共查询到19条相似文献，搜索用时 171 毫秒
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野外观测和室内试验表明,地震孕育和发生过程中可能产生电磁信号。地震电磁现象在防震减灾中具有潜在的应用价值,已成为21世纪国内外地学研究热点之一。由于地震电磁信号较弱,通常混杂于空间场源信号及人文噪音中,不易在观测数据中提取出来。以2003年1月日本茨城县5.1级地震为例,探讨远场参考在超低频(ULF)地震地磁数据处理中的应用,进而检测震前局部磁场异常。在此基础上,讨论远场参考法的优势及可能存在的不足。分析结果表明,2003年1月日本茨城县5.1级地震发生前存在局部磁场异常,验证了远场参考方法的有效性,相关成果可为地震地磁数据处理提供有益参考。 相似文献
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南京地磁台地铁干扰特征分析与抑制处理 总被引：2，自引：1，他引：1
地铁运行时产生的漏电流而形成的附加磁场会对附近的地磁观测造成严重干扰。通过对地铁供电系统的模拟分析得出了地铁干扰的一些基本特征。选取了2008年5月1日到30日南京地磁台受地铁干扰的日变数据和泉州参考地磁台日变数据,利用Welch功率谱估计法进行功率谱对比分析,发现地铁干扰主要对地磁场的Z分量、D分量的功率谱的高频部分造成影响,并且影响的频带范围几乎一致,主要集中在0．004-0．03Hz范围,而对H分量的影响比较微弱。在此基础上,通过小波变换对受干扰数据的Z分量和D分量进行干扰抑制处理,处理结果表明该方法能够有效抑制地铁造成的地磁场干扰。因此本文研究也提供了地磁台站干扰抑制的一种方法。 相似文献
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北京地磁台的磁环境监测 总被引：1，自引：0，他引：1
对北京地磁台建台以来,台站周边环境随着北京城市化进程发生的变化做了较详细的描述.利用几次在台站地磁观测区范围内的地磁场梯度观测资料,分析了台站地磁观测场地磁场梯度的变化情况,并对现有地磁场梯度环境进行了评估.为北京地磁台及全国其他台站,在现有条件下的地磁观测工作提供了有益的参考. 相似文献
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(1 回顾整理佘山与白水营地磁台历史概况及其观测资料,比较分析其磁倾角和磁偏角长年变化趋势大致相同,反映了地磁场长期变化现象.随着时间推移,研究分析历史地磁资料显得有其独特意义.不少地磁台观测环境受到干扰破坏,甚至新建地磁台观测也受到某些干扰影响,历史地磁观测资料对地震电磁学研究更显得可贵. 相似文献
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We investigate the features of the planetary distribution of wave phenomena (geomagnetic pulsations) in the Earth’s magnetic shell (the magnetosphere) during a strong geomagnetic storm on December 14–15, 2006, which is untypical of the minimum phase of solar activity. The storm was caused by the approach of the interplanetary magnetic cloud towards the Earth’s magnetosphere. The study is based on the analysis of 1-min data of global digital geomagnetic observations at a few latitudinal profiles of the global network of ground-based magnetic stations. The analysis is focused on the Pc5 geomagnetic pulsations, whose frequencies fall in the band of 1.5–7 mHz (T ～ 2–10 min), on the fluctuations in the interplanetary magnetic field (IMF) and in the solar wind density in this frequency band. It is shown that during the initial phase of the storm with positive IMF Bz, most intense geomagnetic pulsations were recorded in the dayside polar regions. It was supposed that these pulsations could probably be caused by the injection of the fluctuating streams of solar wind into the Earth’s ionosphere in the dayside polar cusp region. The fluctuations arising in the ionospheric electric currents due to this process are recorded as the geomagnetic pulsations by the ground-based magnetometers. Under negative IMF Bz, substorms develop in the nightside magnetosphere, and the enhancement of geomagnetic pulsations was observed in this latitudinal region on the Earth’s surface. The generation of these pulsations is probably caused by the fluctuations in the field-aligned magnetospheric electric currents flowing along the geomagnetic field lines from the substorm source region. These geomagnetic pulsations are not related to the fluctuations in the interplanetary medium. During the main phase of the magnetic storm, when fluctuations in the interplanetary medium are almost absent, the most intense geomagnetic pulsations were observed in the dawn sector in the region corresponding to the closed magnetosphere. The generation of these pulsations is likely to be associated with the resonance of the geomagnetic field lines. Thus, it is shown that the Pc5 pulsations observed on the ground during the magnetic storm have a different origin and a different planetary distribution. 相似文献
