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1.
为配合汶川地震断裂带科学钻探工程(WFSD),中国地震局地球物理研究所在四川省绵竹市天池乡和灌县—安县断裂附近分别架设了15套微震仪器和17个短周期地震台.基于WFSD-3附近的微震、短周期和区域台网的固定台站记录的近震数据,通过横波窗内S波分裂计算,得到其上地壳各向异性参数,即快波偏振方向和慢波的时间延迟,并分析了研究区的上地壳各向异性特征.结果显示,研究区大部分区域的快波偏振方向为NE向,与龙门山断裂带走向一致,但在研究区微震台阵布设小区域内,快波偏振方向表现出东西分区特征,东部为NE向,西部为NW向.上地壳各向异性主要是受到岩层中随应力分布排列的微裂隙和岩石或矿物结构的影响,研究区内快波偏振方向主要表现为NE方向,与断裂走向一致,反映了研究区上地壳各向异性主要受控于结构控制的各向异性,局部区域的快波偏振方向为NW向,与区域最大主压应力方向一致,说明区域应力场对研究区上地壳各向异性也有影响.通过分析微震台阵的归一化时间延迟随时间的变化情况可以反映区域应力场的变化情况.微震台阵的慢S波时间延迟在2012、2013年较为离散,在2014年有收敛的趋势,反映了强震后区域应力场逐渐稳定的趋势. 相似文献
2.
基于汶川科钻4号井孔（WFSD-4）附近的较小尺度的南坝微震台阵以及较大尺度的川西流动台站和区域台网的固定台站记录到的近震波形资料,通过横波窗内的S波分裂计算,分析了龙门山断裂带北段南坝地区的上地壳介质各向异性特征,并对区域应力场及构造特征展开讨论.S波分裂计算的结果显示研究区快波偏振方向主要表现为NE-NEE向,与北川断裂的走向一致,也与区域主压应力方向一致.小尺度密集分布的南坝微震台阵的计算结果进一步显示,靠近北川断裂的台站,其快波偏振方向与断裂走向一致,而距北川断裂较远的西北部台站的快波偏振方向与断裂走向不一致,反映了上地壳各向异性特征与地表的活动断裂结构密切相关.从南坝微震台阵的归一化时间延迟随时间的变化情况可以发现,在一个震中位于台阵布设范围内的地震事件发生前后,时间延迟有明显的变化,表明时间延迟随时间变化较为敏感,地震的能量影响了介质的性质.对比龙门山断裂带中段的科钻3号井孔周边地区的S波分裂计算结果,归一化时间延迟与本文结果一致,表明龙门山断裂带中段和北段的上地壳介质各向异性强度基本相同. 相似文献
3.
基于青藏高原东北缘甘肃区域台网41个宽频带地震台站的远震记录资料,通过PKS、SKS和SKKS震相的剪切波分裂分析,获取了台站下方介质的各向异性分裂参数,得到该地区上地幔各向异性分布图像,并结合GPS速度场和地壳剪切波各向异性分析青藏高原东北缘各向异性形成机制及壳幔各向异性特征.分析结果认为,在阿尔金断裂带西侧,各向异性快波偏振呈NWW-SEE方向,与断裂带走向有一定夹角,与塔里木盆地向柴达木盆地俯冲方向一致,说明该地区上地幔物质变形主要受古构造运动的影响,属于"化石"各向异性.在祁连山-河西走廊构造区,XKS快波偏振呈NW-SE方向,一致性较好,与区域断层走向方向相同;由区域小震的地壳剪切波分裂分析得到的地壳剪切波快波偏振在该区域呈NE-SW方向,与相对于稳定欧亚大陆GPS运动速率一致,地壳和地幔快波偏振方向的差异表明壳幔变形可能有不同的形变机制.在陇中盆地及其周缘,由于处于活跃青藏地块与稳定鄂尔多斯地块之间的过渡带,相对于其他区域具有更加复杂的构造背景,地壳快波偏振和地幔快波偏振总体上呈NWW-SEE方向,说明壳幔变形机制可能相同;但不同台站结果之间存在一定离散性,推测是由于受局部构造特征差异性造成. 相似文献
4.
三江地区位于青藏高原东南缘,川滇菱形块体的西侧.受陆-陆板块碰撞作用的影响,构造活动强烈,地震活动频繁.为研究该区的应力环境、构造特征及二者间的关系,本文使用三江流动线性地震台阵SL-Array（2016-12—2017-05）和国家固定地震台网（2015-01—2017-12）记录到的地震波形资料,运用剪切波分裂分析技术研究三江地区上地壳各向异性研究.计算得到该区域快剪切波优势偏振方向为NNW向,与区域主压应力方向一致.结果显示各向异性特征有分区性,以维西—乔后断裂和小金河—丽江断裂为界,将线性台阵划分为A、B和C三个区域.A区快波优势偏振方向表现出与区域主压应力方向的一致性.B区局部构造复杂,快波优势偏振方向表现为近NS向.C区结果比较离散,无明显快波优势方向.自西向东,研究区域快波优势偏振方向表现为NNW至近NS向的变化趋势.计算得到研究区域慢剪切波时间延迟为2.8±1.7 ms·km-1,其中B区最大,A区最小,反映了该区地壳介质各向异性强度的不均匀分布,也揭示了区域构造复杂程度与地震各向异性强度的关系. 相似文献
5.
