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1.
根据Schaff和Richards[1]对“重复地震”的定义,利用波形相关识别出首都圈地区2002~2006年发生的“重复地震事件”.对宽频带/甚宽带和短周期记录,分别采用0.5~5.0 Hz、1.0~5.0 Hz带通滤波,识别出859例“重复地震”事件,占总数约24%.假定“重复地震对”间的距离小于1 km,地震台网测得的两个地震之间的距离系台网定位误差所致,而相应的震相走时差为人工拾取误差,给出了首都圈数字地震台网的定位精度估计.结果显示观测条件较好的首都圈东北部地区平均定位精度约为5 km;西南部地区约为13 km,是观测条件有待改善地区.  相似文献   

2.
孟真  宋晓东 《地震》2019,39(3):166-177
利用国家测震台网数据备份中心时间跨度超过7年的连续波形资料, 设定至少三个台站记录的垂直分量波形互相关系数大于0.8的地震对为一组重复地震, 通过波形互相关分析, 识别出龙门山断裂带周缘波形相关意义上的“重复地震”2790次, 构成2907组重复地震。 沿用Schaff和Richards的研究结果, 假定“重复地震”间距很小(小于1 km), 地震目录记录的重复地震对位置之差主要为地震台网的定位误差所致, 基于此误差给出了龙门山断裂带周缘地震台网的定位精度估计: 台网的水平定位精度较高, 水平定位误差约为2.8 km(2倍标准差), 且西南段台网的水平定位精度优于中北段; 垂直定位精度较差, 垂直定位误差约为10 km(2倍标准差), 现有地震定位方法对震源深度的测定有待改善。  相似文献   

3.
利用辽宁区域地震台网记录分析重复地震   总被引:10,自引:3,他引:7       下载免费PDF全文
将Schaff和Richards所选的通过远震波形相关得到的分布在辽宁地区的23对ldquo;重复地震rdquo;,利用辽宁区域地震台网记录的波形资料进行相关计算,得到辽宁区域台网波形相关意义上的ldquo;重复地震rdquo;,并与Schaff和Richards的结果进行了对比分析. 利用辽宁区域台网得到的ldquo;重复地震rdquo;对辽宁区域地震台网的震相拾取和地震定位进行了评估. 结果表明,远震波形相关意义上的ldquo;重复地震rdquo;与区域台网波形相关意义上的ldquo;重复地震rdquo;有一定差别,它们只有部分交集. 但是,从总体上评估辽宁区域台网的定位能力和震相拾取误差,用两种方法得到的ldquo;重复地震rdquo;所给出的评估结果无实质差别——尽管用区域台网得到的ldquo;重复地震rdquo;似乎效果更好. 基于ldquo;重复地震rdquo;之间在理论上距离应小于1 km的工作假定,可以得到辽宁区域台网地震目录中的定位误差在5 km之内,平均为2 km;Pg震相的拾取误差94%在plusmn;1 s之间,Sg震相的拾取误差88%在plusmn;1 s之间.   相似文献   

4.
乌鲁木齐遥测地震台网和新疆地震台网的地震定位与分析   总被引:1,自引:0,他引:1  
利用新疆地震台网和乌鲁木齐遥测地震台网在乌鲁木齐地区100km范围内1993年6月至1993年12月10日各自定位的地震资料,以新疆地震台网为参考基准,将乌鲁木齐遥测地震台网的资料与其进行了对比。对比发现遥测地震台网比新疆地震台网在地震数量上多32.9%,在定位精度上也相对要高一些。另外,根据地震定位的三种交切结果,分析了遥测台网地震定位现状。  相似文献   

5.
利用重庆数字地震台网2010年1月至2017年12月的地震波形资料和观测报告,选出5个研究区1 251个M_L≥1.5地震进行波形互相关计算,识别出358对同时被2个地震台站记录且各台波形互相关系数(cc)不小于0.8的重复地震对,涉及342个地震事件,约占地震总数的27%。将筛选出的重复地震对用于定量判断地震目录中震相拾取误差及评估台网定位精度,结果显示:重庆数字地震台网的垂直定位误差约为3 km,水平定位误差约为5 km,Pg、Sg震相拾取误差分别为0.5 s和0.7 s;其中武隆区地震定位和震相拾取精度最高,綦江区最低。  相似文献   

