共查询到18条相似文献，搜索用时 275 毫秒
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利用中国数字台网（CDSN）记录的85个远震事件的宽频带P波波形数据和分离接收函数的最大或然性反褶方法,获得了CDSN台网10个台站不同方位的岩石层接收函数.利用这些台站不同方位的平均接收函数和非线性接收函数反演方法,获得了上述各台站下方100km深度范围内的岩石层S波速度结构.结果表明CDSN台网各台站下方的地壳厚度和岩石层速度结构存在明显的差别.其中,拉萨台下方的地壳厚度为66kin,壳幔界面较模糊,而余山台下方的地壳厚度为34km,壳慢界面两侧速度反差明显.刮用本文方法估计的地壳厚度与已有的结果基本一致,由于CDSN台网覆盖了中国大陆的各主要构造单元,本文的结果为研究中国大陆的岩石层S波速度结构及其横向变化提供了新的证据. 相似文献
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远震接收函数方法及其在海域岛礁区地壳结构研究中的应用 总被引：1，自引：0，他引：1
远震接收函数方法从远震P波波形中提取出台站下方主要速度间断面的信息,是研究地壳、上地幔结构的有效方法。该方法通过拟合转换波波形来约束间断面深度和横波速度。传统的接收函数线性反演方法强烈依赖于初始模型的选取,其反演结果存在较大的不确定性,为此新的基于非线性的反演方法逐渐发展起来,另外,接收函数与面波联合反演以及S波接收函数方法的提出也在一定程度上降低了反演结果的非唯一性。接收函数方法在大陆区地壳结构的研究中得到了广泛运用,但对于海区和岛礁区的研究却非常缺乏,本文回顾了国内外一些岛礁区的接收函数研究实例,介绍了西沙群岛琛航岛的天然地震观测及其结果,探讨了接收函数方法在岛礁区地壳结构研究中的应用前景。 相似文献
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收集整理2007年以来延边地震台记录的113个远震数字波形资料,采用远震接收函数反演延边地震台下方地壳结构,运用H-Kappa叠加方法,计算得到台站下方地壳厚度和泊松比.采用全球平均地壳模型作为初始模型,反演台站下方0-100 km的S波速结构.反演结果表明,延边地震台下方地壳厚度为30.8 km,波速比为1.84,泊松比较高,为0.29.在台站下方15-20 km及25-30 km处存在低速层. 相似文献
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利用小湾电站水库诱发地震台网之青华地震台记录到的93个远震地震事件,挑选其中效果较好的55个远震地震事件进行接收函数的计算,研究同一个台站下方地壳厚度随反方位角的变化情况。结果表明:①在青华地震台下方地壳平均厚度约为40.5 km;②不同方位的远震事件反映出台站下方不同方位的地壳厚度存在差异;③青华地震台下方地壳厚度存在由南向北逐渐增厚的特点,而东西向的横向变化不明显;④青华地震台反方位角在112°附近区域地壳厚度变化异常明显。 相似文献
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远震接收函数已广泛用于反演台站下方的结构,然而由于地球的非弹性衰减作用,远震数据较难获得高频接收函数,对浅地表结构约束不足.为了克服这一问题,我们使用近震数据的高频接收函数来研究浅表速度结构,并应用于四川理县西山村滑坡体上3个宽频带地震仪记录到的近震事件.本文发展了接收函数V_P-k(V_P/V_S)叠加方法,结合接收函数H-k叠加和波形反演方法获得了台站下方滑坡体的厚度、S波速度和平均V_P/V_S比,并与钻孔得到的滑坡体厚度进行对比.结果表明,滑坡体具有小尺度的横向不均匀性,台站下方滑坡体的平均V_P/V_S比在2.4~3.1之间变化并且在底层存在78~143m·s~(-1)左右的S波低速层.本文观测到的高V_P/V_S比和底层低的S波速度结构,与电磁法获得的滑坡体底层低的电阻率和底部富水特征一致,表明滑坡体h1底界面的抗剪强度相对较弱,是潜在的滑坡危险区域.本文研究结果表明,利用近震接收函数能有效约束浅表的速度结构,进而能为滑坡灾害治理提供一定的地震学参考. 相似文献
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接收函数方法及研究进展 总被引：8，自引：4，他引：8
远震P波波形数据中包含了大量在台站下方地壳上地幔速度间断面所产生的P-S转换波及其多次反射波的信息，是研究台站下方局部区域S速度分布理想的震相，由此产生的接收函数方法是反演台站下方S波速度结构的有效手段。接收函数方法可以通过波形反演拟合接收函数的径向分量，对观测台站下方地球介质的S波速度结构进行估计，也可以通过偏移叠加获得的接收函数道集（地震剖面图）追踪速度间断面。这种方法避免了对天然地震震源及其附近结构混响效应等复杂因素的影响，对S波速度的垂向分布敏感，垂向分辨率高。由于宽频带流动地震台阵的发展，用此方法还可获得研究区域速度结构的横向变化，横向分辨能力主要取决于台站的间距。本文回顾20年来接收函数研究的进展，探讨了方法研究的发展趋势，介绍了对地壳-上地幔结构的部分研究结果。 相似文献
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Mapping crustal S—wave velocity structure with SV—component receiver function method 总被引：1，自引：0，他引：1
In this article,we analyze the characters of SV-component receiver function of teleseismic body waves and its advantages in mapping the S-wave velocity structure of crust in detail.Similar to radial receiver function,SV-component receiver function can be obtained by directly deconvolving the P-component from the SV-component of teleseismic recordings.Our analyses indicate that the change of amplitude of SV-component receiver function against the change of epicentral distance is less than that of radial receiver function.Moreover,the waveform of SV-component receiver function is simpler than the radial receiver function and gives prominence to the PS converted phases that are the most sensitive to the shear wave velocity structure in the inversion.The synthetic tests show that the convergence of SV-component receiver function inversion is faster than tnat of the radial receiver function inversion.As an example,we investigate the S-wave velocity structure beneath HIA sta-tion by using the SV-component receiver function inversion method. 相似文献