本文利用布设在云南腾冲地区的15个固定和流动地震台站记录的近震波形数据,采用剪切波分裂分析方法得到了593对高质量的各向异性分裂参数.结果显示,腾冲火山区地震台站下方的近震各向异性的慢波延迟时间为0.02~0.37 s,平均延迟时间0.2 s.结合已有接收函数地壳各向异性研究结果,推测研究区地壳各向异性的主要贡献源自中上地壳.研究区不同台站的快波偏振方向变化很大,似乎反映了构造和区域应力场的共同作用.其中腾冲火山断裂西侧多数台站的快波偏振方向呈近N-S向,而东部多数台站的快速偏振方向呈NE-SW向,与区域主压应力方向一致,暗示研究区中上地壳各向异性主要是受主压应力引起定向排列的裂隙所致.基于近震走时得到的研究区平均VP/VS为1.68,推测腾冲火山区地壳应力场的局部变化可能与上地壳中富含气体的中酸性岩浆膨胀活动有关.另一方面,在腾冲火山区外围个别台站(MIZ、MZT)观测到了快波偏振方向与主压应力、已知断层等构造走向不一致的现象,暗示其各向异性是构造或构造和区域应力场共同作用的结果. 相似文献
6.
利用中国地震科学台阵第一期(2011-01-2014-06)及部分中国地震科学台阵第二期(2013-02-2015-12)的流动地震台阵记录到的小震波形资料,运用剪切波分裂系统分析(SAM)方法,分析南北地震带的地壳各向异性,对剪切波分裂参数所反映的区域应力环境及构造特征,以及区域内主压应力方向与断裂分布的关系展开讨论.研究结果表明,南北地震带快剪切波偏振方向自北向南由NE向逐渐转变为NNW向,与南北地震带区域主压应力的方向变化具有一致性.区域内分布的大量NE及WNW或NW向断裂构造同样对快波偏振方向有比较大的影响,位于走滑断裂附近的台站,其快波方向与断裂走向大致平行,部分位于走滑断裂附近的台站其快波方向几乎垂直于断裂走向,而与构造应力场方向一致性较好.个别台站表现出复杂快波优势方向特征,反映出研究区内构造环境的复杂性.慢波时间延迟结果显示,南北地震带南段的平均时间延迟高于北段,反映了受印度板块和欧亚板块的碰撞挤压作用,南段地壳介质各向异性程度更大,构造变形更加剧烈.对比南北地震带上地幔各向异性特征,推测在川滇菱形块体内部可能存在复杂的壳幔耦合现象,地壳剪切波分裂除了反映区域应力特征,还可以揭示出区域构造信息. 相似文献
7.
南迦巴瓦地区位于喜马拉雅山脉构造结东端,地壳各向异性具有其特殊性和复杂性.本研究收集了布设在南迦巴瓦地区的流动地震台站和固定台站于2017—2019年记录的近震波形数据,利用剪切波分裂偏振分析方法得到了研究区内10个地震台站的剪切波分裂参数快波偏振方向和慢波延迟时间,分析了剪切波分裂参数在空间上和时间上的分布,探讨了南迦巴瓦地区上地壳地震各向异性特征,以及2017年11月18日米林MS6.9地震发生后地壳应力状态的变化.结果显示,南迦巴瓦地区快波偏振优势方向有两个,即北西向和北东向.位于米林断裂、嘉黎断裂、墨脱断裂和雅鲁藏布江断裂附近的台站,快波偏振方向基本平行于断裂走向.研究区域上地壳各向异性方向受区域应力场的控制,另外还受到断裂构造的影响.南迦巴瓦地区慢波延迟时间均值为4.13 ms·km-1.距离米林地震主震震中位置较近的L0230台站慢波延迟时间较大.本研究没有观测到快波偏振方向在时间上的规律性变化.L0230台站的慢波延迟时间在米林MS6.9地震之后表现出明显的降低,反映了大地震之后地壳应力的释放与调整. 相似文献
8.
