提高任意广角波动方程计算效率及压制倏逝波干扰方法   总被引：1，自引：1，他引：0       下载免费PDF全文

周辉  陈汉明  李绪宣  范廷恩 《地球物理学报》2014,57(4):1188-1198

任意广角波动方程（Arbitrarily Wide-angle Wave Equation,AWWE）是一种高精度的时空域单程波动方程,与其他时空域单程波方程相比,具有更大的成像倾角,因此是偏移成像的有力工具之一.本文改进了现有的AWWE有限差分计算方案,避免了原计算方案中对矩阵反复求逆的过程,同时减少了矩阵相乘的次数,显著地提高了AWWE数值计算的效率.数值实验证实,采用改进之后的计算方案,其计算结果与原方案完全一致.此外,本文采用了一种方法,在有倏逝波干扰的情况下,能在频率-波数（f-k）域区分出倏逝波与非倏逝波,为设计f-k滤波器提供合理的视速度门槛信息.偏移实验证实,在深度延拓时仅仅进行数次f-k滤波就能很好地抑制倏逝波干扰,提高偏移成像质量.  相似文献   

Generalized diffraction‐stack migration and filtering of coherent noise     

Ge Zhan  Wei Dai  Min Zhou  Yi Luo  Gerard T. Schuster 《Geophysical Prospecting》2014,62(3):427-442

We reformulate the equation of reverse‐time migration so that it can be interpreted as summing data along a series of hyperbola‐like curves, each one representing a different type of event such as a reflection or multiple. This is a generalization of the familiar diffraction‐stack migration algorithm where the migration image at a point is computed by the sum of trace amplitudes along an appropriate hyperbola‐like curve. Instead of summing along the curve associated with the primary reflection, the sum is over all scattering events and so this method is named generalized diffraction‐stack migration. This formulation leads to filters that can be applied to the generalized diffraction‐stack migration operator to mitigate coherent migration artefacts due to, e.g., crosstalk and aliasing. Results with both synthetic and field data show that generalized diffraction‐stack migration images have fewer artefacts than those computed by the standard reverse‐time migration algorithm. The main drawback is that generalized diffraction‐stack migration is much more memory intensive and I/O limited than the standard reverse‐time migration method.  相似文献   

Crust and upper mantle structures beneath Northeast China from receiver function studies          下载免费PDF全文

Zhen Guo  Yuliang Cao  Xianguang Wang  Y. John Chen  Jieyuan Ning  Weiguang He  Youcai Tang  Yongge Feng 《地震科学（英文版）》2014,27(3):265-275

P-wave and S-wave receiver function analyses have been performed along a profile consisted of 27 broadband seismic stations to image the crustal and upper mantle discontinuities across Northeast China. The results show that the average Moho depth varies from about 37 km beneath the Daxing’anling orogenic belt in the west to about 33 km beneath the Songliao Basin, and to about 35 km beneath the Changbai mountain region in the east. Our results reveal that the Moho is generally flat beneath the Daxing’anling region and a remarkable Moho offset (about 4 km) exists beneath the basin-mountain boundary, the Daxing’anling-Taihang Gravity Line. Beneath the Tanlu faults zone, which seperates the Songliao Basin and Changbai region, the Moho is uplift and the crustal thickness changes rapidly. We interpret this feature as that the Tanlu faults might deeply penetrate into the upper mantle, and facilitate the mantle upwelling along the faults during the Cenozoic era. The average depth of the lithosphere-asthenosphere boundary (LAB) is ~80 km along the profile which is thinner than an average thickness of a continental lithosphere. The LAB shows an arc-like shape in the basin, with the shallowest part approximately beneath the center of the basin. The uplift LAB beneath the basin might be related to the extensive lithospheric stretching in the Mesozoic. In the mantle transition zone, a structurally complicated 660 km discontinuity with a maximum 35 km depression beneath the Changbai region is observed. The 35 km depression is roughly coincident with the location of the stagnant western pacific slab on top of the 660 km discontinuity revealed by the recent P wave tomography.  相似文献   

