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1.
The German Regional Seismic Network (GRSN) comprizes now 16 digital broadband stations equipped with Wieland-Streckeisen STS-2 seismometers, 24-bit dataloggers and a seismological data center at Erlangen. It covers the whole territory of Germany with station-spacings between 80 km to 240 km. The stations are sited in very different environments ranging from near shore at the Baltic Sea coast up to distances of about 700 km from the coast, both within cities and up to about 10 km away from any major settlement, industry or traffic roads. The underground varies from outcropping hard rocks in Hercynian mountain areas, sedimentary rocks in areas of Mesozoic platform cover to up to 1.5 km unconsolidated Quarternary and Tertiary subsoil. Accordingly, seismic background noise varies in a wide range between the upper and lower bounds of the new global noise model. The noise conditions at the GRSN have been investigated systematically by means of displacement power spectral analysis within the frequency range 10-2 5 for RUE and > 10 for BSEG have been confirmed for frequencies between about 0.6 Hz 3 Hz. Strong lateral velocity and impedance contrasts between the outcropping Triassic/Permian sedimentary rocks and the surrounding unconsolidated Quarternary/Tertiary sediments are shown to be the main cause for the strong noise reduction and signal-to-noise ratio improvement at RUE and can account for about 50% of the noise reduction at BSEG.  相似文献   

2.
The directional effect of shaped charge is a well-known feature used for a long time in military weapons, oil well guns, and steel industry. This charge was successfully applied as a seismic energy source by Petrobrás during the past three years under different surface and geological conditions. Preliminary amplitude measurements taken with fixed gain shallow refraction instruments showed a consistent difference between conventional and shaped charges. Lately, a similar difference has been noted in deep reflection energy recorded with digital binary gain instruments as well as in deep oil well velocity surveys. Direct comparisons along more than 50 km of multiple coverage field reflection shooting are in agreement with these results and have proved the practical advantage of this source as compared to conventional dynamite. This source has been used since 1971 in routine seismic operation in the Amazon jungle with 300 gram unit charges distributed in small and large shot arrays increasing substantially the coverage and halving the cost at a higher record quality. A large amount of production seismic field work has been carried out in several other areas attesting the successful application of the shaped charges.  相似文献   

3.
—?Two chemical calibration explosions, conducted at the former Semipalatinsk nuclear test site in 1998 with charges of 25 tons and 100 tons TNT, have been used for developing travel-time curves and generalized one-dimensional velocity models of the crust and upper mantle of the platform region of Kazakhstan. The explosions were recorded by a number of digital seismic stations, located in Kazakhstan at distances ranging from 0 to 720?km. The travel-time tables developed in this paper cover the phases P, Pn, Pg, S, Sn, Lg in a range of 0–740?km and the velocity models apply to the crust down to 44?km depth and to the mantle down to 120?km. A comparison of the compiled travel-time tables with existing travel-time tables of CSE and IASPEI91 is presented.  相似文献   

4.
云南地区地脉动噪声特征分析研究   总被引:2,自引:0,他引:2  
王伟涛  倪四道  王宝善 《地震》2011,31(4):58-67
对地震台站记录到的长时间背景噪声进行互相关可以得到台站间的格林函数, 进而可以对地下介质波速结构和波速变化进行研究。 对背景噪声来源方向和时空演化规律的分析, 是提高结果可靠性的重要基础。 本文利用分布在云南境内的43个宽频带固定台站2008—2010年的垂直分量记录, 计算了两两台站之间的互相关函数, 并用平均能量流的方法研究了云南地区5~10 s以及10~20 s两个频段内地脉动噪声能量的空间分布和时间演化。 研究结果表明, 云南地区5~10 s的地脉动噪声能量优势方向存在明显的季节性变化, 夏季优势能量方位角为180°~210°, 冬季则为70°~100°。 而10~20 s的地脉动噪声优势方向方位角较为稳定, 为180°~210°。 在这两个频段内噪声能量的强度都表现出了较强的季节性变化。 同时发现在5~10 s频段瑞利面波之前存在视速度接近30 km/s的前驱信号, 并对其可能来源进行了分析。  相似文献   