6.
应用广东数字遥测地震台网数据,通过对广东省周边50 km以外的62次地震重新定位,对比研究广东数字遥测地震台网数据处理软件提供的几种地震定位程序,初步认为:中国东南部、西北部地区及国外距广东地区较近的位于中国东南方向的印尼、日本等地区的地震,3种定位方法均可对其进行定位;而分布在国外较远地区的地震,用Hyposat及locSAT定位程序尚可,且locSAT优于Hyposat定位程序,而单纯型定位程序几乎不能用。  相似文献   

7.
提高地震定位精度方法的研究   总被引:1,自引:0,他引:1  
本文对地震定位产生误差的原因进行分析,并且对提高地震定位精度的方法进行了研究。随着沈阳数字化地震台网即将投入运行,需要将原有的DOS环境下运行,用BASIC语言编写的地震定位软件,移植到新的系统运行环境,并且在吸收原定位系统的优点的基础上作了重大改进,进一步提高了网缘地震定位精度和可靠性,对提高地震台网监测能力有重大的意义。  相似文献   

8.
人工爆破检验区域地震台网地震定位精度   总被引:1,自引:1,他引:0  
利用广东地震台网记录的2015年6月珠江口海陆联合地震构造探测项目人工爆破资料,采用MSDP地震分析软件提供的3种常用地震定位方法,对6次人工爆破事件进行分析,将定位结果与已知爆破位置进行对比,验证地震定位精度。结果表明,当地震定位数据满足台网分布方位均匀度ΔU≤0.35、次空隙角(S_(gap))≤160°时,广东地区地震震中定位精度优于3 km。  相似文献   

9.
利用非线性定位方法NLLoc,对新疆精河地区2017年8月9日至9月30日期间M≥3.0级的22个地震进行重新定位,并与中国地震台网中心正式目录结果进行对比,讨论了NLLoc方法在速度模型复杂的新疆地区定位的可行性.研究结果表明,NLLoc方法重定位新疆精河地震事件中,在发震时刻、震中方面误差较小,满足定位精度要求,但深度值上相差较大.NLLoc方法定位结果相对较为集中,主要分布于14~21 km,与CAP反演的深度分布为12-21 km,平均深度17 km,主震的震源深度21 km结果相符合,且与新疆地区的平均震源深度21±10 km和北天山地震带的平均震源深度19 km的结论相符.结果显示:NLLoc方法可用于地壳速度结构变化大、分布复杂地区的新疆地震定位,且有助于更好地解决震源深度测定问题,提高地震定位精度.  相似文献   

10.
对1995年加利福尼亚里奇克雷斯特地震序列,使用伯克利数字地震台网(BDSN)的宽带,大动态范围仪器记录的数据进行了地震定位和震源参数估计。本文的目的是研究稀疏宽带合网对网外区域的监测能力,它也适合于全面禁止核试验条约(CTBT)监测小震级地震事件的情况,另外,我们还介绍一个震例研究,这是其他区域宽带台网检测能力的代表。为了评估稀疏台网的检测能力,我们把根据BDSN震相测量所估计的地震位置与“直实位置”目录中由南加州地震台网(SCSN)记录数据得出的高质量地震位置做了比较。为了确定不同类型数据对绝对事件定位的重要性,使用了一个自适应网络搜索定位程度,它利用了一个或多个台站的多震相拾取的时间和方位角。我们使用了BDSN台站距离范围在250-500km和500-800km内的稀疏子台网,结果表明:在区域距离范围内,可能得到达到18km以内的绝对事件定位,这是CTBT所要求的,然而,在远区域距离范围内,较低的保噪水平不可能使事件的定位达到CTBT所要求的目标。  相似文献   

