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1.
利用中国大陆东部21个台站的43条面波大圆路径上瑞利面波记录的双台资料,计算出双台间地震面波相速度频散,采用Tarantola概率反演的方法求得相速度频散曲线的分布,并由各处相速度频散曲线反演得到地壳上地幔的三维横波波速图像,进而得到中国东部地壳上地幔的S波速度结构.结果表明:我国大陆东部地壳厚度总体上呈东薄西厚的趋势,以105°E为界向西地壳厚度逐渐加深到55 km以上,其中有一个北东向的h形地壳厚度的坡度带.豫西及晋南地区为相对薄地壳的地区.大别山地区和泰山附近地区地壳变厚,但秦岭地区地壳不变厚.上地幔低速层上界面的深度在华北地区较浅,为80-90km,在鄂尔多斯、四川东部以及黔湘地区为120-130km.扬子地块东部及华南褶皱系中、东部上地幔顶部速度偏低使低速层的速度反差不明显.滇黔褶皱系的西部在200 km以内的上地幔中未出现低速层. 相似文献
2.
面波频散和接收函数是研究地壳上地幔速度结构的重要方法.面波频散对绝对S波速度较为敏感,但对界面结构约束不强;而接收函数对间断面具有很好的分辨能力.二者优势互补,通过联合反演,可以得到更为准确的壳幔内部界面及绝对S波速度结构.近十几年来,随着噪声地震学的迅猛发展以及大量宽频带地震仪的架设,该联合反演方法得到了更进一步的应用.为了便于梳理该研究方向的脉络,本文分别回顾了面波频散与体波接收函数的方法原理及其在壳幔结构反演中的应用,并分析了两种方法的优势与不足.在此基础上,介绍了二者的联合反演方法,以及在地壳上地幔速度结构研究中的应用.展望了联合反演方法的进一步发展,以及加入多种地球物理观测数据对反演地壳上地幔结构的意义. 相似文献
3.
本文对利用体波波形资料研究地壳上地幔速度结构的理论与方法进行了系统的研究 ,通过引入非线性反演中的遗传算法 ,发展了一种灵活有效的体波波形反演方法。利用中国的CDSN台网和中美合作在青藏高原架设的PASSCAL临时地震台站记录的宽频带体波波形资料 ,对中国大陆地区地壳上地幔速度结构进行了研究。在青藏高原地区 ,通过对高原中部地区瑞利波衰减特性及相速度频散特性的测定 ,反演了该地区地壳上地幔的 Qβ结构和 S波速度结构 ,并对 S波速度的横向不均匀特征进行了探讨。本文对上地幔速度结构的主要研究方向进行了系统的总结 ,这些… 相似文献
4.
华北地区三维地壳上地幔结构 总被引：40，自引：7，他引：33
本文用均等显示滤波频时分析方法分析了长周期瑞利面波资料,获得了路经中国大陆及邻区的238条混合路径的面波群速度频散,其周期范围为10.5-113s.用改进的分格反演方法从混合路径频散中提取出位于华北地区的12个4°×4°网格单元的纯路径频散并反演其地壳上地幔结构.所得结果表明,华北地区地壳上地幔结构横向变化显著;从东向西地壳逐渐变厚;位于华北东部的分格在地壳中20km深处普遍存在低速层,整个华北地区上地幔低速层埋藏较浅,一般为55-100km之间.各个网格上地幔低速层的速度不尽相同. 相似文献
5.
讨论了利用面波与布格重力异常联合反演三维地壳速度结构的新方法,并利用该方法联合反演获得山西断陷带地壳S波速度结构.通过建立速度与密度之间的经验关系,利用非线性迭代反演方法获得最终速度模型.结果显示,联合反演获得的速度模型可以同时提高对面波及重力数据的观测拟合程度,而面波单独反演得到的速度模型则无法很好的拟合重力观测数据.相比较,联合反演速度模型中的大同火山区中下地壳的低速异常幅值小于面波单独反演模型中低速异常体的幅值.联合反演速度模型结果揭示,吕梁山地区在中下地壳存在低速异常,并且和北部的大同火山区低速异常相连接,说明可能导致新生代以来大同火山区岩浆活动的上地幔构造活动(上地幔局部上涌,地幔柱)可能对山西断陷带的形成和构造活动起到了一定的控制作用,并且导致了吕梁山地区中下地壳的低速异常. 相似文献
6.
