“十五”期间山东数字地震台网的建设

“十五”期间．由山东省人民政府和中国地震局共同投资建设．山东遥测数字地震台网新建、改建、扩建为山东数字地震台网。建成后的台网与“九五”期间建设的观测系统比较,提高了整个台网的观测动态范围,扩大了台站的观测频带,丰富了记录的信息量;台站数量与密度的增加,使台网监测能力得到提高。本文介绍了山东数字地震台网的建设内容、台网布局、监测能力和功能。     

我国地震电磁监测卫星总体技术研究

地震孕育和发生过程会引起震中附近上空的电离层异常,通过空间观测手段对由地震引起的空间电磁异常现象进行观测有着地面观测手段难以企及的优势.本文对我国地震电磁监测试验卫星科学任务进行了分析,在此基础上,给出了卫星的总体方案设计,并对卫星的工作模式、轨道和卫星构型进行了详细的论证、设计与分析,提出了满足地震电磁观测要求的卫星总体技术方案.     

地震电离层探测技术及其应用研究进展

2017年即将发射的中国电磁监测试验卫星将填补地震电离层立体监测体系中不可或缺的空白区域,也将为天地一体化地震电磁对比校验及圈层耦合机理认识提供重要的科学支撑.针对近期地震电离层立体监测体系发展的需求,本文主要介绍了目前国内用于地震研究的地基及空基电离层探测技术,包括电离层垂测/斜测、甚低频(VLF)电波观测、舒曼谐振观测、GPS及空间卫星电磁等,并总结了各种探测技术在国内外地震应用研究中的进展; 最后结合不同探测手段的优势,探讨了地震电磁立体探测系统的构建,并就未来的多手段综合应用发展提出了建议.      

南黄海海底大地电磁测深试验研究

针对南黄海盆地深层地震地质条件差,地震波受屏蔽,能量严重衰减,在海洋反射地震资料中很难识别反映中-古生界的反射地震波组,不能满足南黄海盆地前第三系油气资源前景评价的需要等问题,于2006年5月,开展了南黄海海域海底大地电磁测深试验,在盆地内五莲斜坡和胶州凹陷区布设了3个海底大地电磁测深点,取得了可靠的海底观测数据.本文详细阐述了海底大地电磁测深与常规大地电磁测深在数据处理方法上的差别,论述了海洋电磁噪声对海底大地电磁场观测的影响,提出了海底大地电磁场实测资料“水平姿态”校正、“方位”校正和“海洋电磁噪声”校正的方法.通过对试验观测资料的处理和反演,并结合地质、物性资料进行综合分析,结果表明在南黄海盆地海底以下深部还存留有古生代地层,这对于南黄海前第三系含油气前景的评价具有重要意义.试验结果也证明了海底大地电磁测深技术在研究古生代残留盆地方面的问题可以发挥相当好的作用.     

2013年甘肃岷县漳县MS6.6地震震电磁信号和同震信号观测

2013年岷县漳县MS6.6地震发生时,位于距震中约286km外的固原地区的两个地点正在实施大地电磁测量,对这两个测点电磁仪器记录到的电磁场时间序列和邻近固原地震台站记录的地震波形进行了对比分析,并结合岷县漳县地震震源区的深部电性结构特征和震电场理论数值模拟研究等结果,探讨了震电磁信号的激发机理。结果表明：大地电磁仪器不仅记录到了该次地震的地震波传播过程中“地震波驱动同震电磁效应”产生的同震信号波形,而且记录到了地震破裂过程中所激发的震电磁信号波形;岷县漳县地震震源区和震中到观测点一线区域中下地壳存在的低阻层,构成了震电磁信号传播的“导电通道”;岷县漳县地震电磁震电磁信号早于地震P波38s左右到达,且持续了4s左右,如果能捕捉到震电磁信号并用于地震预警,将可以大大减少因地震导致的人员伤亡。     

