to the craton, the other as a Meso–Neoproterozoic mobile belt. The host to the deposit, a member of the  1590 Ma Hiltaba Suite of granites, is situated above a zone of reduced impedance contrast in the lower crust, which we interpret to be source-region for its  1000 °C magma. The crystalline basement is dominated by thrusts. This contrasts with widely held models for the tectonic setting of Olympic Dam, which predict extension associated with heat from the mantle producing the high temperatures required to generate the Hiltaba Suite granites implicated in mineralization. We use the seismic data to test four hypotheses for this heat-source: mantle underplating, a mantle-plume, lithospheric extension, and radioactive heating in the lower crust. We reject the first three hypotheses. The data cannot be used to reject or confirm the fourth hypothesis.  相似文献