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安徽地区地震波衰减、场地响应及震源新参数的测定 总被引：5，自引：2，他引：5
根据安徽数字地震台网7个地震台的143条波形资料,研究了安徽地区的衰减模型和各台站的场地响应。采用三段几何衰减模型拟合,得到了安徽及邻近地区的几何衰减函数,得到安徽地区非弹性衰减Q值随频率f的关系为Q(f)=235.3×f0.616;7个台站的场地响应均无明显的放大效应,这与它们均处于岩石地基相符;并在本地区地震预测研究中尝试使用新参数,进行了初步的应用。 相似文献
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甘肃地区S波非弹性衰减Q值研究 总被引：3，自引：0，他引：3
文中利用新建"十五"数字化地震观测网络项目记录到的甘肃地区地震波形资料,研究了甘肃地区S波的非弹性衰减Q值,得到甘肃东南地区Q值与频率的关系为Q(f)=374.0f0.3084;祁连山中东段地区Q值与频率的关系为Q(f)=693.6f0.2865。从分区Q值研究结果看,各分区之间存在较大差异,显示出了Q值空间分布的非均匀性特征,这种区域差异性与甘肃地区构造活动、地震活动、地壳速度结构及热活动状态的区域差异性有较好的一致性,活动强烈、高热活动以及低速区为相对低Q值区,地震波衰减较快。 相似文献
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根据广东数字地震台网14个地震台的249条波形资料，研究了广东地区的衰减模型和各台站的场地响应. 采用三段几何衰减模型拟合，得到了广东地区的几何衰减函数. 同时也采用线性几何衰减模型和两段几何衰减模型对观测数据进行了拟合. 残差比较表明，线性几何衰减模型的残差最大，两段几何衰减模型的残差其次，而三段几何衰减模型的残差最小. 由此可以推论广东地区采用三段几何衰减模型具合理性和适用性. 得到广东地区非弹性衰减Q值随频率f的关系为Q(f)=481.5·f0.31；14个台站的场地响应均没有显示出明显的放大效应，这与它们均处于岩石地基相符. 相似文献
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宁夏地区Lg波衰减及场地响应特征 总被引：2，自引：2，他引：0
本文采用2008—2017年宁夏及邻区内15个数字地震台站记录的131次地震的波形资料，基于地震波衰减与场地响应联合反演方法，分析频率介于1—7 Hz之间的Lg波衰减及场地响应。采用2.2—3.6 km/s的速度窗截取了1 069条Lg波，计算得到Lg波各分量的地震波衰减品质因子Q（ f ）与频率f之间的关系。结果显示:Lg波垂直、东西及南北向各分量的Q0分别为237.1，201.8及245.9；Q（ f ）对f的依赖性指数分别为0.44，0.52及0.44，该结果与全球其它地震活跃地区的相应研究结果相一致。对Q（ f ）在时间域的分析结果表明，研究时段内该地区地壳介质的衰减属性并未改变，15个台站的最大场地响应幅值不大于6。 相似文献
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利用2009~2013年间新疆数字地震台网中12个地震台所记录的34个地震事件的数字地震波形资料,以南天山西段及交汇区作为研究区,采用3段几何衰减模型及Atkinson联合反演方法对地震波形资料进行非弹性衰减研究,得出介质品质因子Q(f)与频率的关系:Q(f)=337f0.577。为验证不同时段的地震事件对Q(f)计算结果是否有影响,将上述研究中2009年发生的前24个事件保持不变,对后10个事件做3次更换研究,分别得到介质品质因子Q(f)与频率的关系:Q(f)=329f0.565;Q(f)=324f0.520;Q(f)=363f0.526。结果表明不同时段内的地震事件对Q(f)值的影响不大,采用Atkinson联合反演方法计算介质品质因子Q(f)较为稳定、可靠。 相似文献
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《内陆地震》2016,(1)
利用新疆数字地震台网记录的15个台站的720条地震波形资料,用Atkinson方法联合反演得到南天山西段Q值随频率f的关系式为Q(f)=313.4f0.548;在400 km的震源距范围内,研究区地震波的几何衰减满足三段衰减模型;研究区的Q值小于天山中东段、北天山和柯坪地区的Q值,说明该区域构造活动强烈。其次根据S波衰减记录得到观测振幅谱,采用Moya遗传算法得到了新疆南天山西段15个台站的场地响应。结果显示,大多数台站的场地响应在1附近,西克尔台(XKR)、塔什库尔干台(TAG)、乌什台(WUS)和神木园台(SMY)的场地响应在1~4 Hz之间均大于2,表现出一定的放大效应,岳普湖台(YPH)呈现余弦波动,可能与台基岩性和仪器的工作状态有关。区域的选择对台站场地相应计算结果影响不大。 相似文献
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The determination of the coefficient of viscosity of eruptive products gives useful elements to the knowledge of possible variations of composition and physical conditions of the magmas. 相似文献
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As is known, the secular deceleration of the Earth's diurnal rotation is explained mainly by the tidal friction in the ocean. Below we consider this mechanism in some detail, taking into account also elastic deformations of the mantle under the action of ocean loading and the interaction between the tide-generating body, ocean tidal wave, liquid outer core, and solid inner core. It is shown that elastic displacements of the core-mantle boundary under the action of ocean loading are of about the same amplitude and phase as the elastic loading displacements of the Earth's outer surface. As a result, side by side with the mechanism of secular deceleration of diurnal rotation of the mantle, there are also (1) the opposite mechanism of secular acceleration of diurnal rotation of the outer liquid core and of the solid inner core and (2) the mechanism of excitation of differential rotation in the liquid core. Taking these effects into account, we compare theoretical and modern observed data on the eastward drift of the solid inner core. It is shown that the best agreement may be obtained if the turbulent viscosity of the liquid core is about 2 × 10
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Poise 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 magnetic evolution of the active region of the Sun at the level of the photosphere has been studied. Magnetic synoptic maps of the 2007 Kitt Peak Observatory were... 相似文献
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Studia Geophysica et Geodaetica - 相似文献
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地震激励下处于深水中的桥墩和周围水体的相互作用将对桥梁结构的动力响应产生较大影响。首先对地震作用下水-桥墩的相互作用理论做了概括,给出了动水压力对桥墩的作用效应及各自的适用范围;对主要的三种考虑流固耦合效应的分析方法做了对比,探讨了地震作用下影响水-结构相互作用的主要因素,并对今后的研究提出了建议。 相似文献
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Josef Vykutil 《Studia Geophysica et Geodaetica》1968,12(2):217-220
Резюме Дается вывод формул для вычислений длины хорды, длины и азимутов нормаляных сечений и длины геодезической линии эллипсоида.
Применяются тригонометрические функции данных величин и постоянные принятого ргфгргнц-эллипсоида, что является целесообразным
при использовании вычислителQjных машин, особенно автоматов. Рабочие формулы рекомендуются в форме (8–11).
Dedicated to Professor František Fiala on His 85th Birthday
Address: Veveři 95, Brno. 相似文献
Dedicated to Professor František Fiala on His 85th Birthday
Address: Veveři 95, Brno. 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