5.
索伦-西拉木伦缝合带中段及周边区域先后经历了古生代古亚洲洋闭合、中生代蒙古鄂霍茨克洋闭合和中新生代太平洋俯冲等构造复合叠加,导致该区深部构造异常复杂。本研究从该区近年来累积的宽频地震探测资料的地震面波和环境噪音互相关格林函数中提取瑞雷波群速度频散,并据此反演区域尺度的三维横波速度。结果发现:区域地壳厚度横向变化不大,松辽盆地和下辽河盆地地壳比大兴安岭薄,地壳厚度与地形吻合表明这些地区基本达到重力均衡状态;而辽东隆起和渤海湾盆地地壳厚度与地形高度呈反相关,表明这些地区可能仍处于构造改造过程中。在80 km深度之下,波速分布则呈现与索伦-西拉木伦缝合带走向近似平行的东西向展布。以索伦-西拉木伦缝合带为界,南北两侧横波速分布复杂程度明显不同且南侧的东西两部分复杂程度也不同。这些结果表明区域受太平洋俯冲体系冲破坏程度存在明显差异,同时索伦-西拉木伦缝合带以南可能仍有古亚洲洋板片残留。  相似文献   

6.
The paper presents the results of studies of the resonance structures of the background electromagnetic noise spectrum obtained in a series of experiments in the autumn of 2012 in Karelia. The experiments are unique because the background noise was detected at stations spaced by a distance much less than the doubled effective waveguide height (about 50 km) in a region close to the main ionospheric trough, the structure and position of which were determined based on radiotomographic data. It is shown that the dimensions of the ionospheric local region, which affects both the generation of spectral resonance structures in particular and the propagation of electromagnetic waves in the considered range in general, depend significantly on the variation of ionospheric parameters in regions with strong horizontal inhomogeneity.  相似文献   

7.
The dynamics of seismic noise before the catastrophic earthquake of March 11, 2011 in Japan is studied in a minute period range using the records of broadband IRIS stations. It is found that the dispersion of the noise and the number of asymmetric pulses recorded within 500 km from the epicenter of the earthquake have drastically increased 1.5 months before the event. This is the highest enhancement ever recorded by these stations during the same interval of the year for the past 15 years since the IRIS network started stably operating. No increase is revealed in the noise recorded beyond 1200 km from the epicenter. The pattern of decay in amplitudes of the anomalous noise with increasing distance from the epicenter to the corresponding stations likely indicates that the sources of the noise were located close to the source of the earthquake. The noise contains both regular and chaotic components.  相似文献   

8.
本文利用在龙门山断裂带周边布设的57个台站自2008年11月至2009年11月为期一年的垂直分量连续地震环境噪声数据,通过短周期地震环境噪声成像方法,获得了龙门山断裂带中北段地壳25km深度范围的S波精细速度结构.结果表明:(1)龙门山断裂带周边区域10km以上的速度结构与地表断裂的分布形态具有良好的一致性,速度结构控制了龙门山主要断层的深部延展特征;在15km及以下深度,S波速度结构呈现沿龙门山和沿岷山隆起走向的交叉构造格局,由此造成的速度结构差异可能影响了汶川地震的破裂过程;(2)速度结构随深度的分布特征为龙门山断裂带主要断层的深部延伸形态给出了良好的约束,结果进一步确认了龙门山断裂中段的高角度铲型断裂构造特征;(3)研究区的南端发现了龙门山断裂下方20km以下深度具有与松潘地块中地壳低速层相关的低速结构的迹象,这可能是汶川地震破裂带南段22km左右深度存在脆韧转换带的一个证据.研究结果显示出密集台阵和短周期环境噪声成像方法在地壳浅部精细结构和断层探测研究中具有巨大潜力.  相似文献   

9.
中国东北地区地壳上地幔三维S波速度结构   总被引:12,自引:9,他引:3       下载免费PDF全文
收集了中国东北地区159个固定地震台2011年1月至2012年6月和27个流动地震台2011年1月至2011年6月间的垂向连续记录,根据噪声成像方法得到研究区(105°E-135°E, 39°N-52°N)较短周期(8~30 s)的瑞雷波群速度和相速度频散资料,再结合该区已有的天然地震长周期瑞雷波(36~145 s)的群速度频散资料,我们反演得到了中国东北地区200 km以浅深度范围内的三维壳幔S波速度结构,并得到了该区的岩石圈厚度分布图.结果表明:研究区中、下地壳S波速度结构的横向分布,在重力梯度带两侧有很大的不同,以东地区显示为大范围的高速,以西地区则呈现为大面积的低速;松辽盆地下方岩石圈地幔表现为显著的高速,岩石圈地幔底界面深度可能在90~100 km,薄的岩石圈盖层暗示东北地区的岩石圈可能发生了减薄;郯庐大断裂下方呈现出大范围的比较显著的低速特征,断裂下方上地幔顶部可能有热物质活动.  相似文献   

