应用布格重力异常研究郯庐断裂构造

使用布格重力资料对郯庐断裂带的中段部分（沂沭断裂带）进行了研究. 结果表明， 郯庐断裂带莫霍面及地壳内界面均发生错断，断裂带两侧地壳各界面起伏平缓. 该结果与前人的郯庐断裂带是切穿地壳的深大断裂的认识相一致. 在郯庐断裂带两侧，地壳结构明显不同，西侧沉积层较薄，平均在5 km以下；东侧多数在6 km以上；在断裂带中央沉积物最薄，大约为3～4 km. 断裂带东侧莫霍面埋深浅，大约为33～34 km；西侧莫霍面埋深明显增加，达到36～38 km．反映了莫霍面深度在断裂带附近整体是向西增加的. 郯庐断裂带在重力场分布中则表现为一条宽度较大的线性布格重力异常梯度带.      

龙门山断裂带地壳密度结构

研究龙门山及邻区地壳密度结构对于认识该地区地震活动性具有重要意义.根据龙门山及邻区( 100°～105°E,28°～33°N)的布格重力异常资料,选取了跨越龙门山断裂带的6条重力测线,在深地震测深资料约束下,使用Geosoft软件分别反演出了龙门山地区地下的沉积层、康拉德界面和莫霍面的深度分布.研究结果表明:龙门山断裂带两侧的地壳结构明显不同,西面高原地区沉积层较薄,大部分为基岩出露;而东边盆地沉积层明显较厚,多在6km以上.莫霍面和康拉德面在两侧均相对平缓,康拉德面从东部的大约24km增加到青藏高原山区的35km左右;莫霍面深度从东部盆地的大约42km增加到西部青藏高原的67km左右.龙门山断裂带整体表现为一条近SN向的陡变重力梯度带,并在其地壳内各界面均发生错断,莫霍面和康拉德面错断距离分别达6 ～ 7km和3～ 5km.该区地壳的这种陡变和不均匀性是导致地震活动性强烈的主要原因之一.     

地震方法探测太行山山前断裂的活动特征(英文)

太行山山前断裂位于太行山脉与华北平原过渡地带,是华北及我国东部地区一条重要的构造带,有关该断裂带的活动性有以下观点:1)它属深大断裂带;2)它是活动断裂带和地震构造带;3)它不是地震构造带。。为研究和评价该断裂的活动性,利用最近获得的地震资料和钻探联合剖面研究了太行山山前断裂的深部构造背景和第四系以来的活动特征。钻探验证以及研究结果与表明:太行山山前断裂不是岩石圈深大断裂,该断裂在第四系仅错断了中更新世QP2早期,中更新世QP2晚期和晚更新世地层没有发生错断。由此得出,太行山山前断裂不是活动断裂,也不是岩石圈深大断裂。该研究结果为跨越太行山山前断裂的城市进行规划和建设提供了重要的地质和地球物理资料,对于首都圈地震危险性评价也具有十分重要的意义。     

中国南海地区重力剥离对莫霍面反演的影响分析

确定更为精细的中国南海地区莫霍面对认识该地区内部结构、形成机制及相关动力学问题具有重要意义.重力剥离的精度直接影响莫霍面反演结果的质量.本文将由XGM2019e解算的自由空气重力扰动进行地形水深、沉积层、固体地壳密度异常和岩石圈热膨胀重力剥离,提取出莫霍面重力扰动,结合线性回归法和地震资料估计反演参数,并采用直接迭代法反演南海莫霍面模型,最后利用地震资料对反演结果进行精度评定.研究结果表明：仅顾及地形水深重力剥离的莫霍面反演结果整体精度较高,为1.94 km;在沉积物较厚的陆坡盆地,忽略沉积层的影响可使莫霍面最大加深6.30 km,但在沉积物较薄的南海海盆,考虑沉积层重力剥离会降低反演精度;利用CRUST1.0进行固体地壳重力剥离会使反演结果的精度降低0.22 km,表明CRUST1.0在南海地区并不准确;热膨胀重力剥离对反演精度的影响不大,但若忽略该效应,可能会高估洋壳区的莫霍面深度．针对南海重力莫霍面研究,笔者建议:若无精细地壳资料,忽略固体地壳重力剥离;若主要关注南海海盆可忽略沉积层的影响,但应考虑热膨胀重力剥离;若研究区覆盖沉积盆地,则应考虑沉积层重力剥离,并仔细选取密度-深度...     

