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近地表沉积层的S速度结构是强地面震动模拟和地震灾害估计的重要参数,尤其是浅部的S波速度结构在工程上具有重要的应用意义．目前大部分资料来源于工程钻孔或工程地震探测,很少有地震波频率范围内的S波速度结构,或者深度达数百米的S波速度结构．通过对天然地震的井下摆波形记录的分析,提供了一种测量地震波频率范围深达数百米的S波速度的有效方法．收集了首都圈地区44个井下摆的近震记录,利用广义射线方法确认了直达S波及其在地表的反射波震相,并通过测量不同台站上两个震相的到时差,获得了首都圈地区浅层100——500m 深度范围的S波速度结构．研究发现,浅部100m 的平均S波速度低于300m/s．当深度增加到500m 时S波速增加到800m/s,平均速度梯度为0.8 （m/s）/m．研究结果表明,井下摆地震记录波形是研究沉积盆地浅层S波结构的重要资料,将为沉积盆地的强地面震动模拟提供重要基础参数． 相似文献
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文中收集了2009年1月—2019年1月青海、甘肃固定地震台网及野外流动观测台阵记录的青海共和及周边地区的P波和S波到时数据,应用双差层析成像方法反演了该地区地壳的三维速度结构和震源位置参数,分析了共和1990年4月26日MW6.4地震孕育发生的地质构造背景与该地区速度结构和地震活动性之间的关系。结果显示,共和地区的地壳速度结构呈现出明显的横向不均匀性,共和主震位于共和盆地正下方区域的低速异常体内,主震的SW侧为高速异常,该异常从地下向NE向上逆冲至近地表处,推测35.95°N处即为哇玉香卡-拉干隐伏断裂。共和主震发生在水平NE向构造应力作用下,由走向NWW、倾向SSW的隐伏断层的滑动造成。 相似文献
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本文收集了1986年11月10日北京顺义M_s4.2级地震(主震)前后河北区域台网记录到的小震波谱最大振幅资料,利用P、S最大振幅比及P波初动资料,根据Delta矩阵的分离形式,对波场基本传播项进行重新组合,计算出记录资料较好的小震机制解参数。结果表明,顺义地震震中区及其附近小震主压应力(P)轴分布比较集中,并且在“主震”前小震机制解一致性较好,主震之后较前者有一定的紊乱,这可能是识别主震的一个标志。 相似文献
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2008年汶川地震震源区横波分裂的变化特征 总被引：7，自引：0，他引：7
对2008年汶川地震序列的横波分裂的时空变化现象进行了研究．通过在横波窗内S波质点运动图的分析,从地震余震区附近台站的近场地震记录中提取了S波分裂的快波偏振方向和快慢波之间的时间延迟．龙门山断裂附近7个台站的S波分裂的结果显示了快波偏振方向的空间分布特征,断裂带东南侧（四川盆地一侧）台站的快波偏振方向总体为北东方向,而在断裂西北侧高原内部的PWU（平武台）则为近东西方向．观测到了快慢波之间到时差的趋势性变化,靠近余震带南端的L5501台的到时差在主震后持续减小,北端PWU台的到时差比主震前明显增大．横波分裂现象主要由台站下方岩层中随应力场方向排列的微裂隙控制,结果显示了主震和余震过程中区域应力场的变化,汶川地震余震活动带南部的应力在主震和余震中得到了释放,地壳应力场在余震带北部集中,导致了PWU台在主震后介质各向异性强度的增强． 相似文献
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《地震学报》2010,(2)
近地表沉积层的S速度结构是强地面震动模拟和地震灾害估计的重要参数,尤其是浅部的S波速度结构在工程上具有重要的应用意义.目前大部分资料来源于工程钻孔或工程地震探测,很少有地震波频率范围内的S波速度结构,或者深度达数百米的S波速度结构.通过对天然地震的井下摆波形记录的分析,提供了一种测量地震波频率范围深达数百米的S波速度的有效方法.收集了首都圈地区44个井下摆的近震记录,利用广义射线方法确认了直达S波及其在地表的反射波震相,并通过测量不同台站上两个震相的到时差,获得了首都圈地区浅层100—500m深度范围的S波速度结构.研究发现,浅部100m的平均S波速度低于300m/s.当深度增加到500m时S波速增加到800m/s,平均速度梯度为0.8(m/s)/m.研究结果表明,井下摆地震记录波形是研究沉积盆地浅层S波结构的重要资料,将为沉积盆地的强地面震动模拟提供重要基础参数. 相似文献
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利用2015年1月至2021年5月28日期间我国云南省漾濞县及周边地区固定台站和漾濞地震后布设的流动台站所记录到的近震资料,使用双差层析成像方法获得了该地震震区的高分辨率地壳三维速度结构和震源位置。重定位结果显示,漾濞M6.4地震序列主要沿NW?SE向展布,与维西—乔后—巍山断裂走向一致,地震主要集中在4—10 km的深度范围,呈约80°高倾角分布。结合定位结果与三维速度结构显示:漾濞M6.4地震序列的空间分布与速度结构变化具有相关性,主震位于P波、S波高低速异常交界处,这种介质物性变化的交界地带可能有利于中强地震的孕育和发生,余震主要分布在低P波速度、高S波速度和低波速比的脆性区域;沿漾濞地震序列的分布走向,主震两侧呈现完全不同的速度结构,其西北部具有明显的高P波速度、低S波速度特征,该地区高密度、强韧性的地层可能是阻挡漾濞地震的NW向破裂而呈单向破裂特征的原因。 相似文献
