影区地震的识别与定位

通过分析西安地震台近几年各个方向记录到的影区地震,详细阐述 Lg1、Lg2波的确认方法,运用 Matlab对数据进行分析,给出S波与 Lg1、Lg2波的走时关系式,提高影区地震的分析速度和准确度,为单台大震速报和日常分析提供借鉴经验。     

影区地震的识别与定位

通过分析西安地震台近几年各个方向记录到的影区地震,详细阐述Lg1、Lg2波的确认方法,运用Matlab对数据进行分析,给出S波与Lg1、Lg2波的走时关系式,提高影区地震的分析速度和准确度,为单台大震速报和日常分析提供借鉴经验。     

灌云地震台面波震级偏差分析

选取2019年1月—2021年12月灌云地震台远震事件记录,将灌云地震台测算的面波震级与中国地震台网中心统一正式报目录震级进行对比,计算二者面波震级偏差平均值,并分析震级偏差与震级、震中距、震中方位之间的关系。结果表明：灌云地震台面波震级与中国地震台网中心统一正式报目录震级平均偏差为-0.08,总体偏差较小,表明该台地震记录精度较高。     

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。     

大连地震台面波震级偏差及其校正

文章采用大连地震台1983年到1986年四年间所记录的面波震级Ms≥4.0级的地震一千余例与《中国地震台临时报告》中所给定的面波震级进行比较,算出大连地震台的台基校正值,以及不同震中距,不同震中方位,不同震级的震级偏差及其校正值.     

第二影区地震震相到时特征变化浅析

运用国家台甚宽和超宽频带地震计记录的波形数据,对震中距介于105°~128°(即第二影区)的地震波形进行仿真处理,分析各台站地震波由地幔传播到核幔交界面时,各震相记录特征发生的变化。结果表明,当震中距增大到105°左右时,地震波进入到核幔过渡带这一复杂的低速层中,地震波能量衰减加快;P波与Pdif波震相未表现出明显的分界,S波震相也未出现断崖式消失,且随着震中距的增大还会出现。这也间接印证这一低速层的不均匀性。     

北京地震台远震Pn、PnPn波分析

在北京地震台NCDSN宽频带地震图集编辑工作中,发现Pn波在远至震中距16．8°的地震中仍然作为初至波被清晰记录,而PnPn波则延续至震中距30°左右仍以非常明显的震相特征被记录下来。     

北京地震台宽频带面波震级公式建立

利用IASPEI推荐的宽频震级计算公式MBB,重新量取并计算北京地震台1993—2003年(数字宽频地震记录系统与模拟地震仪器记录并行时期)的MBB、MSK、MKIRNOS震级,并分别同中国地震台网中心发布震级MCENC进行震级偏差比较。对比结果显示:采用宽频带垂直向速度型面波震级的MBB,震级偏差在震中距0°—180°范围内均呈现良好的稳定性,且与中国地震台网中心发布的震级偏差最小。遂利用最小二乘法,采用IASPEI公布的宽频带面波震级计算框架,拟合出北京地震台宽频震级公式。     

赤峰中心地震台面波震级偏差分析

地震震级是地震三要素之一,如何准确测定震级对于地震速报与应急工作至关重要。选取赤峰中心地震台2016年1月1日到2019年5月31日测定的674个地震事件的面波震级进行分析,并与中国地震台网中心发布的正式目录进行比较,并根据不同的震中距和方位角,给出面波震级偏差及校正值。结果表明:随着震级和震中距增大,震级偏差增大;赤峰中心地震台以北地区的不同方位角范围内,地震面波震级偏差分别为0.15、-0.13,以南地区的不同方位角范围内,地震面波震级偏差分别为0.22、0.16;根据参考校正值重新计算震级,通过震级对比结果表明校正效果较好。     

利用P波“影区”特征探测青藏高原东部岩石层内低速层

选用我国西藏及其周边地区测震台网35个台站宽频带数字地震仪记录到的2014年10月7日云南普洱M_S6.1地震的波形资料,分析了垂直向分量初至P波的幅度特征.结果表明:在震中距处于5°-18°之间的P波初动幅度相对较小,存在“影区”特征,推测该“影区”是由青藏高原下方岩石层内低速层所引起的;通过试错法,多次对比不同模型的理论波形与观测波形的P波初动振幅随震中距的变化形态,最终确定在78 km深处存在一厚度为24 km的低速层,层内速度梯度约为-0.05/s.      

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。     

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.     

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     

Pictorial Series of the Manifestations of the Dynamics of the Earth

Studia Geophysica et Geodaetica -     

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.     

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。     

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...     

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.     

Study of the Influence of the Indirect Effect of Ocean Tides and of the Direct Deformation Effect of the Atmosphere on the Results of GPS Observations

The geodynamic interpretation of the results of GPS observations among the permanently operating stations which establish the frame for defining and conserving the coordinate system and simultaneously for describing the fundamental tendencies of dynamics in the area represented by them, should be deprived of the effects of geodynamic phenomena, which can be either periodic or short-term (even non-periodic) so that secular changes may be found. Some of these influences are included in scientific processing software, others have to be modelled later. The purpose of this project is to determine the influences of the indirect effect of ocean tides and the direct deformational effect of the atmosphere on the results of GPS observations, performed at stations Pecný (Czech Republic), Wettzell (FRG) and Graz (Austria), and also for the GPS stations of the Central Europe Regional Geodynamic Project (CERGOP) in the region of Central and East Europe. On the basis of analyses and results it is possible to claim that at the present accuracy of GPS observations the influence of ocean loading and atmospheric pressure effects for geodynamic campaigns in the region of the Czech Republic is negligible. For campaigns in larger regions (i.e. Central Europe) atmospheric corrections will have to be applied to height differences. These corrections, however, due to their periodicity have negligible influence on secular changes.