3-D multi-parameter type traveltime tomography in a spherical coordinate frame: comparison of double and triple class simultaneous inversions          下载免费PDF全文

Chaoying Bai  Jiayu Sun  Xingwang Li  Stewart Greenhalgh 《地震科学（英文版）》2018,31(2):62-74

It is now common practice to perform simultaneous traveltime inversion for the velocity field and the reflector geometry in reflection/refraction tomography, or the velocity field and the hypocenter locations in regional earthquake tomography, but seldom are all three classes of model parameters updated simultaneously. This is mainly due to the trade-off between the different types of model parameters and the lack of different seismic phases to constrain the model parameters. Using a spherical-coordinate ray tracing algorithm for first and later(primary reflected) arrival tracing algorithm in combination with a popular linearized inversion solver, it is possible to simultaneously recover the three classes of model parameters in regional or global tomographic studies. In this paper we incorporate the multistage irregular shortest-path ray tracing algorithm(in a spherical coordinate system) with a subspace inversion solver to formulate a simultaneous inversion algorithm for triple model parameters updating using direct and later arrival time information.Comparison tests for two sets of data(noise free and added noise) indicate that the new triple-class parameter inversion algorithm is capable of obtaining nearly the same results as the double-class parameter inversion scheme. Furthermore,the proposed multi-parameter type inversion method is not sensitive to a modest level of picking error in the traveltime data, and also performs well with a relatively large uncertainty in earthquake hypocentral locations. This shows it to be a feasible and promising approach in regional or global tomographic applications.  相似文献   

主反射面变形引起的天线指向误差修正方法          下载免费PDF全文

梅庚君  项斌斌  王娜  王兆军 《天文学报》2020,61(6):62

射电天线指向精度通常要求小于主波束宽度的1/10, 对于短厘米波段或毫米波段的大口径反射面天线, 指向精度要求高达几个角秒, 对于天线性能目标的实现是个巨大的挑战, 因此对于大口径高频段的反射面天线来说指向问题成为天线性能实现的重要关注焦点. 在众多影响天线指向精度的结构子系统因素中, 对主反射面变形因素的研究很少. 文章结合天线的结构特点建立了反射面空间坐标系统, 并基于变形后主面点的空间坐标值, 提出了3自由度下的非线性最小二乘吻合的方法去精准预测天线指向. 最后利用空间几何关系严格推导出了服务于天线指向误差修正的俯仰和方位的精确调整量, 从而构建了主面变形同指向误差之间的间接关系, 这对大型射电天线指向精度的提升具有一定的指导意义.  相似文献   

地震地层解释系统开发研究   总被引：7，自引：3，他引：4  

颜琰 《物探化探计算技术》2000,22(1):40-47

机会的出现,往往并没有立刻被注意到,特别是在不熟悉的地区进行新的勘探。如何抓住机会,迅速有效地工作并尽可能多的利用相关信息迅速得出结论,这里所介绍的地震地层解释技术(Stratimagic)为我们提供了快速有效的工作方法和手段。  相似文献   

Implications for focused fluid transport at the northern Cascadia accretionary prism from a correlation between BSR occurrence a d near-sea-floor reflectivity anomalies imaged in a multi-frequency seismic data set     

L. Zühlsdorff  V. Spieß  C. Hübscher  H. Villinger  A. Rosenberger 《International Journal of Earth Sciences》2000,88(4):655-667

 A high-resolution seismic survey was carried out at the accretionary prism on the continental slope off Vancouver Island, Canada. Two GI-Gun data sets with different source frequency ranges of 50–150 and 100–500 Hz were combined with 4 kHz narrow-beam echosounding data (Parasound). The data allow spatial correlation between a gas hydrate bottom simulating reflector (BSR) and distinct areas of high near-sea-floor reflectivity. An integrated interpretation of the multi-frequency data set provides insight into the regional distribution of tectonically induced fluid migration and gas hydrate formation in the vicinity of ODP Leg 146 Sites 889 and 890. The BSR at the base of the gas hydrate stability field is observed within accreted and deformed sediments, but appears to be absent within bedded slope basin deposits. It is suggested that these basin deposits inhibit vertical fluid flow and prevent the formation of a BSR, whereas the hydraulic conductivity of the accreted sediments is sufficiently high to allow for pervasive gas migration. An elevation of the BSR beneath the flanks of a topographic high is interpreted as an indicator for local upflow of warm fluids along permeable pathways within outcropping accreted sediments. Parasound data reveal discontinuous zones of high reflectivity at or directly beneath the sea floor, which may indicate local cementation of surface sediments. In combination with GI-Gun data, the occurrence of these reflective areas can be related to the location of slope sedimentary basins acting as hydraulic seals. It is proposed that the seals sometimes fail along faults extending beneath the BSR, leading to focused upflow of methane-bearing fluid and the formation of carbonate pavements at the sea floor. Received: 9 November 1998 / Accepted: 6 April 1999  相似文献   

Disparity between measured and BSR heat flow in the Xisha Trough of the South China Sea and its implications for the methane hydrate   总被引：3，自引：0，他引：3  

Lijuan He  Jiyang Wang  Xing Xu  Jinqiang Liang  Hongbin Wang  Guangxue Zhang 《Journal of Asian Earth Sciences》2009,34(6):771-780

