地震台站观测资料的质量管理

提高台站观测工作效益，重点在于抓好台站观测资料的质量，台站观测质量的提高是一项复杂的系统工程。我们在观测台站工作中紧紧抓住三个环节：应用现代观测技术；依靠科学管理；加强精神文明建设。十年来在仪器设备陈旧，人员文化素质偏低和台站条件相对艰苦的情况下，不断提高观测资料质量，取得了长足的进步。     

太原基准地震台震相分析在数字地震观测中的应用

以太原基准地震台数字观测记录的地震波形为基础,对不同类型地震所出现的震相从到时、周期、先后次序等方面进行了对比分析,对台站一线的观测人员在震相的准确判别,提高地震定位精度方面,有实际的指导意义。     

河南洛阳地震台影区地震震相特征

以河南洛阳基准地震台数字观测记录的地震波形为基础,总结了震中距6°～20°的影区地震的震相特征,对台站一线观测人员在震相的准确判别及提高地震定位精度方面具有实际的指导意义。     

全国测震基本台站技术交流会在九江召开

1991年6月21日至25日在江西省九江市江西省地震局科技培训中心召开了全国测震基本台网技术交流会。近几年来,由于我国的地震形势和地震工作均发生了较大的变化,台站以及有关人员迫切需要了解上级精神与要求,特别是在1990年国家地震局科技监测司制定了全国地震监测系统调整优化方案之后、对全国测震基本台站进行了布局的调整与优化,对台网观测系统的仪器装备也开始进行技术改造,又下发了新的《地震台站观测规范》,这些情况,对台站的仪器观测、资料的分析处理与交换以及在台站的观测资料质量的评比内容和方法等方面都提出了新的要求和作了较大的改进。     

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。     

地震台站管理效益研究

从台站规划、建设和改造情况,管理体制、工作方式和运行模式,监测设施、观测设备和观测环境,观测质量与技术支撑,工作生活环境,人员结构共六个方面分析了天津市地震台站的工作现状,指出了其中存在的问题,并给出了对策与建议,为提高地震台站的管理效益进行了有益的探索。     

红山地磁台绝对观测室部分技术改造

为红山地磁台绝对观测仪器 DI 仪配备防尘防潮罩,为避免照明灯泡金属螺旋帽磁性对绝对观测数据造成影响,对灯泡进行人工改造。两项技术简单、实用,为产出高质量的数据提供保障,值得在全国基准地磁台站推广应用。     

地震台站管理效益研究

从台站规划、建设和改造情况,管理体制、工作方式和运行模式,监测设施、观测设备和观测环境,观测质量与技术支撑,工作生活环境,人员结构共六个方面分析了天津市地震台站的工作现状,指出了其中存在的问题,并给出了对策与建议,为提高地震台站的管理效益进行了有益的探索。     

关于数字地磁台站观测系统的发展与观测资料应用的一点思考

针对地球科学和国家建设对地磁观测与研究的需求，结合“九五”地磁台站观测技术数字化改造，对地磁台站观测系统的发展及数字观测资料的应用提出了一些见解。     

微信企业号在福建GNSS台网运维管理中的应用

福建省地震局GNSS连续观测台网中61个基准站多为无人值守台站,将微信企业号引入台站系统运维管理,实现对台站设备运行状态检测,并实时推送检测结果,及时进行故障排查,提升GNSS台网运行率;实现每日9时对前一日观测数据的完整性统计,并群发统计结果,提醒工作人员进行补数处理;实现台站故障类型统计,为各台站整顿及改善工作提供资料。实际运行结果表明,该系统运行可靠,有效提高了GNSS连续观测台网的工作效率,保证了各基准站的实时高效运行。     

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.