10.
We collected continuous noise waveform data from January 2007 to February 2008 recorded by 190 broadband and 10 very broadband stations of the North China Seismic Array.The study region is divided into grid with interval 0.25°×0.25°,and group velocity distribution maps between 4 s and 30 s are obtained using ambient noise tomography method.The lateral resolution is estimated to be 20-50 km for most of the study area.We construct a 3-D S wave velocity model by inverting the pure path dispersion curve at each grid using a genetic algorithm with smoothing constraint.The crustal structure observed in the model includes sedimentary basins such as North China basin,Yanqing-Huailai basin and Datong basin.A well-defined low velocity zone is observed in the Beijing-Tianjin-Tangshan region in 22-30 km depth range,which may be related to the upwelling of hot mantle material.The high velocity zone near Datong,Shuozhou and Qingshuihe within the depth range of 1-23 km reveals stable characteristics of Ordos block.The Taihangshan front fault extends to 12 km depth at least.  相似文献   

11.
—?Microseismic monitoring systems are generally installed in areas of induced seismicity caused by human activity. Induced seismicity results from changes in the state of stress which may occur as a result of excavation within the rock mass in mining (i.e., rockbursts), and changes in hydrostatic pressures and rock temperatures (e.g., during fluid injection or extraction) in oil exploitation, dam construction or fluid disposal. Microseismic monitoring systems determine event locations and important source parameters such as attenuation, seismic moment, source radius, static stress drop, peak particle velocity and seismic energy. An essential part of the operation of a microseismic monitoring system is the reliable detection of microseismic events. In the absence of reliable, automated picking techniques, operators rely upon manual picking. This is time-consuming, costly and, in the presence of background noise, very prone to error. The techniques described in this paper not only permit the reliable identification of events in cluttered signal environments they have also enabled the authors to develop reliable automated event picking procedures. This opens the way to use microseismic monitoring as a cost-effective production/operations procedure. It has been the experience of the authors that in certain noisy environments, the seismic monitoring system may trigger on and subsequently acquire substantial quantities of erroneous data, due to the high energy content of the ambient noise. Digital filtering techniques need to be applied on the microseismic data so that the ambient noise is removed and event detection simplified. The monitoring of seismic acoustic emissions is a continuous, real-time process and it is desirable to implement digital filters which can also be designed in the time domain and in real-time such as the Kalman Filter. This paper presents a real-time Kalman Filter which removes the statistically describable background noise from the recorded seismic traces.  相似文献   

12.
本文利用热层-电离层-中间层能量和动力学卫星TIMED中宽带发射辐射计SABER观测的临边大气长波红外背景辐射数据来研究平流层增温效应,基于2012/2013年1—3月在20~100 km高度内的临边大气长波红外背景辐射数据,采用微扰方法,得到辐射扰动的时空分布.结果显示:大气长波红外背景辐射扰动数据能够更精细的展示平流层增温事件的发生,2013年平流层爆发性增温效应下最大辐射扰动幅度出现在40 km处可达160%,而利用温度扰动数据表征此事件的发生时最大温度扰动幅度出现在40 km处只有21%.针对2012年弱平流层增温效应,温度扰动幅度最大值出现在40 km处为16.4%,而辐射扰动幅度的最大值在40 km处可达91%.大气长波红外背景辐射的纬度分布体现出此事件发生于高纬度地区;其经度分布在20~50 km范围内呈现"w"形状;而50 km和80 km处大气长波红外背景辐射的极值区域范围随着事件的发生在高纬度地区都是先扩大随后缩小的过程.这表明高层大气临边红外辐射信号可用于研究平流层增温效应,尤其是对于温度弱起伏的小扰动事件.这对于掌握临近空间环境辐射形成机理及其变化特性亦具有重要意义.  相似文献   

13.
本文选取呼图壁气枪发射台周边流动台记录的2016年6月至2017年12月气枪震源信号和背景噪声信号,分别采用互相关时延检测法和移动窗互谱法研究2016年12月呼图壁6.2级地震前后波速变化特征,得到以下初步结果:呼图壁6.2级地震前后,距6.2级地震60 km的流动台记录的气枪震源信号未发现明显的波速变化,距6.2级地震27 km的固定台石梯子台在6.2级地震前出现了较为明显的波速变化异常,可能与信号传播路径不同有关;流动台记录到的背景噪声信号出现与呼图壁6.2级地震有关的波速异常变化;气枪主要利用体波信号,背景噪声主要利用面波信号,两者射线路径不同可能是导致不同波速变化特征的主要原因。  相似文献   