太行山东缘石家庄南部地壳结构及断裂活动性探测

采用深、浅地震反射和钻孔地质剖面相结合的方法,对太行山东缘石家庄南部的地壳结构和隐伏断裂的活动性进行了研究.深地震反射探测结果表明,该区地壳厚度33~38km,莫霍面从华北平原向太行山下倾伏.石家庄—晋县凹陷是受拆离断层控制的盆岭构造,太行山山前断裂为凹陷的西边界断裂,表现为上陡下缓的铲形断裂.石家庄—晋县凹陷中还发育北席断裂和栾城断裂,它们与太行山山前断裂一样受拆离断层的控制,未错断早更新世晚期以来沉积的地层不属于活动断裂.深地震反射剖面的中部还揭示了一个近垂直的穹窿状反射异常体,它可能起源于莫霍面,向上,穿过上、下地壳分界面,并延伸至上地壳.穹窿状反射异常体内部反射波视频率随深度增加而降低,在莫霍面附近的壳幔过渡带也出现明显的频率降低、界面扭曲和变形现象,推断它可能是上地幔岩浆上涌到地壳内部的侵入体.结合电磁测深结果可以发现,上地幔热物质的上涌和东、西向拉张可能是形成石家庄—晋县凹陷的动力学机制.探测结果为深入理解石家庄地区的深部地球动力学过程、华北克拉通破坏机制、深浅构造关系和地震构造提供了依据.     

大陆深俯冲带的地壳速度结构——东大别造山带深地震宽角反射/折射研究

在安徽大别山(东大别)进行的深地震宽角反射/折射探测获得6条二维地壳速度结构剖面. 结果显示，东大别造山带地壳为一高速穹隆构造，在其核部中、下地壳变质岩出露于地表，波速高达5.0km/s；在其翼部，上、中地壳发育速度约6.1km/s的壳内低速层(体). 莫霍面的起伏变化较大，中心部位深达41km左右，周边地区则抬升到32～34km. 在晓天—磨子潭断裂一线下方莫霍面垂向错断，断距约4km. 东大别造山带具有大陆深俯冲-碰撞造山带地壳结构的典型式样. 莫霍面错断与扬子陆块深俯冲有关，错断处表征扬子与华北陆块碰撞缝合的深部位置. 高速穹隆构造可能是两陆块碰撞挤压的产物，穹隆翼部上、中地壳发育的低速滑脱带(面)可能在碰撞期之后的地壳伸展、超高压变质岩从中地壳抬升出露于地表过程中起到重要作用.     

华北克拉通东部地壳和上地幔结构的接收函数研究

利用北京大学和早期中国科学院地质与地球物理研究所在华北克拉通东部地区布设的共34台宽频带地震仪记录的远震体波资料,获取P波接收函数和S波接收函数,再分别通过偏移成像和共转换点叠加(CCP)和倾斜叠加得到了华北克拉通东部横跨郯庐断裂带地区沿剖面的地壳和上地幔速度间断面分布.研究结果表明,鲁西隆起下方的莫霍面的深度要比华北盆地和青岛地区浅约5 km,形成类似屋顶状的莫霍面隆起.郯庐断裂带和聊考断裂带下方的莫霍面有明显的错断.岩石圈与软流圈的分界面(以下简称LAB)的深度从太行山山前的约100 km深度上升到鲁西隆起下方约60 km深,向东在青岛地区下方LAB深度进一步变浅.我们利用倾斜叠加计算台站下方波速比得到地壳内的泊松比变化,结果显示鲁西隆起泊松比值分布相对均匀,而青岛地区内泊松比变化剧烈,可能反应了该地区作为苏鲁大别超高压变质带的北缘经历了较为复杂的地质演化过程.     

川西高原重磁异常特征与构造背景分析

川西高原位于青藏高原东缘,是我国大陆地壳构造变形及地震活动最强烈的区域.利用最新重力、航磁资料,通过异常分析和反演计算,研究了该区鲜水河断裂、理塘断裂、金沙江断裂的重磁异常特征、莫霍面特征、居里面特征,分析得出了这些断裂的深部地质结构与构造背景.计算表明:川西高原莫霍面东南浅、西北深,地壳厚度在43~63km之间.居里面特征表现为条带状,深度在17~23km之间.其中,鲜水河断裂带对应莫霍面深度梯度带,居里面为高低起伏圈闭.理塘断裂带北段莫霍面局部隆坳相间,南段莫霍面逐渐抬升,居里面呈现由西向东加深的梯度带.金沙江断裂带,居里面形成局部抬升,深部可能存在高温地热异常源.综合分析认为,川西高原地壳结构主要特点为:增厚的下地壳,热-塑性变形的中地壳,脆性变形的上地壳.     