利用中美合作在青藏高原布设的11台 PASSCAL 宽频带数字地震仪记录到的瑞利面波资料,测得青藏高原内不同块体的瑞利面波相速度(周期为10——120s),并反演了不同路径的地壳上地幔 S 波速度结构,发现青藏高原 S 波速度结构的横向变化显著.亚东——安多裂谷带的面波频散与相邻的块体差异最大,温泉至日喀则路径的相速度比其它路径的相速度明显偏高.该路径的地壳平均速度为3.79km/s,比其它路径的地壳平均速度3.40——3.50km/s高得多.青藏高原内不同块体的地壳中均有低速层存在,但低速层的厚度和速度不尽相同.位于北部的松潘甘孜块体。其地壳较薄约为65km,Sn 速度为4.48km/s,而且在约120km 深处的上地幔中存在一厚度为60km,速度为4.15km/s 的上地幔低速层.其它路径的上地幔速度相近,均没有明显的上地幔低速层出现.羌塘块体与拉萨块体的瑞利波相速度和 S 波速度结构极为相似,上地幔顶部的速度较松潘甘孜块体略高.在青藏高原广大地区中,地壳的平均速度低,普遍存在地壳低速层;上地幔顶部的横波速度为4.50——4.65km/s,上地幔中或者没有低速层或者低速层埋藏较深. 相似文献
7.
利用云南数字地震台网的区域地震波形资料,对川滇地区的地壳上地幔速度结构进行了初步研究. 结果表明,川滇地区上地幔顶部P波速度较小,约78 km/s,P波速度在上地幔表现为较小的正速度梯度,S波在100～160 km深度范围内表现为弱低速层. 对于较短的观测路径,不同路径的平均P波和S波速度存在明显的横向变化. 与川滇菱形块体内部的速度结构不同,在块体边界附近可以观测到比较明显的上地壳低速层,我们认为它可能与块体边界的断裂带有关;川滇菱形块体内部存在的下地壳低速层,有利于块体向南滑动,而中上地壳没有明显低速结构,可能表明川滇菱形块体向南滑动的解耦深度至少在下地壳. 根据不同路径的反演结果,给出了云南中部地区地壳内部的平均速度结构. 相似文献
8.
收集了南北地震带区域地震台网中292个地震台站2008年1月至2011年3月期间的地震波形数据,由频时分析方法提取了Love波相速度频散曲线,经过反演得到了研究区内的Love波相速度分布.根据Love波纯路径频散,采用线性反演方法对0.25°×0.25°的网格点进行了一维S波速度结构反演,利用线性插值获取了南北地震带地区的三维S波速度结构.结果显示了松潘—甘孜地体和川滇菱形块体地区的下地壳具有明显的S波低速层分布,该异常分布特征支持解释青藏高原隆升及其地壳物质运移的下地壳流模型.在100至120km深度上,川滇菱形块体西北部呈现较强的S波高速异常,这可能是印度岩石圈板块沿喜马拉雅东构造结下插至该区域所致,该区域下地壳的低速软弱物质与上地幔的高速强硬物质形成了鲜明对比,暗示了地壳和上地幔可能具有不同的构造运动和变形方式,这为该区域的壳幔动力学解耦提供了条件. 相似文献
9.
采用波形反演方法对青藏高原地区震中距8°-38°范围内的宽频带炸波波形进行拟合,研究该地区上地幔平均速度结构以及上地幔纵、横波速度的横向不均匀性结果表明青藏高原地区的平均地壳厚度约为68km,上地幔盖层平均厚度约为30－40km,速度约为8.10km／s雅鲁藏布江附近地壳厚度最大,约80km,相应的上地幔Pn速度为8．15km／s左右,青藏高原中部地区的地壳平均厚度约68-70km．位于拉萨地块北部的羌塘地块S波速度相对较低,其地壳和上地慢的平均S波速度分别比拉萨地块低1％和2％以上34°N以北,90°E附近的区域存在明显的上地幔P波低速异常区,P波的平均速度小于7．8km／s据此结果及前人工作,推断印度板块的俯冲可能以雅鲁藏布江缝合带附近为界,青藏高原巨大的地壳厚度是由于欧亚板块碰撞造成地壳缩短与增厚引起. 相似文献
10.