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V. B. Belakhovsky V. A. Pilipenko S. N. Samsonov D. Lorentsen 《Geomagnetism and Aeronomy》2016,56(1):42-58
Simultaneous morning Pc5 pulsations (f ~ 3–5 mHz) in the geomagnetic field, aurora intensities (in the 557.7 and 630.0 nm oxygen emissions and the 471.0 nm nitrogen emission), and riometer absorption, were studied based on the CARISMA, CANMOS, and NORSTAR network data for the event of January 1, 2000. According to the GOES-8 satellite observations, these Pc5 geomagnetic pulsations are observed as incompressible Alfvén waves with toroidal polarization in the magnetosphere. Although the Pc5 pulsation frequencies in auroras, the geomagnetic field, and riometer absorption are close to one another, stable phase relationships are not observed between them. Far from all trains of geomagnetic Pc5 pulsations are accompanied by corresponding auroral pulsations; consequently, geomagnetic pulsations are primary with respect to auroral pulsations. Both geomagnetic and auroral pulsations propagate poleward, and the frequency decreases with increasing geomagnetic latitude. When auroral Pc5 pulsations appear, the ratio of the 557.7/630.0 nm emission intensity sharply increases, which indicates that auroral pulsations result from not simply modulated particle precipitation but also an additional periodic acceleration of auroral electrons by the wave field. A high correlation is not observed between Pc5 pulsations in auroras and the riometer absorption, which indicates that these pulsations have a common source but different generation mechanisms. Auroral luminosity modulation is supposedly related to the interaction between Alfvén waves and the region with the field-aligned potential drop above the auroral ionosphere, and riometer absorption modulation is caused by the scattering of energetic electrons by VLF noise pulsations. 相似文献
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任熙宪 《地震学报(英文版)》2006,19(1)
Introduction It is well known that the local geomagnetic field would change during the pregnancy of an earthquake, which may be associated with the change of the electromagnetic impedances of the crust medium. This phenomenon has been paid attention for a long time and up to now a lot of work both in observation and theory of tectonomagnetism has been carried out and much progress has been achieved (Stacey, 1964; Johnston, 1978; QI, 1977; Rikitake et al, 1980; Shapiro and Ab-dullabekov, 1982… 相似文献
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Ren Xi-xian 《地震学报(英文版)》2006,19(1):87-92
A new concept is suggested on tectonomagnetic research about the noise in simultaneous geomagnetic difference data caused
by the effect of S
q local-time variation, together with the method of theoretical calculation. The level of the noise and its contribution to
the total noises of the differences data are analyzed. The result indicates that the noise increases linearly with the increase
of the distance between the two stations in the range of 40° longitude-difference, and its increasing rate is about 0.4 nT/(°)
at latitude 40°N. The example calculated at a pair of sites with longitude-difference 0.357°, shows that the noise is about
one fifth of the total noises of the difference data on geomagnetic quiet-day.