11.
The data on geomagnetic reversals are compared with the changes in the organic world and with the lower-mantle plumes. The times of the formation of plumes and the times of their appearance on the Earth’s surface relate to the intervals characterized by the different frequencies of geomagnetic reversals, i.e., there is no interrelation between the formation of plumes and the frequency of the changes in the geomagnetic field polarity. At the same time, a certain synchronism is observed between the frequency of the geomagnetic reversals and the boundaries of the biostratigraphic ages, i.e., the changes in the organic world in the long-period range. A hypothesis is proposed, which explains the change in the sign of the geomagnetic field by the combined effect of the irregular rotation of the internal core relative to the mantle and the changes in the slope angle of the axis of the Earth’s rotation, which, in turn, results in synchronous events on the Earth’s surface: the rates of changes in the organic world.  相似文献   

12.
Summary The author mentions the aims of the World-wide gravity project he established in the Ohio State University in Columbus, in 1950. He outlines the practical procedure of the gravimetric computations of the undulationsN and the vertical deflection components and and emphasizes that only by the global international cooperation and additional gravity observations at sea carried out during the last decade it has been possible to gather to Columbus the needed gravity material. Since there exist still large gravimetrically unsurveyed areas it is of vital significance to study what gravity anomalies are best to be used for these regions. The given figures concerning the accuracy of theN, and , estimated theoretically and obtained in practice, indicate that in the gravimetrically well surveyed parts of the world like in Europe and the United States we can get gravimetrically on basis of existing gravity material theN-values with accuracy of about 5–10 meters, and and with the accuracy of about 1. The geoid undulationsN are already computed in Columbus for more than 6000 points of the northern hemisphere. The sample maps show the interesting geoid of Europe and vicinity between the latitudes 60° and 30° and longitude 5° W and 30° E, drafted on basis of more than 1000N-values computed at the corners of 1°×1° squares. It is interesting to realize that the geoid undulations in all this area are positive, the extreme values being between 40 and 50 meters. The geophysical significance of the geoid maps of this kind is pointed out.  相似文献   

13.
Summary The maintenance of the axisymmetric component of the flow in the atmosphere is investigated by means of a steady-state, quasi-geostrophic formulation of the meteorological equations. It is shown that the meridional variations in the time-averaged axisymmetric variables can be expressed as the sum of three contributions, one being due to the eddy heat transport, another to the eddy momentum transport, and a third to the convective-radiative equilibrium temperature which enters the problem through the specification of a Newtonian form of diabatic heating. The contributions by the large scale eddies are evaluated through the use of observed values for the eddy heat and momentum transports.The contributions from each of the three forcing mechanisms to the temperature and zonal wind fields are invstigated individually and found to be of about equal importance. The sum of the three contributions are also presented for the temperature, the zonal wind, the stream function associated with the mean meridional circulation and the corresponding vertical motion. Although the results fail to reproduce the main observed features of the lower stratosphere, they are found to be in good agreement with observations in the middle latitude troposphere. At any pressure level, for example, the computed mean zonal wind has a jet-like profile and the axis of the jet is found to slope to the south with height, as observed in the atmosphere.Based in part on a thesis submitted by the first author as partial fulfillment of the requirements for the Ph.D. degree at the University of Michigan. — Publication No. 194 from the Department of Meteorology and Oceanography, The University of Michigan.  相似文献   

14.
15.
陈伯舫 《华南地震》2004,24(4):8-10
综合APIA、HONOLULU、PAMATAI 3个地磁台三分量的11年周期变化的形态后,可定性地提出该变化源于内场。如内源为核幔边界的电涡流,则其中心点应位于3台之间。  相似文献   