天山造山带是一条由陆陆汇聚而形成的陆内造山带,经历了长期的构造演化,尤其是新生代以来的再次活化导致其复杂的构造特征.文章利用新疆区域数字地震台网(2009~2019年)记录到的波形资料,使用剪切波分裂系统分析法,获得研究区内33个台站的剪切波分裂参数,分析了天山构造带的上地壳各向异性特征.结果表明,天山构造带不同区域上地壳各向异性存在差异,快剪切波优势偏振方向可以反映区域构造应力的空间变化,慢剪切波时间延迟则表明了上地壳介质各向异性的强弱变化.北天山西段地区、塔里木盆地的西北角和帕米尔东北缘各台站的快波优势偏振方向基本与其所在地区的构造应力场特征相符,柯坪块体北部地区各台站的各向异性特征受到这一地区断裂构造的影响较大,表现为快波优势偏振方向与断裂走向较为一致,而与区域构造应力场特征不符;南天山东段与乌鲁木齐周边地区的各向异性则表现出同时受到应力和断裂影响的特征,部分台站的快剪切波偏振方向与区域应力场方向一致,部分台站的快波偏振方向与其附近的断裂走向一致的特点.上述天山构造带大部分地区快波偏振方向与其附近的构造应力场特征展现出很好的一致性,显示出明显的应力挤压现象,天山造山带相对于南北两侧的盆地相对较软,是地壳缩短变形的主要区域,受到印度板块与西伯利亚板块敛合作用的远程影响,塔里木地块向天山地壳与上地幔层间插入与俯冲消减.此外慢波时间延迟分区特征也较为明显,北天山和南天山地区的慢波时间延迟自东向西均呈现递增的趋势,这一结果与跨天山的南北向汇聚变形从东到西递增的特征呈现出较高的一致性.构造运动最为剧烈的帕米尔东北侧地区的慢波时间延迟平均值显著高于其他地区,显示出这个地区的各向异性显著强于天山构造带其他地区. 相似文献
9.
通过收集鄂尔多斯块体西缘固定地震台网2010年6月至2017年8月的近场地震资料,选择符合剪切波分裂分析的14个台站记录的共137个有效事件波形,得到了剪切波分裂参数,即快剪切波（简称快波）偏振方向和慢剪切波（简称慢波）时间延迟.结果表明,研究区的快波偏振方向和慢波时间延迟具有明显的分区特征,快波偏振方向主要与构造应力场方向或者断层走向大体一致.鄂尔多斯西缘紧邻块体边界的台站,快波偏振方向自北向南呈现NS、NNE、NE向的变化,与青藏高原东北缘主压应力方向变化基本一致.银川地堑东西两侧的快波偏振方向有差异,东侧区域主要受青藏高原NNE向挤压和黄河-灵武断裂共同影响,而西侧区域可能受到阿拉善块体与鄂尔多斯块体之间的NW方向的主张应力和阿拉善块体内部应力分布的影响;鄂尔多斯块体、阿拉善块体与青藏高原的交汇区快波优势偏振方向为NE向,与青藏高原东北缘主压应力方向一致;海原断裂带及以南区域快剪切波优势偏振方向为WNW向,与断裂走向基本一致,较好的说明了海原断裂带为活跃的活动断裂.构造与断裂分布都是控制快波偏振方向的主要因素,走滑断裂上的台站快波偏振方向与断裂走向一致,表明这些台站主要受到断裂的强烈影响;走滑断裂附近的个别台站快波偏振方向呈现与构造应力场一致的方向,表明几乎没有受到断裂的影响.鄂尔多斯、阿拉善与青藏高原的交汇区平均时间延迟高于其他地区,反映了青藏高原在NE向运动过程中,受到稳定的鄂尔多斯块体阻挡作用,导致了交汇区地壳介质各向异性程度增加.以海原断裂带到六盘山断裂带为界,其两侧区域的各向异性差异性明显,揭示了应力与介质特性的差异,暗示其邻近区域,特别在海原断裂带东端到六盘山断裂带与鄂尔多斯块体西缘交汇区域,可能有较高的强震危险背景.本研究还对该区域的地壳和上地幔的耦合问题进行了初步讨论. 相似文献
10.
本文使用中国地震局地壳应力研究所2010—2011年期间在云南地区布设21个宽频带野外流动地震台记录到的波形资料,经时间域迭代反褶积求取远震接收函数,并挑选高质量Pms （莫霍面转换）震相,利用切向能量最小化方法获得283对高信噪比的径向和切向对应的Pms分裂参数,从而得到云南地区各台下方地壳各向异性. 结果显示,研究区内慢波时间延迟量在0.125 s和0.40 s之间变化,平均为0.25 s,且各向异性强弱与构造分布有一定相关性. 在扬子地台和保山地块表现为相对较强的各向异性,而思茅地块相对弱些,说明这些块体受下地壳流的影响作用各不相同. 从各向异性快波方向分布来看,在扬子地台和思茅地块除红河断裂带和澜沧江断裂带走向变化明显地区（如YNL04和YNL12台）外,各向异性方向均与断裂带走向近似平行,说明研究区内大型断裂带控制着下地壳流的构造变形. 腾冲地区的各向异性与其他三个块体均不相同,在该块体内部各向异性快波方向近似呈现出以火山为中心发散状分布,可能说明腾冲火山下方地幔热物质上涌到达下地壳后受上地壳的阻挡作用向四周发散的原因. 相似文献
11.
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
12.
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
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
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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
16.
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 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
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.
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