收集了研究区域(68°-150°E,5°-55°N)内33个数字地震台站记录的面波资料,利用多重滤波技术提取了4000余条路径上的Love波群速度频散曲线. 将研究区域划分成1°×1°网格,采取Occam反演方法得到了7.3-184s共43个周期的Love波群速度分布图;然后对网格结点进行S波速度结构反演,得出研究区域内420km深度内的地壳上地幔三维速度结构. 并采用Checkerboard方法对分辨率进行检验,得到横向的分辨率约为3°-5°. 研究结果表明:中国大陆地壳上地幔结构的横向不均匀性非常明显,内部结构与地表特征的相关性可以达到0-150km深度. 大陆地区东西分带、南北分块,块体的边界反映比较清晰. 相似文献
11.
Surface waveform modeling has played an important role on many continental-scale studies of upper mantle ve-locity structure, but it was seldom applied to the Chinese mainland study. The present study firstly analyzed sur-face waveform fittings for eight wave paths crossing through four different regions of the Chinese mainland (east-ern, central, northern and western China), and then inverted for 1D path-averaged S-velocities for these paths. The inverted crustal and upper-mantle S-velocities showed obvious region-related features, which are well consistent with known geotectonic units and previous research results. These results indicate that surface waveform modeling is a reliable method to get crustal and upper-mantle velocity structure. Furthermore, this method has a prominent advantage in detecting upper-mantle structure compared with fundamental-mode surface-wave dispersion method. 相似文献
12.
IntroductionHistorically, surface waves provided much of our understanding of the lateral heterogeneity in the crust and the upper mantle, especially in oceans or desert areas. Traditional method utilizes the great circle theorem for surface waves. It assumed that surface wave propagates along the great circle connecting epicenter with station. Firstly, traditional surface wave analysis was carried out by using multi-frequency-filter dispersion analysis to acquire the group or phase velocity d… 相似文献
13.
14.
Suzan van der Lee 《Earth and Planetary Science Letters》2002,203(1):15-23
This paper presents a new three-dimensional (3-D) model, NA00, of the S-velocity of the upper mantle beneath North America. The model differs from its predecessor NA95 in that it exploits seismograms recorded by a recent dense, broadband array, MOMA, and from independent measurements of North American crustal thickness. Model NA00 is derived by fitting the waveforms of broadband seismic S and surface waves recorded by the MOMA array and inverting them together with the database of waveform fits used for NA95 and the crustal thickness estimates. It is demonstrated that including data from the dense, broadband MOMA array yields a resolving power beneath the array that is of unprecedented quality and relatively constant over a large depth range. This improved resolution provides a unique opportunity for quantifying the structure of the upper mantle in and below the lower, thick Precambrian lithosphere. The high-resolution seismic structure of the imaged high-velocity lithosphere is compared with the thermal structure (estimated from heat flow), compositional structure (estimated from xenoliths and electrical conductivity) and the elastic structure (estimated from gravity and topography). There is a remarkable agreement between the seismic, thermal, and compositional estimates. The seismic lithosphere is 180 km thick below Missouri and Illinois, 200 km thick below Indiana, Ohio and Pennsylvania, practically undefined below New York, and 80 km below Massachusetts and the Atlantic continental shelf. The thick lithosphere is underlain by a layer with lower S-velocities that could represent a relatively low-viscosity channel. However, the S-velocities in this layer are much higher than those of typical oceanic asthenosphere. 相似文献
15.
Alan R. Leeds 《Physics of the Earth and Planetary Interiors》1975,11(1):61-64
Rayleigh wave phase velocities were determined by the single-station method for ten paths in the western Pacific. The data show that even 100 m.y. after formation, the phase velocity and upper-mantle structure are still dependent upon age. Inversion of the data gave a model with a lithospheric thickness of 76 km at 100 m.y., increasing to 104 km at 150 m.y., measured from the base of the crust. 相似文献
16.