大地电磁测深和电偶源频率电磁测深资料反演

在研究大地电磁响应函数频散关系的基础上,构制了一套滤波系数算法,以用于由一套视电阻率资料估算相应的阻抗相位.理论模型和实际大地电磁观测资料的数字试验表明,该法是行之有效的.由频散关系估算的相位值与观测的相位资料的比较,可用于检验观测资料是否满足频散关系.利用经频散关系校正的阻抗相位值,进行大地电磁阻抗的联合反演则可望获得更为可靠的结果.研究了观测频带相互衔接的电偶源频率电磁测深和大地电磁测深视电阻率的一维联合反演问题.对两个实测点两种电磁法的观测资料进行了联合反演试验,与钻井资料对比表明,所获得的电性分层参数是较为可信的.在补充了由频散关系获取的电偶源频率电磁相位资料后,对于两种电磁法的视电阻率————阻抗相位、阻抗实部视电阻率-阻抗虚部视电阻率进行了拟大地电磁反演,获得了相近的反演结果.      

“时分”式多通道数据采集器的附加相位移及其对大地电磁数据处理结果的影响

本文讨论了“时分”式多通道数据采集系统讨于相关信号同步采集时的“伪同步”现象及其所产生的附加相位移;同时以实测MT资料的数据处理结果验证了采集器的附加相位移对大地电磁数据处理结果的影响,得出了有意义的结论:(1)采集器的“伪同步”采集所引进的附加相位移对大地电磁测深结果中的阻抗相位曲线有显著影响。(2)附加相位移对大地电磁测深数据处理结果中视电阻率曲线的影响不明显。由于第(1)方面的原因,所以在大地电磁测深数据处理中必须对采集器“伪同步”采集所引进的附加相位移进行校正。本文给出了附加相位移的定量计算公式。     

基于DDS技术的电磁扰动 观测系统检查装置

电磁扰动方法作为捕捉地震短临异常的较好方法之一, 受到国内外地震学家的广泛重视. 在没有电磁事件时, 观测仪器记录到的是没有规则的背景电磁场, 无法确定观测系统运作是否正常. 本文按照《地震地电观测方法电磁扰动观测》(DB/T35-2009)标准要求, 研发了基于直接数字合成(DDS)技术的电磁扰动观测系统检查装置, 目前已成功应用到了观测台站. 台站每月定期启动检查装置, 确定电磁扰动观测系统日常工作是否正常; 在记录到一些异常事件后, 也可以及时启动检查装置, 为判别异常事件提供技术支持.      

地震电磁卫星交变电磁场的数据处理

地震电磁卫星的迅速发展也带来了一些相关的研究课题,本文根据地面地震电磁观测中成熟的监测手段和参数,来分析如何根据地震电磁卫星记录的电、磁场分量提取可能与地震电磁异常现象有关的信息.介绍了电磁场时间序列的幅值统计;电磁波谱尤其是自功率谱对噪音干扰敏感,介绍了自功率谱的计算方法;正交电磁场相关度的变化分析方法;空间电磁波平面特征指标求取;以及在简单平面波特征下,提出空间阻抗张量的计算方法.     

地震电磁前兆的观测

地震的电磁前兆现象越来越受到人们的关注,地震电磁观测技术也在不断地得到发展和改进,已经由被动的观测发展到主动的观测,由地面局部的观测扩展到空间卫星全球范围的观测。文中介绍当前国内外在地震电磁观测方面的研究进展和实例,展望了我国未来地震电磁观测技术的发展。     

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 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.     

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.     

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。     

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.     

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.     

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.     

Structure of the poleward wall of the trough and the inclination of the geomagnetic field above the EISCAT radar

A special high-resolution routine of the EISCAT radar has been used to investigate the structure and development of the poleward wall of a deep trough in electron density. The feature was tracked by the radar during a 7-hour period under very quiet geomagnetic conditions. The field-aligned nature of the structure enabled an estimate to be made of the inclination of the geomagnetic field above EISCAT that was in good agreement with the current model. Observations of narrow field-aligned enhancements in electron temperature demonstrated that the wall of this trough is a dynamic feature, reforming regularly as the electron density responds on a time scale of tens of minutes to energy input from soft-particle precipitation.