Rebuttal to the comment by Malhotra and Strom on “Constraints on the source of lunar cataclysm impactors”     

Matija ?uk  Brett J. Gladman 《Icarus》2011,216(1):363-365

?uk et al. (?uk, M. Gladman, B.J., Stewart, S.T. [2010]. Icarus 207 590-594) concluded that the the lunar cataclysm (late heavy bombardment) was recorded in lunar Imbrian era craters, and that their size distribution is different from that of main belt asteroids (which may have been the dominant pre-Imbrian impactors). This result would likely preclude the asteroid belt as the direct source of lunar cataclysm impactors. Malhotra and Strom (Malhotra, R., Strom, R.G. [2011]. Icarus) maintain that the lunar impactor population in the Imbrian era was the same as in Nectarian and pre-Nectarian periods, and this population had a size distribution identical to that of main belt asteroids. In support of this claim, they present an Imbrian size distribution made from two data sets published by Wilhelms et al. (Wilhelms, D.E., Oberbeck, V.R., Aggarwal, H.R. [1978]. Proc. Lunar Sci. Conf. 9, 3735-3762). However, these two data sets cannot be simply combined as they represent areas of different ages and therefore crater densities. Malhotra and Strom (Malhotra, R., Strom, R.G. [2011]. Icarus) differ with the main conclusion of Wilhelms et al. (Wilhelms, D.E., Oberbeck, V.R., Aggarwal, H.R. [1978]. Proc. Lunar Sci. Conf. 9, 3735-3762) that the Nectarian and Imbrian crater size distributions were different. We conclude that the available data indicate that the lunar Imbrian-era impactors had a different size distribution from the older ones, with the Imbrian impactor distribution being significantly richer in small impactors than that of older lunar impactors or current main-belt asteroids.  相似文献   

基于波场垂向和水平方向外推的高陡构造偏移          下载免费PDF全文

陈生昌  张博 《地球物理学报》2012,55(4):1300-1306

常规的单程波波动方程偏移成像方法对大角度的高陡构造偏移成像存在内在的限制.根据波动方程在各个空间方向的数学特性和高陡构造反射地震波的传播特征,通过把地震波分解为垂向的上下行波、水平方向的前后行波和左右行波,提出基于波场垂向外推和水平方向外推相结合的单程波波动方程高陡构造偏移成像方法,即用波场垂向外推的单程波波动方程偏移成像方法解决中低角度平缓构造的偏移成像,用波场水平方向外推的单程波波动方程偏移成像方法解决中高角度陡倾构造的偏移成像.这种基于波场垂向和水平方向外推相结合的高陡构造偏移成像方法是常规单程波波动方程叠前深度偏移成像方法的补充和改进,它相对基于全波方程的逆时偏移具有计算效率上的优势.  相似文献   

非洲的移民汇款及其对国家发展的作用     

丁金宏 《世界地理研究》2008,27(3):26-36

近几十年,全球汇款流在稳步增长并越来越成为发展中国家财政发展的重要源泉。汇款成为家庭收入中稳定的一部分,并组成了发展中国家第二大资金流——处于外国直接投资（FDI）之后,海外开发援助（ODA）之前。在撒哈拉以南非洲地区,流动工人的汇款成为财政发展以及救助穷人的财政服务的重要主题。本论文分析撒哈拉以南非洲地区迁移人口的汇款及其作用,并以马里作为重点研究对象。研究结论是,汇款在国家收入中占有重要比例,并将继续对个人家庭和社区提供重要支持,应该鼓励当地引导汇款促进基础设施发展和收入产生。  相似文献   

闽台主要城市人口迁移模式及其与经济发展耦合关系的比较分析     

CHEN Yan-hua  韦素琼 《世界地理研究》2008,17(2):129-136

在不同经济模式下的城市人口迁移模式及其与经济发展的耦合关系都必然存在着差异,这里选取了具有典型的地理相似性和经济发展时序递差性的福建省和台湾省的主要城市（福州、厦门、泉州和台北、基隆、台中、台南、高雄）为研究对象,从迁入人口、迁出人口和净迁移人口3个角度,详尽地比较分析了这8大主要城市人口迁移模式的特征和差异,并在此基础上分别建立了闽台城市人口迁移模式与其社会经济发展阶段的耦合关系,以期能够为福建省未来的人口迁移的发展和管理提供一定的借鉴作用.  相似文献   