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详细讨论了远震体波SV分量接收函数的特点及其在反演地壳S波速度结构中的优势．与径向接收函数类似，SV分量接收函数可通过对远震体波的SV分量直接反褶积P分量获得．研究分析表明:与径向接收函数相比，SV分量接收函数的振幅随震中距的变化更加稳定，波形简单且突出了对结构最敏感的PS转换波信息．理论数值实验显示:在反演地壳S波速度结构时，SV分量接收函数比径向接收函数具有更好的收敛性．作为实例，利用SV分量接收函数反演方法反演了海拉尔台下的S波速度结构． 相似文献
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Jens-Ove Nslund 《地球表面变化过程与地形》1997,22(5):441-455
On the high altitude polar plateau of Amundsenisen, western Dronning Maud Land, East Antarctica, a subglacial valley, with a broad horizontal valley floor interpreted as a sediment floodplain or valley delta, was studied by radio echo sounding. In addition, a small, probably glacial, valley was mapped within the same subglacial massif. Basal ice temperatures were calculated using field data on precipitation, air temperature and ice sheet thickness. Discoveries of old landforms which have been preserved more or less intact beneath the former Fennoscandian and Laurentide ice sheets have received increasing attention during the last decade. The aim of this study is to investigate whether preservation of landforms occurs under the East Antarctic Ice Sheet, and to discuss under that climatological and glaciological circumstances preservation may take place. The results show that the ice sheet covering the investigated localities is frozen to bed, and therefore has an insignificant erosional capability. The observations suggest that a large-scale subglacial sediment deposit and a small valley formed by glacial erosion have survived beneath a cold-based ice sheet marginal zone for a long time period. The process of glacial preservation, recognized for bedrock features and tentatively observed for sediment accumulations, should act on similar large-scale landforms under any cold-based ice sheet, present or past. On the basis of existing studies of the age and stability of the East Antarctic Ice Sheet, a Middle Pliocene age is suggested for the preserved landforms. The presence of the presumed sediment-filled valley further indicates that no prolonged periods of basal melting have occurred at the Amundsenisen study area during the ice sheet history, which includes the Quaternary glaciation periods. Finally, calculations of basal temperature for localities at different altitudes within the same subglacial massif were used to demonstrate local altitudinal control of glacial preservation. © 1997 by John Wiley & Sons, Ltd. 相似文献
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本文针对天然地震波形反演面临的困难及其复杂性，提出了逐步波形反演方法，第一步，运用波形反演中的试错法，求得地震台站下方成层介质的初步结构；第地一步，以第一步结果为初值，令各层厚度不变，反演速度；第三步，以第二步结果为初值，令速度不变，反演厚度。以上各步还可交替进行，直至得到满意结果。 相似文献
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考虑到面波频散对介质S波速度、接收函数对界面深度的各自敏感性优势,综合利用面波和接收函数资料实现联合反演,求取滇西地区壳幔速度结构. 本文利用适配滤波频时分析技术处理覆盖滇西地区的长周期面波资料,获得105～1050s周期范围内的面波群速度频散,进而利用分格反演方法提取研究区内1°×1°网格纯路径频散;基于滇西地区宽频带三分量远震记录,经反褶积后得到台站下方的远震P波接收函数. 联立面波纯路径频散信息和接收函数资料建立系统方程,利用阻尼最小二乘法实现联合反演,从而获得滇西地区壳幔S波速度结构. 结果表明,滇西地区以红河断裂为界,东西两侧壳幔结构存在明显差异,断裂西侧约20km深度处存在一厚度为10km左右的低速层,而东侧并不明显;滇缅泰块体上的畹町、沧源一带属于上地幔低速区,而另一个地幔低速区则位于滇中块体上的康滇古隆起上,两处地幔低速区与大地高热流分布、强震活动具有较好的对应关系. 相似文献
