大跨度钢、木混合结构屋盖设计并基于实例分析对抗震性能的研究

为有效提高建筑中屋盖的抗震性能、节约建筑施工成本,深入研究大跨度钢、木混合结构屋盖的抗震性能。基于一个工程实例对该问题进行研究。分析从基本周期与抗侧刚度比、地震作用估算、承载力设置、抗震变形验算、连接与基础设计五个测试参数展开,在此基础上确定预应力拉索的地震响应及张拉控制应力。设计的混合屋盖是使用4道X形布置的屋面预应力主索与外柱斜拉索结构,这样是确保屋盖结构在地震下能够有效工作,根据该结构结合一工程实例展开大跨度钢、木混合结构屋盖抗震性能测试。实验结果表明,大跨度钢、木混合结构屋盖相对单一结构屋盖而言,抗震性能更强;同时实例分析表明,在多向地震输入下大跨度钢、木混合结构屋盖的各个构件中,内柱是抗震性能较弱的部位。     

大跨度空间网架结构屋盖隔震设计研究

针对大跨度空间网架屋盖隔震结构响应的问题,采用简化后的质点力学模型,对其进行理论研究,分析质量比、刚度比、阻尼比对屋盖隔震结构地震响应的影响,以基底剪力最小为原则确定隔震层的最优参数.建立相应的三维有限元模型,对其进行屋盖隔震设计,分别与非隔震和基础隔震结构的响应对比.结果 表明:屋盖隔震结构由于隔震层直接设置在屋盖支撑处,能明显减小上部网架的杆件轴力和支撑处的剪力.虽然其隔震层位置较高,但对结构的基底剪力和屋盖的挠跨比仍有减震效果;对于下部框架结构,直接与隔震层连接的框架的层间位移角有所减少,但未直接连接隔震层的较远部分框架的层间位移角略有增大,在结构设计时不容忽视,应适当加强.     

大跨维修机库结构采用耗能支撑的减震研究

大跨维修机库动力特性复杂,针对该类结构的减震研究则刚刚起步。本文结合大跨机库的地震响应特点,提出支撑柱顶与屋盖节点之间设置黏滞流体阻尼支撑的减震方案,对一大跨机库结构采用该减震方法进行了时程分析,对比减震前后结构基底剪力、柱顶侧移以及屋盖的杆件内力、位移。结果表明,该方法可以有效地吸收地震动输入能量,降低整体结构地震响应。由于机库结构特点决定了支撑柱间阻尼器的不均匀布置,导致减震效果在屋盖范围内的不均匀分布,分析结果表明屋盖杆件内力减震效果与杆件地震内力分布规律相吻合,表明该类减震方案对于大跨度维修机库屋盖地震响应具有非常好的针对性。     

双层球面网壳结构的阻尼替代杆件减振控制研究

采用阻尼杆件替代双层网壳结构中的部分下弦杆件,既不改变原结构的网格形式,又对其进行有效的减振控制。在ANSYS软件中建立粘弹性阻尼杆件的数值模型,采用阻尼杆件对网壳部分下弦杆件进行替换,建立网壳减振结构数值模型;分别采用8种阻尼杆件替换方式对结构进行控制,进行结构的三维地震作用分析,在三种常用II类场地地震作用下考察替换杆件布局对结构控制效果的影响。研究表明:阻尼杆件布局方式对结构动力响应的控制效果有较大影响,合理布置阻尼替换杆件可以有效降低结构最大节点位移、最大节点加速度、最大杆件轴力等响应,控制效果可以达到20%～30%。     

基于BP神经网络的网格结构损伤识别与试验研究

针对网格结构中杆件数量众多,但节点数总是远远小于杆件数的特点,损伤识别中采用了基于BP神经网络技术和面向节点的损伤初步定位方法的网格结构损伤识别的三步法。对双层柱面网壳结构模型在不同杆件去掉时的四种损伤情况下的振动特性进行了实测,并以实测低阶模态的频率变化率和少数测点的振型分量作为神经网络输入参数,对模型的各种损伤情况进行了识别。结果表明,所用的方法可以精简神经网络的结构,并提高其模式识别的能力。该方法可用于对大型复杂结构的损伤识别。     

"工字型"平面不规则钢结构的弹塑性时程分析研究

为了研究"工字型"平面不规则钢框架体系结构,分析房屋的抗震技术性能影响以及此种不规则建筑的薄弱位置,应用Abaqus有限元软件建立一个三维杆系模型对"工字型"平面不规则钢框架进行模拟.通过对钢框架结构在3种不同地震波作用下进行动力弹塑性时程分析,对产生的结构顶层位移、最大层间位移、层间位移角和底部剪力进行对比研究,以及对钢结构的薄弱环节进行了分析.最后从计算结果得出结论,"工字型"不规则钢架结构的抗震性能良好,主要控制指标符合规范要求.     