We calculate the heat flow from the depth of bottom-simulating seismic reflectors (BSRs) on a seismic profile in the Xisha Trough of the South China Sea, and compare them with the probe heat flow measurements. The BSR heat flow turn out to be 32–80 mW/m², significantly lower than the measurements of 83–112 mW/m². Such big disparity cannot be ascribed only to the errors from parameters (parameter errors) that traditionally believed to influence the BSR heat flow. Besides the parameter errors, we discuss emphatically the errors coming from the theoretical assumption for the BSR heat flow determination (theoretical errors), which occur when the BSR depth does not coincide with the base of the methane hydrate stability zone (MHSZ). If BSR stays bellow the base of MHSZ, lying at the top of free gas zone, the derived heat flow would be underestimated. Compared with the parameter errors, the theoretical errors would be relatively larger in some geological settings. The disparity between measured and BSR heat flow in the Xisha Trough might be mainly due to the theoretical error. Based on the theoretical model, assuming that the BSR lying at the top of the free gas zone, the methane flux along the Xisha seismic profile is estimated, and the thickness of the methane hydrate occurrence zone is predicted.  相似文献   

Seismic data processing approaches for the study of gas hydrates in the east China sea     

Liu Huaishan  Zhou Zhengyun 《中国海洋大学学报(英文版)》2002,1(1):87-92

A comprehensive study of the data profiles, including the 2D seismic data, single channel seismic data, shallow sections, etc., reveals that gas hydrates occur in the East China Sea. A series of special techniques are used in the processing of seismic data, which include enhancing the accuracy of velocity analysis and resolution, estimating the wavelet, suppressing the multiple, preserving the relative amplitude, using the DMO and AVO techniques and some special techniques in dealing with the wave impedance. The existence of gas hydrates is reflected in the subbottom profiles in the appearance of BSRs, amplitude anomalies, velocity anomalies and AVO anomalies, etc. Hence the gas hydrates can be identified and predicted. It is pointed out that the East China Sea is a favorable area of the gas hydrates resource, and the Okinawa Trough is a target area of gas hydrates reservoir.  相似文献   

光学反射望远镜主、副镜安装调整不良引起的象差     

谭徽松 《天文研究与技术》2003,(3):56-61

一架先进的设计、精心加工的光学望远镜,在工厂或组装车间检查光学质量合格后,在观测地点安装调整后必须要经过检验。因为在安装调整中,如果光学部件(如主镜和副镜)的光轴有横向偏离、倾斜,或者相互间距有偏差,都会使星象质量变坏。以我台将要进口的2.4m反射望远镜为例,讨论了在主副镜的安装调整中若产生误差,给星象质量带来的影响,从而可作为检验和验收望远镜时的参考。  相似文献   

不依赖人工定标器的全极化SAR定标研究进展     

史磊  杨杰  李平湘  杨乐  赵伶俐 《遥感学报》2021,25(11):2211-2219

极化定标是极化合成孔径雷达应用的前提。传统极化定标方法以地面布设的人工定标器为参考,通过极化畸变模型对系统误差进行求解与标定。然而,人工定标器价格昂贵、数量稀少,每次定标任务都需根据传感器过境方向、雷达视角等信息进行设备调整;此外,现代雷达系统工作波位多、入射角调节范围大,不同视角获取影像的定标参数也不相同,这对地面定标设备的布设精度、调整的时效性提出了更高要求。为了及时、快速地完成极化定标,如何以自然界中的某些特殊地物作为人工定标器的替代品来完成定标具有重大的科学价值。本文综述了近年来国内、外提出的不依赖人工定标器的SAR极化定标研究进展（即自主定标）。首先阐述了极化定标的基本流程与极化质量评价体系;然后对近年来高精度自主定标相关研究进行了梳理,根据技术特点将其分为基于自然地物约束的自主极化定标、基于似角反射器的自主极化定标两类,对不同算法适用性进行了分析;最后对未来的研究方向进行了展望。  相似文献   

Five-hundred-meter Aperture Spherical Telescope project   总被引：2，自引：0，他引：2  

B. Peng  R. Nan  Y. Su  Y. Qiu  L. Zhu  W. Zhu 《Astrophysics and Space Science》2001,278(1-2):219-224

A Five hundred meter Aperture Spherical Telescope (FAST) is proposed to be built in the unique karst area of southwest China, and will act, in a sense, as a prototype for the Square Kilometer Array (SKA). It will be over twice as large as the Arecibo telescope coupled with much wider sky coverage. Some results from site surveys for such a SKA concept are briefly reported. Technically, FAST is not simply a copy of the existing Arecibo telescope but has rather a number of innovations. Firstly, the proposed main spherical reflector, by conforming to a paraboloid of revolution in real time through actuated active control, enables the realization of both wide bandwidth and full polarization capability while using standard feed design. Secondly, a feed support system which integrates optical, mechanical and electronic technologies will effectively reduce the cost of the support structure and control system. Pre-research on FAST has become a key project in the CAS. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

威特DI2002测距仪性能及其与ME－3000反射镜匹配研究     

巩守文  祝意青  任道胜 《大地测量与地球动力学》1995,(2)

本文通过对威特ＤＩ２００２测距仪性能的测试。发现影响测距精度的主要因素是ＧＲＴ１０－ＧＰＨ１Ａ的反射镜系统。威特ＤＩ２００２测距仪匹配ＭＥ－３０００反射镜后，需加两项改正，但观测精度显著提高，实测表明达到与ＭＥ－３０００测距仪相同的精度。  相似文献