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2021年5月21日云南漾濞县发生M_S6.4地震、5月22日青海玛多县发生M_S7.4地震,分别分析漾濞震中500 km内12个地电场台数据、玛多震中500 km内8个地电场台数据,获知:(1)漾濞地震周围罗茨等8台优势方位角在震前出现了异常变化,弥渡等4台看不出明显异常变化;盐源等7台相关系数在震前2～6个月出现了大幅度下降,元谋、苴林等5台相关系数看不出明显异常变化。(2)玛多地震周围门源等4台方位角在震前出现了异常变化,都兰等4台方位角看不出明显异常变化;门源等5台在玛多地震前2～6个月相关系数出现了大幅下降、变化范围明显变窄等现象,都兰、白水河、金银滩等3台优势方位角和相关系数都看不出明显异常变化。(3)两次地震分析中地电场优势方位角和相关系数异常变化在时间上皆具有同步或准同步性。 相似文献
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对太原台BM_3井、S_1井、夏县台2井地下水位与短水准测量资料进行了分析,并以代县台3井作为例证,利用低通滤波、回归方法对资料进行了处理,表明山西省多数定点短水准测量受地下潜水位变化的影响明显,最大量级可达0.7mm/1m水位,水准点的变化随农用机井抽水方式的不同而有所差异。 相似文献
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利用新疆伽师震区附近的喀什、乌什、巴楚3个数字台记录到的伽师地震序列波形资料,开展地震波谱研究。首先分析了伽师6.8级地震序列各台的地震波拐角频率及其比值的时序变化特征,然后从中选出对这3个台都有较好记录的66个地震事件,进行拐角频率比时序变化特征的对比研究。结果表明,这3个台的拐角频率及其比值在伽师6.8级地震前后都出现了不同的变化趋势,尤以比值的变化更为明显,而且不同台站间的变化趋势存在较为明显的差异。最后讨论了这些差异可能存在的一些原因。 相似文献
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通过甘肃省嘉峪关台地磁场观测资料,研究嘉峪关台、瓜州台磁静日地电场日变化的时频特征波;由地电场分钟值观测数据的时序叠加残差方法,研究嘉峪关、瓜州山的地电暴变化。结果表明:(1)两台地电场静日变化以两次起伏变化为主,无相位差,但两台之间日变幅差异较大;(2)地电场分量变化与地磁场正交分量变化显著相关;地电场与地磁场日变波形不同,极值时间有差异。2个台存在很明显的高频成分,在去除了高频变化后,其优势周期也相同,从大到小依次为12 h、8 h、24 h。地磁场H分量因存在磁暴影响,故高频变化较多,在去除了磁暴影响后,其优势周期从大到小依次为24 h、12 h、8 h;(3)当电磁暴扰动剧烈时,两台可以较清晰地记录到地电暴的完整变化。在发生电磁暴时,地电场与地磁场的相关性明显降低,且不同台、不同测向之间的变化幅度也不尽相同。两台东分量E_Y暴日的日变幅较静日明显增大,磁暴期间Y分量变化率与地电场东分量E_Y观测数据显著相关,由此说明:两台日变幅的不同与台站台址电导率有关,太阳风引起的电离层活动是引起了地电场日变化主因。引起电暴的原因可能不同于引起日变化的原因,主要是两台之间及不同测向之间的浅、深层电阻率和地质构造等诸多因素的结果。 相似文献
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地磁观测要达到为国民经济、科学研究和地震预报服务的目的 ,必须保证观测资料的质量。泾县台目前仅有磁绝对值观测 ,使用 FG-861质子旋进磁力仪作北京时 2 1时 0 0分定点观测 ,测量地磁场总强度 F和垂直分量 Z。 1 997年 3月 2 2日 ,泾县台地磁垂直分量 Z突跳1 0 n T,而安徽省的蒙城、蚌埠、金寨等台的垂直分量均变化平稳 ,蒙城台三分量磁照图亦变化平稳 ,没有磁扰。毗邻的江苏省溧阳、南京台的垂直分量变化亦在 1～ 3n T以内。从1 995年 1 0月到 1 996年 1 0月的泾县台与蒙城、上海、武昌台的观测值对比图上也可看出 ,泾县台曾多次出现… 相似文献
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应用差分法分析了高淳台、溧阳台、高邮台、连云港台、宿迁台、海安台地磁垂直分量Z的变化,以加卸载响应比方法研究地磁极值的变化,用Z极小值时间进行地磁低点位移分析,对这些台站资料进行相关分析,研究发现中强震前高淳台的地磁场存在明显的异常变化. 相似文献
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利用球冠谐分析法对2009年我国35个绝对观测地磁台站的Sq太阳静日变化进行内外源场分离,反演得到三个劳埃德季节(冬季D,分点E,夏季J)相应的内、外源等效电流体系,结果表明Sq外源电流体系在该区域D、E、J三个季节的电流涡中心强度分别为56.2 kA、137.7 kA、137.9 kA,电流涡中心位置的地方时由冬季的1124LT前移至夏季的约1030LT;Sq内源电流体系在该区域D、E、J三个季节的电流涡中心强度分别为21.1 kA、63.4 kA、72.7 kA,电流涡中心位置的地方时由冬季的1100LT前移至夏季的约1000LT. 相似文献
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2000年Jerk存在吗 总被引：2，自引：0，他引：2
陈伯舫 《地震地磁观测与研究》2006,27(5):50-52
从分布在欧亚美太平洋几个质量较好的台站的dY/dt变化曲线看,2000年或2001年似乎没出现新的Jerk(Y)。 相似文献
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Wallace H. Campbell 《Pure and Applied Geophysics》1987,125(2-3):427-457
The electrical conductivity of the Earth's upper mantle can be inferred from geomagnetic quiet-day,Sq, variations recorded at the world's observatories using the, coefficients of a spherical harmonic analysis (SHA) that separate the external (source) and internal (induced) parts of the surface field. The conductivity profile determined from such an analysis can be sensitive to special characteristics of the quiet field itself as well as the separation techniques employed. This review of the Sq-analysis features critical to a conductivity derivation is pictorially presented along with the equations for application of theSchmucker (1970) technique to theSHA coefficients for a conductivity determination. Three examples illustrate the use of these equations with differentSq models. 相似文献
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陈伯舫 《地震地磁观测与研究》2002,23(5):6-8
从太平洋4台的分析显示，APIA，GUAM和PAMATAI台Z分量的太阳黑子周变化与HONOLULU台的相位相反。可是，CANBERRA台的变化又和HONOLULU台同相。这种表现复杂的地方性差异，更反映出太阳黑子周变化源于外场之说的有问题的。 相似文献
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S. S. Starjinsky 《Geomagnetism and Aeronomy》2008,48(2):265-276
Results of studying the lunar daily geomagnetic variations in the spectral and time regions at the network of observatories are presented. The seasonal variations in the amplitudes of the fundamental harmonic constituents of three lunar variation components have been revealed. The seasonal time variations have been analyzed using the digital bandpass filtering and harmonic synthesis based on the data of the Kakioka and Memambetsu geomagnetic observatories. The 11-year solar cycle and annual and semiannual periods have been distinguished in the seasonal variation spectrum. Studying the spectral singularities of the lunar daily variation at these observatories and the sea level variations in daytime and nighttime hours has made it possible to identify the contribution of the oceanic dynamo to the lunar variation vertical component. 相似文献