Using seismic data from regional earthquakes in Tibet recorded by the Hi-CLIMB experiment, Pn attributes are used to constrain the velocity gradient and attenuation structure of the Tibetan lithosphere under the Hi-CLIMB array. Numerical modeling is performed using the spectral-element method (SEM) for laterally varying upper-mantle velocity and attenuation, and the seismic attributes considered include the Pn travel-time, envelope amplitude, and pulse frequency. The results from the SEM modeling provide two alternative models for the upper-mantle beneath the Hi-CLIMB array in Tibet. The first model is derived from the 3D velocity model of Griffin et al. (Bull Seism Soc Am 101:1938–1947, 2011) with a constant upper-mantle velocity gradient, and laterally varying upper mantle attenuation. The second model has a laterally varying upper-mantle velocity gradient, and constant upper-mantle attenuation. In both cases, the Qiangtang terrane is distinguished from the Lhasa terrane by a change in Moho depth and upper-mantle velocities. The lower upper-mantle velocities, as well as higher Pn attenuation, suggest hotter temperatures beneath the Qiangtang terrane as compared to the Lhasa terrane. Although the fits to the Pn amplitude and pulse frequency data are comparable between the two models, the first model with the constant upper-mantle velocity gradient fits the travel times somewhat better in relation to the data errors. 相似文献
17.
Forough Keshvari Z. Hossein Shomali Mohammad Tatar Ayoub Kaviani 《Journal of Seismology》2011,15(2):329-339
Non-linear teleseismic S-phase tomography across the Zagros collision zone in southwestern Iran is used to determine a high-resolution
image of the upper-mantle structure. The inversion was done using 41 high-quality earthquakes recorded by 19 broad-band and
medium-band stations along a 620 km long profile across the collision zone. Smearing from strong crustal velocity anomalies
into the upper-mantle is suppressed by travel-time corrections calculated based on a 3-D crustal model for the study area.
Our results show that the relatively old and cold Arabian shield has a higher velocity (up to 6% faster, at depths between
70 and 300 km) than the younger lithosphere farther north in Central Iran. These two upper-mantle domains are separated by
a sharp near-vertical transition whose surface expression coinciding with the Main Zagros Thrust. 相似文献
18.
本文提出了一种初至纵波(P波)与瑞雷面波的交叉梯度联合反演策略.通过对初至P波进行全波形反演可以获得近地表P波速度结构;通过对仅含瑞雷面波信息的地震数据转换到频率-波数域进行加窗振幅波形反演(Windowed-Amplitude Waveform Inversion,w-AWI)可获得近地表横波(S波)速度结构.在二者反演的目标函数中均加入P波速度和S波速度的交叉梯度作为正则化约束项,使得在反演过程中P波速度和S波速度相互制约,相互约束,从而实现对地震初至P波与瑞雷面波的联合反演.数值模拟结果表明交叉梯度联合反演可以提高S波速度反演分辨率,而P波速度反演结果并没有得到提高.实际资料的反演结果表明,交叉梯度联合反演能够获得更加可信的近地表速度结构. 相似文献
19.
Fresnel zone inversion for lateral heterogeneities in the earth 总被引：2，自引：0，他引：2
Kiyoshi Yomogida 《Pure and Applied Geophysics》1992,138(3):391-406
We propose a different kind of seismic inversion from travel-time or waveform inversion for lateral heterogeneities in the earth: Fresnel zone inversion. Amplitude and phase delay of data in several frequency ranges are inverted for model space around ray paths with a width corresponding to the considered frequency so that primary effect of finiteness of wavelength be included. For vertically heterogeneous media, Fréchet derivatives for inversion are obtained very efficiently using the paraxial ray approximation, with nearly similar amounts of computation compared to travel-time inversion. As an example, Fréchet derivatives are computed for a teleseismic observation system for a three-dimensional structure in the lithosphere beneath an array of seismic stations. Even if the used frequency is around 2 Hz, the width of Fréchet derivatives cannot be neglected, particularly near the bottom of the lithosphere. Sensitivity of model parameters to observations is, moreover, different in our approach from conventional travel-time inversion: it is zero along ray paths but large slightly away from them. Some model calculations show that travel-time inversion, particularly with models divided into very fine meshes or blocks, might give misleading results. An example of inversion for a simple Camembert model, in the event that travel-time inversion gives no reliable results, shows how this technique works with much smaller data sets and computation than waveform inversions. 相似文献