14.
2019年6月17日在四川长宁县(104.9°E、 28.34°N)发生6.0级地震。 本文以该地震为例, 基于中国地磁台网提供的地磁台站资料, 利用帕金森矢量方法, 计算出每个台站在不同频段的帕金森矢量方位角异常之后, 将同一频段的多个台站的异常进行叠加, 提取和分析该地震前震中周围地磁场变化特征。 结果显示, 震中周围多个台站短临地磁异常时空特征明显, 通过异常综合叠加分析可以较好地估计震中方位。 该研究结果可为今后短临地震预报提供一定参考价值。  相似文献   

15.
Stochastic models can generate profiles that resemble topography by taking uncorrelated, zero-average noise as input, introducing some correlation in the time series of noise, and integrating the resulting correlated noise. The output profile will depict a nonstationary, randomly rough surface. Two models have been chosen for comparison: a fractal model, in which the noise is correlated even at large distances, and an autoregressive model of order 1, in which the correlation of the noise decays rapidly. Both models have as an end-member a random walk, which is the integration of uncorrelated noise. The models have been fitted to profiles of submarine topography, and the sample autocorrelation, power spectrum and variogram have been compared to the theoretical predictions. The results suggest that a linear system approach is a viable method to model and classify sea-floor topography. The comparison does not show substantial disagreement of the data with either the autoregressive or the fractal model, although a fractal model seems to give a better fit. However, the amplitudes predicted by a nonstationary fractal model for long wavelengths (of the order of 1000 km) are unreasonably large. When viewed through a large window, ocean floor topography is likely to have an expected value determined by isostasy, and to be stationary. Nonstationary models are best applied to wavelengths of the order of 100 km or less.  相似文献   

16.
本文设计了一种高-低卫星跟踪卫星、低-低卫星跟踪卫星和卫星重力梯度测量相结合的新型重力测量卫星系统,其可在一定程度上发挥卫星重力梯度和低低卫星跟踪卫星两种测量模式各自的优势.基于重力卫星系统指标设计的半解析法,深入分析了不同重力测量卫星系统配置和不同观测量及其不同白噪声水平情况下,新型卫星重力测量模式反演重力场模型的能力.数值模拟分析结果表明:在观测值精度和星间距离相同的条件下,轨道高度是影响重力场反演精度的关键因素;随着星间距离的增大,高频重力场信号反演精度会先提高后降低,轨道高度在200~350 km之间时,星间距离在150~180 km之间时反演精度最优;星间距离变率和卫星重力梯度两类观测值仅在某些精度配置时可达到优势互补,如果某一类观测值精度很高,则另一类观测值在联合解算时贡献非常小或者没有贡献.在300 km轨道高度,若以GRACE和GOCE任务的设计指标1 μm·s-1/√Hz和5 mE/√Hz来配置新型重力测量卫星系统中星间距离变率和引力梯度观测值的精度,联合两类观测值解算200阶次模型大地水准面的精度比独立解算分别提高1.2倍和2.8倍.如果以实现100 km空间分辨率1~2 cm精度大地水准面为科学目标,考虑卫星在轨寿命,建议轨道高度选择300 km,星间距离变率和卫星重力梯度的精度分别为0.1 μm·s-1/√Hz和1 mE/√Hz.本文的研究成果可为中国研制自主的重力测量卫星系统提供参考依据.  相似文献   

17.
Marine renewable developments have raised concerns over impacts of underwater noise on marine species, particularly from pile-driving for wind turbines. Environmental assessments typically use generic sound propagation models, but empirical tests of these models are lacking. In 2006, two 5 MW wind turbines were installed off NE Scotland. The turbines were in deep (>40 m) water, 25 km from the Moray Firth Special Area of Conservation (SAC), potentially affecting a protected population of bottlenose dolphins. We measured pile-driving noise at distances of 0.1 (maximum broadband peak to peak sound level 205 dB re 1 μPa) to 80 km (no longer distinguishable above background noise). These sound levels were related to noise exposure criteria for marine mammals to assess possible effects. For bottlenose dolphins, auditory injury would only have occurred within 100 m of the pile-driving and behavioural disturbance, defined as modifications in behaviour, could have occurred up to 50 km away.  相似文献   