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The crust and upper mantle discontinuity structure beneath Alaska inferred from receiver functions 总被引：1，自引：0，他引：1
Yinshuang Ai Dapeng Zhao Xing Gao Weiwei Xu 《Physics of the Earth and Planetary Interiors》2005,150(4):339-350
In this study, three receiver function stacking methods are used to study the detailed crust and upper mantle structure beneath south-central Alaska. We used teleseismic waveform data recorded by 36 stations in the Broadband Experiment Across the Alaska Range (BEAAR) and 4 permanent stations in Alaska. H − κ stacking method using P-to-S converted wave and its multiply reflected waves between the Earth's surface and the Moho discontinuity is adopted to estimate the crustal thickness (H) and average crustal VP/VS ratio (κ) in this region. The receiver function results for 24 stations show that the crustal thickness under Alaska ranges from 26.0 to 42.6 km with an average value of 33.8 km, and the VP/VS ratio varies from 1.66 to 1.94 with an average value of 1.81 which corresponds to an average Poisson's ratio of 0.277 with a range from 0.216 to 0.320. High Poisson's ratios under some stations are possibly caused by partial melting in the crust and the uppermost mantle. Common converted point (CCP) stacking results of receiver functions along three lines show clear Moho and slab images under this subduction zone. The depths of the slab from our CCP stacking images are consistent with those estimated from the Wadati–Benioff Zone (WBZ). In the area between two stations DH2 (147.8°W, 63.3°N) and DH3 (147.1°W, 63.0°N), a Moho depth offset of about 10 km is found by both the H − κ and CCP stacking techniques. Common depth point (CDP) stacking of receiver functions shows not only the 410-, 520- and 660-km discontinuities, but also significant variations (−30 to 15 km) in the transition zone thickness under the southwest and southeast parts of the study region. The transition zone becomes thinner by 20–30 km, indicating that the temperature there is 150–200 K higher than that of the normal mantle. 相似文献
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To determine the crustal structure in central Tibet, we used teleseismic waveform data recorded by 18 stations in the INDEPTH-Ⅲ seismic array across the central Tibet from the central Lhasa terrane to the central Qiangtang terrane. The S-wave velocity structures beneath stations are determined by inverting the stacked radial receiver function using the GA method. The first order features in the receiver function are modeled. Our results show that the Moho in Qiangtang is about 8 km shallower than that in Lhasa terrane along the INDEPTH-Ⅲ profile. It maybe suggests the northward subduction of the Lhasa mantle lid beneath the Qiangtang terrane is affected by the India-Asia collision. We conclude that there exist low velocity zone in the middle crust across the northern Lhasa and Qiangtang terrane, which can be related to the high temperature upper mantle beneath that. 相似文献