郯庐断裂带中南段的岩石圈精细结构

郯庐断裂带是中国东部规模最大的构造活动带,有着复杂的形成演化历史,对中国东部的区域构造、岩浆活动、矿产资源的形成和分布以及现代地震活动都有重要控制作用.2010年在郯庐断裂带中南段的江苏宿迁市附近,采用深地震反射探测方法对郯庐断裂带及其两侧地块的岩石圈结构进行了解剖.结果表明,该区莫霍面和岩石圈底界均向西倾,其中,地壳厚度约为31~36km,岩石圈厚度约为75~86km,且岩石圈厚度在郯庐断裂带下方出现突变.郯庐断裂带在剖面上表现为由多条主干断裂组成的花状构造,其内部发育有断陷盆地和挤压褶皱,具有伸展、挤压和走滑并存的构造形迹,暗示郯庐断裂带的形成和演化经历了多期复杂的构造活动.这一断裂带错断了近地表沉积层,向下切割莫霍面和岩石圈地幔,属岩石圈尺度的深大断裂构造系统.软流圈高温高压热物质沿断裂带的上涌、岩浆底侵或热侵蚀作用造成岩石圈出现拉张伸展和岩石圈减薄,并可能使岩石圈组构及其物质成分发生改变.本项研究结果不但可进一步加深对郯庐断裂带深、浅部结构的认识,而且还可为分析研究华北克拉通东部的深部过程和浅部构造响应提供资料约束.     

东海及其邻域壳－幔结构与展布特征

莫霍面是地壳和上地幔的分界面，是个重要的密度界面，东海莫霍面的展布特征，对于研究东海深部构造具有重要意义.利用最新重力异常数据反演莫霍面深度，结合前人的莫霍面深度结果，分析东海及其邻域的壳－幔结构与展布特征.从莫霍面深度图可见东海及其邻域莫霍面起伏变化很大，深度在12～34 km之间变化，东海及其邻域地壳厚度为6～34km，东海陆架地区地壳厚度变化与大陆地区相比并不明显，显著减薄开始于冲绳海槽地区，琉球岛弧处地壳厚度明显再度增加，莫霍面呈现两凹两凸形态，认为东海及其邻域地壳自西而东从陆壳－过渡壳－洋壳逐渐过渡的.     

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.     

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.     

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 use of the autocorrelation method for estimating the depth to the magnetic basement

The depth to the top of magnetic dykes can be estimated from total field aeromagnetic data using the relation between the depth to magnetic sources and the autocorrelation function of magnetic data. By using synthetic anomalies we show that in the ideal case, depth can be determined to an accuracy of 10% or better, when the anomaly sources are two-dimensional dykes. However, the estimated depths depend on the width of the dykes. The estimated depth is about 0.6 times the actual depth to the top of thin dykes, and around the true depth for thick dykes having width-to-depth ratio around 3. The depth is considerably overestimated for very thick dykes (e.g., contacts, which is a special case of the thick dyke). Thus, the autocorrelation method requires that the width-to-depth ratio of the dyke is estimated independently to correctly estimate the depths. Alternatively, it must be assumed that the width-to-depth ratio for the two-dimensional source body is between 1.5 and 4.     

固体潮的地震预测研究与地球动力学研究之分析比较

本文分析了现行固体潮地震研究中的历史影响,对比研究了固体潮地震预测研究和固体潮地球动力学研究二者在振动频率、振动源体积、传输距离与介质等方面的地球物理特点与本质区别,强调了固体潮地震预测研究中最根本的工作是建立地震预测的目标和基本概念.     

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     

Macrobenthic communities of the Pechora Sea: the past and the present on the threshhold of the prirazlomnoye oil-field exploitation

On data of bottom sampling, carried out by means of grab, trawl and underwater photography in August–September of 1993 in the area of the Pechora Sea, quantitative regularities of macrobenthos distribution are described for the ecological monitoring purposes. Maps of -biodiversity and biomass indices, bottom communities and trophic zones, singled out by dominant method, are presented. Assessment of structure changes of the investigated area bottom communities during the last 60–70 years is fulfilled. It is shown that the described communities on the whole are of natural undisturbed character and that the revealed changes are within the natural fluctuations in the abundance of benthic populations or may be interpreted in terms of methodical differences in the data analysis and generalization by different authors.     

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。     

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.     

中国大陆构造环境监测网络基准站多路径效应影响因素浅析

在数据完整率达到95%的基础上,为进一步确保中国大陆构造环境监测网络GNSS基准站观测数据质量,选取2010—2020年全国基准站观测数据,采用TEQC软件进行质量检验,分类整理其中多路径效应计算结果呈典型特征的台站,结合观测环境状态,对多路径效应存在的区域性特征进行分析,发现除接收机天线周围发生遮挡外,硬件更换、台站周围地势差等因素,均对多路径效应产生不同程度的影响,可为建站选址和观测环境监测工作提供参考。