18.
南海西沙石岛地震台下的地壳结构研究   总被引:6,自引:5,他引:6       下载免费PDF全文
为加强海上天然地震观测和岩石圈结构研究,我们在南海西沙群岛建立了石岛流动地震台,进行了为期一年多的观测试验.观测结果表明,虽然岛礁区的地震数据受热带气旋影响期间背景噪声较大,但仍能记录到MW 6级以上的地震.本文对具有清晰P波波形的远震记录进行了接收函数处理和计算模拟,得到台站下简单的地壳结构模型,其莫霍面深度为28 km,上地壳顶部有一层2 km厚的低速层,横波速度只有23 km/s,向下逐渐过渡到横波速度为38 km/s的下地壳.与已有的研究结果比较,发现石岛台与琼中台的地壳结构模型是西沙海槽剖面的自然延伸,西沙地块的地壳结构属减薄型陆壳,可与华南地块的正常陆壳对比.  相似文献   

19.
For a low-level geomagnetic satellite survey, for which the motion of the satellite converts spatial variation into temporal variation, the limit on accuracy may well be background temporal fluctuations. The sources of the temporal fluctuations are current systems external to the Earth and include currents induced in the Earth due to these sources. The internal sources consist primarily of two components, the main geomagnetic field with sources in the Earth's core and a crustal geomagnetic field.Power spectra of the vertical geomagnetic field internal component that would be observed by a spacecraft in circular orbit at various altitudes, due to satellite motion through the spatially varying geomagnetic field, are compared to power spectra of the natural temporal fluctuations of the geomagnetic field vertical component (natural noise) and to the power spectrum for typical fluxgate magnetometer instrument noise. The natural noise is shown to be greater than this typical instrument noise over the entire frequency range for which useful measurements of the geomagnetic field may be made, for all geomagnetic latitudes and all times. Thus there would be little benefit in reducing the instrument noise below the typical value of 10?4 gamma2 Hz?1 plus a 1/f component of 10 milligamma rms decade?1.For a given satellite altitude, there is a maximum frequency above which the natural noise is greater than the power spectrum of the crustal geomagnetic field vertical component. Below this maximum frequency, the situation is reversed. This maximum frequency depends on geomagnetic latitude (and to a lesser extent on time of day and season of year), being lower in the auroral zone than at lower latitudes. The maximum frequency is also lower at higher satellite altitudes. The maximum frequency determines the spatial resolution obtainable on a magnetic field map. The spatial resolution (for impulses) obtainable at low latitudes for a 100-km satellite altitude (possibly achievable by tethering a small satellite at this altitude to a space vehicle at a higher altitude) is 60 km, while at the auroral zone the obtainable spatial resolution is 100 km. At the higher satellite altitude of 300 km the obtainable spatial resolution is 230 km at low latitudes and 530 km at the auroral zone. At 500-km satellite altitude, the obtainable spatial resolution is 500 km at low latitudes, while maps cannot be made at all for the auroral zone unless the data are selected for “quiet” days.For the lower satellite altitudes, greater spatial resolution can be obtained than at higher altitudes. Furthermore since the crustal geomagnetic field power spectrum is larger at lower altitudes, the relative error due to the natural noise is less than for higher altitudes.  相似文献   

20.
使用中尺度数值模式WRF-ARW,针对2010年6月发生在中国东北地区一例伴随对流层高空西风急流(位于~9 km高度)演变过程出现的平流层重力波活动特征开展了数值模拟. 事件发生期间,对流层区域环流处在一个东北冷涡系统的控制之下. 模拟结果再现了该东北冷涡的发展和维持过程,以及与之相伴的高空急流的特征. 模拟结果揭示出在急流区域上空的平流层中存在显著重力波活动现象. 分析结果显示,重力波活动与急流存在紧密联系,在水平方向上,重力波呈显著的二维结构,出现在急流出口区上部并逆背景流向西传播. 功率谱分析结果表明盛行波动具有~700 km水平尺度、9~12 h时间尺度以及4~5 km垂直波长. 由于急流的存在,造成其与平流层中下部之间存在显著的水平风速垂直切变,与切变相伴的耗散使得上传的重力波动量通量数值随着高度升高而递减. 同时,在18~20 km高度间出现的西风-东风转换带极大地抑制了波动在垂直方向的传播,形成显著动量通量沉积效应. 估算结果表明,在11~20 km高度之间,这种效应的整体作用相当于对该层背景流施加强度为0.86 m·s-1·day-1的动力阻曳.  相似文献   

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