16.
Until recently, the existing data prevented the geophysicists from accurately dating the Bysy-Yuryakh stratum, which outcrops in the middle reach of the Kotuy River, constraining the time of its formation to a wide interval from the end of the Late Cambrian to the beginning of the Silurian. The obtained paleomagnetic data unambiguously correlate the Bysy-Yuryakh stratum to the Nyaian regional stage and constrain its formation, at least a considerable part of it, by the Tremadocian. This result perfectly agrees with the data on the Bysy-Yuryakh conodonts studied in this work and yields a spectacular example of the successful application of paleomagnetic studies in solving important tasks of stratigraphy and, correspondingly, petroleum geology. Within the Bysy-Yuryakh stratum, we revealed a large normal-polarity interval corresponding to the long (>1 Ma) period when the geomagnetic reversals were absent. This result, in combination with the data for the Tremadocian and Middle–Upper Cambrian sequences of the other regions, indicates that (1) the rate of occurrence of the geomagnetic reversals on the eve of the Ordovician Moyero superchron of reversed polarity was at most one reversal per Ma; (2) the superchron does not switch on instantaneously but is preceded by a certain gradual change in the operation conditions of the dynamo mechanism which, inter alia, manifests itself by the reduction of the frequency of geomagnetic reversals with the approach of the superchron. This finding supports the views according to which a process preparing the establishment of the superchrons takes place at the core–mantle boundary.  相似文献   

17.
The nutations of the planets Mars andEarth are investigated and compared. Alarge number of interior structureparameters are involved in the nutationcomputations. The comparison between the observations and the computationsprovides several constraints on these parmeters andtherefore allows a better understanding of the physics of the interior of theplanet. For the Earth, the high precision of the observations of the nutationshas led to a very good determination of interior properties of the planet. ForMars, observations of nutations are not yet available, and we review how theamplitude of the Martian nutations depends on the hypotheses consideredfor its interior. Although Mars is very similar to the Earth, its interior is not well known;for example, we don't knowif its core is liquid or solid. Only if the core is liquid,the Free Core Nutation (FCN) normal mode exists and can alter the nutationswhich are close to the resonance. From the observed geoids, it is known thatboth planets are not in hydrostatic equilibrium. The departure is larger forMars than for the Earth, and consequently, the implication of considering a convective mantle instead of a mantle in hydrostatic equilibrium described byClairaut's equation for the initial equilibrium state of the planet is largeron the Martian nutations than on the Earth nutations. The consequences of theuncertainty in the core dimensions are also examined and shown to be of a veryhigh influence for Mars if the core is liquid, due to the potential changes inthe FCN resonance. The influence of the presence of an inner core, which isknown to exist for the Earth, could be more important for Mars than for theEarth if the inner core is large. Due to the presence of Tharsis on Mars, thetriaxiality of this planet has, additionally, larger effects than on Earth.  相似文献   

18.
19.
The global database on the paleointensity, containing determinations of the virtual dipole moment (VDM) for a stable (normal) regime of the geomagnetic field in a time interval of up to 3.5 Ga, is supplemented by new VDM determinations and analyzed. The field generation process started no later than 3–3.5 Ga (earlier data are absent) at the stage of the Earth’s core formation. Since that time, the dipole value has differed from its present value by no more than an order of magnitude, and the deviations that have already been detected tend toward smaller values. The distribution of VDM values in the time interval 0–400 Ma is bimodal, which apparently reflects the presence of two different generation levels of the geomagnetic field distinguished by a relatively large value (close to the present field value) and a relatively small value (approximately half as large as the present value). The total duration of decreased VDM values appreciably exceeds that of increased VDM values (179.1 and 28.6 Myr, respectively). On the whole, data on the paleointensity do not contradict the hypothesis about the dipole nature of the field over the last 400 Myr; however, the number of determinations at high paleolatitudes is too small to draw decisive conclusions on the validity (or invalidity) of the dipole field approximation based solely on paleointensity data.  相似文献   

20.
A special high-resolution routine of the EISCAT radar has been used to investigate the structure and development of the poleward wall of a deep trough in electron density. The feature was tracked by the radar during a 7-hour period under very quiet geomagnetic conditions. The field-aligned nature of the structure enabled an estimate to be made of the inclination of the geomagnetic field above EISCAT that was in good agreement with the current model. Observations of narrow field-aligned enhancements in electron temperature demonstrated that the wall of this trough is a dynamic feature, reforming regularly as the electron density responds on a time scale of tens of minutes to energy input from soft-particle precipitation.  相似文献   

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