Contribution No. 06FE3008, Institute of Geophysics, China Earthquake Administration. 相似文献
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Identification and classification of transient pulses observed in magnetometer array data by time-domain principal component analysis filtering 
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下载免费PDF全文 A method for identification of pulsations in time series of magnetic field data which are simultaneously present in multiple channels of data at one or more sensor locations is described. Candidate pulsations of interest are first identified in geomagnetic time series by inspection.Time series of these ‘‘training events' ' are represented in matrix form and transpose-multiplied to generate timedomain covariance matrices. The ranked eigenvectors of this matrix are stored as a feature of the pulsation. In the second stage of the algorithm, a sliding window(approximately the width of the training event) is moved across the vector-valued time-series comprising the channels on which the training event was observed. At each window position, the data covariance matrix and associated eigenvectors are calculated. We compare the orientation of the dominant eigenvectors of the training data to those from the windowed data and flag windows where the dominant eigenvectors directions are similar. This was successful in automatically identifying pulses which share polarization and appear to be from the same source process. We apply the method to a case study of continuously sampled(50 Hz) data from six observatories, each equipped with threecomponent induction coil magnetometers. We examine a90-day interval of data associated with a cluster of four observatories located within 50 km of Napa, California,together with two remote reference stations-one 100 km to the north of the cluster and the other 350 km south. When the training data contains signals present in the remote reference observatories, we are reliably able to identify and extract global geomagnetic signals such as solar-generatednoise. When training data contains pulsations only observed in the cluster of local observatories, we identify several types of non-plane wave signals having similar polarization. 相似文献
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我国每天有数千趟高铁列车运行在两万多公里的高铁线路上,不但会引起高铁路基的振动,还会激发出地震波.地震检波器所接收到的数据中不仅包含窄带分立谱特性的高铁震源地震信号,还包含宽频带特性的背景信号.如何实现从检波器所接收到的高铁震源地震数据中分离出高铁震源地震信号和宽频带背景信号是准确利用该类信号的关键.考虑到高铁震源地震信号与宽频带信号在频率域明显的形态特征差异,本文首次将形态成分分析这种信号分离手段引入到高铁震源地震信号处理中,实现高铁震源地震信号的稀疏化建模并进而实现从接收数据中分离出高铁震源地震信号以及宽频带背景信号.对北京大学在中国南方某高铁沿线采集到的大量高铁震源地震数据进行处理,结果表明:采用形态成分分析并结合分块坐标松弛算法,能够实现实际采集高铁震源地震数据中的高铁震源地震信号和宽频带信号的分离. 相似文献
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为探查1988年3月前后在北京地磁台附近出现的较明显的地磁干扰噪声,我们在苏家坨—卧龙岗一带布设了8个测点,开展了专门的地磁干扰噪声实验观测。结果表明,该地磁干扰噪声主要是来自香山一带的电磁干扰,其次是北京市的地铁干扰。此地磁干扰噪声出现于每天06~h—23~h(北京时),其主要频谱成分在短周期(T=2—4 m)部分。另外本文的观测研究方法对于监测地磁台站(测点)的环境状况,改正受污染的地磁资料等方面具有实际应用价值。 相似文献
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N. G. Kleimenova 《Izvestiya Physics of the Solid Earth》2018,54(5):665-673
A thorough investigation of short-period oscillations in the Earth’s magnetic field as a fundamental natural process of the magnetospheric plasma began in Russia after V.A. Troitskaya established two oscillatory regimes in the geomagnetic field, namely, the regimes of continuous (Pc) and irregular pulsations (Pi). For studying these pulsations, 19 stations recording the telluric currents were installed during the International Geophysical Year (IGY, 1957–1959) on Troitskaya’s initiative. One of these stations was the Borok station. Subsequently, Borok has become the basic site for investigating geomagnetic pulsations and the main center for studying the short-period pulsations (SPPs) in the Earth’s magnetic field. This is the Borok scientific station where the key fundamental regularities of different types of geomagnetic pulsations were established. Troitskaya led and actively participated these works. Troitskaya organized and conducted the first complex geomagnetic observations in the world at the conjugate points Sogra (Arkhangelsk region, Russia) and Kerguelen (Indian Ocean). These studies were initially tested at the Borok observatory, where it was established that the wave packets of Pc1 geomagnetic pulsations are alternately observed in the northern and southern hemispheres in contrast to the other pulsation types which simultaneously occur in both hemispheres. The studies carried out at Borok promoted the establishment of a new direction in geophysics—diagnostics of the state of the magnetosphere based on the ground observations of geomagnetic pulsations. The analysis of simultaneous observations of the geomagnetic pulsations at polar latitudes of the Arctic and Antarctic was also for the first time conducted at the Borok observatory. This analysis revealed the main characteristics of wave phenomena at the geomagnetic poles and in the vicinity of the projection of the dayside polar cusp. Thus, for the first time in the world, Troitskaya and her Borok colleagues established the key patterns of the oscillatory regimes in the geomagnetic field of the Earth. This laid the basis for the further experimental and theoretical investigations which have shown that SPPs play a leading role in the dynamics of the magnetospheric plasma. In this paper we also list of 60 of Troitskaya’s main publications. 相似文献