金属矿地震绕射波分离与成像——以庐枞矿集区和钦杭成矿带为例     

王志辉  吕庆田 《地球学报》2017,38(S1):79-82

不同于油气藏能源大多产于沉积地层之中, 金属矿成矿部位的地质条件要更为复杂多变。通常情况下矿体表现为不规则形状, 且连续性较差, 难以满足现有地震反射波法所以依据的镜面反射条件(徐明才等, 2009)。不同的围岩地震地质条件差异很大, 甚至同一种岩性受到蚀变、构造作用的影响, 表现出不同的阻抗特征, 当围岩与矿体间的波阻抗差异较小, 难以形成有效的反射波。在控矿构造方面, 通常大规模的构造对成矿具有控矿、控岩作用, 而与成矿部位密切相关的一般是小规模的断裂, 反射波较难识别。根据菲涅耳带理论, 当地质体的尺度小于地震波的一个波长时, 反射地震成像精度会骤降, 而来自这些小尺度、非均匀地质体产生的绕射波和散射波成像较反射波成像具有明显的高分辨率、甚至超高分辨率。利用绕射波成像能够探测和识别地下重要的构造信息, 如破碎带、断层、尖灭点、礁体边界、次火山岩、小尺度的侵入体、不规则盐丘体, 以及其他不连续的地质体(Karimpoul et al., 2015)。考虑金属矿围岩及控矿构造复杂, 矿体几何尺寸较小、形状不规则, 容易产生绕射波, 理论上利用地震绕射波识别这些地质体较反射波更具优势。  相似文献   

基于平面波照明的偏移成像补偿   总被引：1，自引：0，他引：1       下载免费PDF全文

陈生昌  王汉闯 《地球物理学报》2010,53(7):1710-1715

受地下复杂构造和地震数据采集系统的影响,地震波对地下目标的照明出现不均匀,在地震数据的偏移成像中出现成像阴影.根据地震数据最小二乘偏移/反演理论,和把地震波场照明结果作为最小二乘偏移/反演中的Hessian矩阵的近似对偏移成像进行补偿的原理,提出一种应用平面波照明结果对平面波偏移成像结果进行补偿以消除偏移成像阴影的方法.这种基于平面波照明的偏移成像补偿方法相对于局部角度域的照明偏移成像补偿方法具有计算效率上的优势.  相似文献   

Migration for velocity and attenuation perturbations   总被引：1，自引：0，他引：1  

Bobby Hak  Wim A. Mulder 《Geophysical Prospecting》2010,58(6):939-952

Migration maps seismic data to reflectors in the Earth. Reflections are not only caused by small‐scale variations of the velocity and density but also of the quality factor that describes attenuation. We investigated scattering due to velocity and attenuation perturbations by computing the resolution function or point‐spread function in a homogeneous background model. The resolution function is the migration image of seismic reflection data generated by a point scatterer. We found that the resolution function mixes velocity and attenuation parameter perturbations to the extent that they cannot be reconstructed independently. This is true for a typical seismic setting with sources and receivers at the surface and a buried scatterer. As a result, it will be impossible to simultaneously invert for velocity and attenuation perturbations in the scattering approach, also known as the Born approximation. We proceeded to investigate other acquisition geometries that may resolve the ambiguity between velocity and attenuation perturbations. With sources and receivers on a circle around the scatterer, in 2D, the ambiguity disappears. It still shows up in a cross‐well setting, although the mixing of velocity and attenuation parameters is less severe than in the surface‐to‐surface case. We also consider illumination of the target by diving waves in a background model that has velocity increasing linearly with depth. The improvement in illumination is, however, still insufficient to remove the ambiguity.  相似文献