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汶川M_S8.0地震:川西流动地震台阵观测数据的初步分析 总被引：20，自引：1，他引：19
2006年10月,中国地震局地质研究所地震动力学国家重点实验室,在中国四川西部(100°~105°E,26;N)布设了由297个宽频带地震台组成的密集流动地震观测台阵。截至2008年6月,川西台阵已记录远震事件(mb>5.0,30;)690个。5.12汶川MS8.0地震的发生为检验川西台阵观测系统的观测能力和工作状况提供了机会。文中对5.12汶川地震及其强余震序列观测记录进行了初步分析。结果表明:1)已发布的5.12汶川地震及其强余震参数有必要进一步修正,它们的震中位置可能存在8~24km误差,主震震源深度为19km的估计可能更接近实际情况;2)2008年5月16日理县(MS5.9)地震的波场分析表明:该地震面波不发育,它不可能是一个浅源地震,地震动速度波场垂直及水平分量峰值的异常增大与断层密切有关,在不考虑地形地貌、土质条件等因素的情况下,震中距200~250km范围内的地震动速度峰值异常增大可达正常衰减的4倍以上;3)利用接收函数方法对四川盆地和松潘-甘孜地块地壳结构的初步分析表明:四川成都北侧地壳厚度达到46km,四川盆地地壳从西向东逐渐增厚,下地壳显示了较为坚硬的特征,松潘-甘孜地 相似文献
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《地球物理学进展》2017,(4)
基于中蒙国际科技合作项目中获取的宽频带地震阵观测资料,利用提取到的周期为10~80 s的每个网格点瑞雷波相速度频散,反演得到了蒙古中南部下方地壳以及上地幔S波速度结构.结果表明:25 km深度处S波速度分布特征受地表构造形态控制,北部杭爱-肯特山脉为明显高速异常(约3.75~3.82 km/s),中南部戈壁沙漠为低速异常(约3.55~3.65 km/s);42 km深度处S波速度受地壳厚度影响,具有西北到东南逐渐增大的趋势,杭爱-肯特山盆下地壳相对较高的S波速(约4.1 km/s)是由盆地形成过程中拉伸作用导致盆地下地壳厚度减薄造成的;60~100 km深度范围内S波速度呈现南北高中部低的形态,分析认为中部戈壁低速异常与该地区新生代火山活动有关,而火山活动范围纵向上由中西部向中东部逐渐变深,横向由中东部向中西部逐渐变宽;此外,中东部地区地壳的隆起可能是由于火山活动引起的地幔热流上涌造成的. 相似文献
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D. M. Pechersky A. A. Lyubushin Z. V. Sharonova 《Izvestiya Physics of the Solid Earth》2010,46(7):613-623
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
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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
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Prof. Dr. W. A. Heiskanen 《Pure and Applied Geophysics》1958,41(1):1-18
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
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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
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V. E. Pavlov T. Yu. Tolmacheva R. V. Veselovskiy A. V. Latyshev A. M. Fetisova I. V. Bigun 《Izvestiya Physics of the Solid Earth》2017,53(5):702-713
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
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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
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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
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Geomagnetism and Aeronomy - The evolution of the magnetic configuration in the solar corona is studied. The curvature of the K-corona helmets obtained from an analytical approximation of the... 相似文献