屋盖悬挑端加固减振试验研究

大跨网架屋盖挑檐部分风致响应较大,提出附加杆件、粘弹性阻尼器及粘滞阻尼器三种加固减振方法。设计制作正置四角锥体单元空间网架足尺子结构试验模型,基于带悬挑平屋盖风压分布风洞试验数据,对三种加固足尺子结构试验模型进行不同风向角下风荷载时程的加载。分析结构风致加速度与位移响应,结果表明:附加杆件加固后网架刚度增大,加速度响应增大,位移响应减小;附加粘弹性阻尼器,结构加速度与位移响应均降低;附加粘滞阻尼器,结构加速度响应减小,位移减小效果不明显。     

青岛邮轮母港客运中心钢屋盖复杂空间节点的有限元分析

青岛邮轮母港客运中心钢屋盖的多根异形变截面杆件通过焊接直接汇交于节点,杆件尺寸大,构造复杂,属于复杂空间节点。以初步设计的节点为研究对象,利用ABAQUS有限元软件对典型的复杂空间节点建立了有限元模型,并进行了静力分析,研究节点在最不利荷载工况作用下的受力性能及破坏机理。结果表明:在最不利荷载工况下,虽然杆件的应力保持在屈服强度内,但节点核心的最大应力超过了屈服强度。本设计通过增加核心区板件厚度30%解决了节点核心应力过大的问题,可为工程中此类节点的设计优化提供参考。     

竖向不规则框架结构连续性倒塌分析

国内外学者利用非线性静力方法进行结构倒塌分析时,研究对象主要集中在规则的结构形式,而针对大量出现的造型独特的竖向不规则建筑的倒塌研究还相对较少。本文基于拆除构件法,利用SAP2000结构有限元软件,对竖向不规则多层框架结构进行了基于非线性静力Pushdown方法的抗连续性倒塌研究。分别研究了拆除同一结构中不同部位构件、不同层数塔楼结构中相同部位构件后剩余结构的承载力变化情况,研究结果表明：拆除竖向承重柱后的剩余结构承载力,随着上部塔楼层数的增加以及拆柱位置的上升而出现不同程度的降低;加强裙楼顶部水平向承重构件,可以使塔楼底部构件破坏后的剩余结构更好地发挥悬链线机制,并防止剩余结构发生无明显征兆的连续性倒塌。     

集中塑性铰在网壳弹塑性地震响应中的应用

运用SAP2000分析设计软件和集中塑性铰理论,对现有振动台试验模型进行弹塑性时程模拟分析,通过试验与模拟分析对比,验证集中塑性铰理论在空间网格结构弹塑性地震响应分析中的适用性。分析中考虑几何和材料双重非线性影响,获得了节点位移响应、杆件塑性铰的分布特征、结构的整体变形及失效形态。振动台试验与模拟分析均表明:单层网壳试验模型在地震作用下的破坏始于支座附近及靠近肋杆的斜杆杆件端部,最终破坏是由网壳模型底部第一圈、第二圈结构杆件动力失稳破坏引起的,模型底部第一圈、第二圈大部分杆件经历了失稳或较大塑性变形,部分杆件达到极限强度与节点拉脱,使结构整体向下凹陷;采用集中塑性铰方法模拟杆系结构的动力弹塑性性能与振动台试验结果基本吻合,较适用于空间杆系结构地震下的弹塑性性能评定,且易被工程师掌握。     

On the synchronism in the events within the core and on the surface of the earth: the changes in the organic world and in the polarity of the geomagnetic field in the phanerozoic

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.     

On the maintenance of the axisymmetric part of the flow in the atmosphere

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.     

On the gravimetric undulations of the geoid and the deflections of the vertical

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.     

太平洋中部地磁台11年周期变化的研究

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。     

On the variation in the geomagnetic dipole over the geological history of the Earth

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.     

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.     

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.     

Evolutionary Changes in the Configuration of the Magnetic Field of the Solar Corona in the Epoch of the Minimum

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...