隧道爆破施工影响下地面既有高耸结构抗震性能分析

为研究地下隧道爆破施工影响下的气象塔高耸结构抗震性能的安全问题,建立隧道爆破施工地震动荷载的确定方法以及隧道施工爆破振动能量的计算方程,重点探讨了地下隧道爆破施工影响下的气象塔高耸结构的位移场分布与地震动力响应,对比分析了地下隧道爆破施工影响下气象塔不同位置的动力响应的差异。结果表明:爆破地震波属近源脉冲型破坏地震波,横波的破坏能力与其破坏能量及强度有关,高细型的气象塔结构质量和刚度突变的结构薄弱层处应力突变现象明显,顶部雷达受鞭梢效应的影响较大,爆破地震动对其动力响应的放大效应明显,严重降低了地面高耸结构的抗震性能。     

爆炸地震波作用下地下结构动力响应数值分析

爆炸地震波荷载类似于天然地震波荷载，但又不完全相同。基于有效应力动力分析法，运用二维显式有限差分程序FLAC对地下结构在竖向和水平爆炸地震波荷载作用下的动力响应进行数值分析。编制了周围土体介质分析模型的程序模块并与FLAC接口。考虑了水平和竖向爆炸地震波荷载对地下结构的耦合效应，得出了一些定性的结论。     

爆破地震波作用下尾矿坝的有限元动力分析

为了了解某钼矿进行爆破采矿是否会对近距离的尾矿坝产生破坏作用,结合实际勘探资料,在二维静力非线性有限元分析的基础上,进行爆破地震波作用下坝体的动力反应分析,综合研究了动位移、动应力和加速度时程等关键物理量变化的规律性,并在此基础上进一步结合试验资料对坝体进行了液化判断及稳定性分析。分析结果表明,该钼矿在规定的爆心距、药量范围内进行爆破采矿时,相邻的尾矿坝是安全稳定的。本文的研究结果对爆破设计、现场采矿及尾矿坝体运行维护均具有一定的指导意义。     

爆破地震作用下桩-土-结构相互作用的数值模拟

土-结构动力相互作用是地震工程和结构抗震的重要研究内容,但目前对爆破地震作用下土-结构动力相互作用的研究较少。运用大型有限元软件ANSYS/LS-DYNA,建立了桩-土-结构相互作用体系的三维有限元模型,由桩尖输入实测爆破地震波,取得了良好的计算效果。计算结果表明：考虑桩-土-结构相互作用后,群桩基础中每个桩的位移、加速度和剪应力幅值均呈桩顶大、桩尖小的倒三角分布,桩与承台的接合部比较容易受到损坏;桩-土-结构相互作用体系在爆破地震波冲击后,还会发生几次振动,但是这些振动产生的影响要小于爆破地震产生的影响,这与实测结果相符合;爆破地震波冲击下,群桩基础中,角桩顶部表面的桩土接触压力较大,但在爆破地震波冲击后,中心桩顶部表面的桩土接触压力较大,且具有一定的周期性,直至衰减为零。     

地震波诱发的深部地层动应力机制及断裂位移研究

借鉴弹性波动力学理论和爆破地震应力计算方法,结合地震波在岩层中的折射效应,以地震波加速度为基础数据,分析岩体在地震波作用下的受力。以汶川地震影响下的龙门山前陆盆地地下岩层的受力变形情况为例,通过计算分析和数值模拟,证实所用方法在求解分析地震波在各向同性岩石层间传播动力的可行性。同时验证汶川地震造成龙门山前陆盆地地下深部地层的断层破坏。      

碟形弹簧竖向减震体系的分析与研究

对碟形弹簧竖向减震体系利用时程分析方法对其进行动力分析，并输入不同场地、不同频谱的地震波考察其减震效果，验证了碟形弹簧在合理控制其刚度的前提下可以起到有效减小竖向地震的作用。     

叠层橡胶支座与柱串联体系动力失稳特性探讨

对叠层橡胶支座与地下室柱串联体系动力稳定性进行了研究。首先,采用动力稳定性理论对此串联体系受到谐波作用下的动力响应进行分析,并得到体系的主要动力失稳区间;其次,针对地震波是一种随机波形,通过快速傅立叶(FFT)算法变换进行频谱分析,将地震波分解为许多不同频率的谐波;分析了不同的静力及动力载荷系数下失稳区间的变化;数值算例分析了此串联体系在某一地震波下的动力稳定特性。分析的结果为此串联系统的工程设计与应用提供理论依据。     

高层框架结构远场长周期地震响应分析

首先对3条普通地震波和3条远场长周期地震波进行了频谱特性分析,并对比了普通地震波与远场长周期地震波傅里叶幅值谱的不同点;其次采用ABAQUS大型通用有限元软件建立了16层钢筋混凝土框架结构有限元分析模型,并对高层结构的动力特性进行分析。按照弹塑性时程分析的方法,研究高层框架结构在远场长周期地震动作用下的响应,包括楼层剪力、楼层位移和楼层位移角,并与普通地震动作用下的结构响应进行对比,得出远场长周期地震动对高层框架结构的各个响应均大于普通地震动。     

高层隔震建筑三维地震响应

对某高层框架－筒体结构进行了三维有限元时程分析，考虑了基础夹层橡胶了隔震垫的弹塑性特性和粘滞阻尼，分析了结构在地震波作用下的动力响应，为高层建筑中推广应用基础隔震技术提供了理论依据。     

不同时频特性近断层地震作用下的结构响应研究

研究不同时频特性的地震波作用下,抗震结构和隔震结构耦合设备的动力响应,对五层钢框架振动台模型试验数据进行小波分析。结果表明:主结构动力响应与地震波时频特性直接相关;由于主结构和隔震支座的滤波作用,设备的动力响应受地震波时频特性影响显著,但不具有直接相关性;隔震结构可以使设备的频率远离主结构的频率,从而降低设备的放大系数;设备耦合之后主体结构加速度的变化趋势取决于不同时频特性的地震波能量分布。      

琼中地震台重力仪记录同震响应特征分析

2013年2月6-8日圣克鲁斯群岛发生6次强震,琼中地震台的重力仪记录都有同震响应出现。本文从重力仪记录的面波的延迟时间、最大变形幅度、同震持续时间3个方面研究了6次强震的同震响应特征。     

On the Mechanism of the Secular Tidal Acceleration of the Solid Inner Core and the Viscosity of the Liquid Core

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 ³ Poise     

Comparison Between the Nutations of the Planet Mars and the Nutations of the Earth

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.     

Contribution to the knowledge of the magmatic evolution by the study of the variation of the coefficient of viscosity

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.     

Pictorial Series of the Manifestations of the Dynamics of the Earth

Studia Geophysica et Geodaetica -     

动水压力对深水桥墩地震响应影响的研究综述

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。     

Magnetic stratigraphy of the Ordovician in the lower reach of the Kotuy River: the age of the Bysy-Yuryakh stratum and the rate of geomagnetic reversals on the eve of the superchron

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.     

Evolution of the Source of the Active Region of the Sun

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...     

On the solution of the reverse problem of geodesics with the help of the chord

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).

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Dedicated to Professor František Fiala on His 85th Birthday

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Address: Veveři 95, Brno.