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An inspection of the long-term behaviour of the range of the daily geomagnetic field variation from comprehensive modelling 总被引：1，自引：0，他引：1
J. Miquel Torta Luis R. Gaya-Piqu Juan J. Curto David Altadill 《Journal of Atmospheric and Solar》2009,71(13):1497-1510
This paper attempts to reveal whether long-term trends in the ionosphere are reflected in the amplitude range of the geomagnetic daily variation recorded at ground level. The smooth and regular variation observed in the magnetograms on magnetically quiet days is induced by the ionospheric currents flowing in the dynamo region. So it is likely that trends in the conductivity or in the dynamics of this region could produce changes in the current densities, and consequently in the range of the geomagnetic variation. The crucial aspect is how to separate the changes produced by the geomagnetic activity itself, or by secular changes of the Earth's magnetic field, from the part of the variation produced by factors affecting trends in the ionosphere, which could have an anthropogenic origin. To investigate this, we synthesized for several geomagnetic observatories the daily ranges of the geomagnetic field components with a comprehensive model of the quiet-time, near-Earth magnetic field, and finally we removed the synthetic values from the observed ranges at those observatories. This comprehensive model accounts for contributions from Earth's core, lithosphere, ionosphere, magnetosphere and coupling currents, and, additionally, accounts for influences of main field and solar activity variations on the ionosphere. Therefore, any trend remaining in the residuals, assuming that all the contributions mentioned above are properly described and thus removed by the comprehensive model, should reflect the influence of other sources. Results, based on series of magnetic data from observatories worldwide distributed, are presented. Trends in the X and Z components are misleading, since the current system changes in form as well as in intensity, producing changes of the focus latitude in the course of a solar cycle and from one cycle to another. Some differences exist between the long-term trends in the Y component between the real and modelled ranges, suggesting that other non-direct solar causes to the amplitude changes of the solar quiet geomagnetic variation should not be ruled out. Nevertheless, the results also reflect some short-comings in the way that the comprehensive modelling accounts for the influence of the solar activity on the range of the daily geomagnetic variation. 相似文献
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Variations of geomagnetic components X, Y, and Z recorded in 19 Intermagnet European observatories in 2004 were analysed. The original data from all observatories were preliminarily
processed. In the first step, periods longer than three hours were filtered out. In the second step, variations of vertical
geomagnetic component Z were separated into external and internal parts. We introduced a non-dimensional index η defined as the square root of a ratio of the energy of the external part of the vertical component to that of the horizontal
components. Maps of the surface distribution of a new magnetic index η for the area of Europe at selected time periods were created, and their time changes are presented. The time changes of η for selected observatories are also shown. Moreover, we discuss a very interesting phenomenon we discovered, that has never
been described in geophysical literature. Namely, in the recordings of all the observatories we noticed the presence of very
regular variations, observed almost exclusively in the vertical component Z, which is quite unusual. These regular variations occur in the form of sinusoidal “wave packets”. The amplitudes of these
variations do not depend on the geomagnetic latitude and appear in the records of all the observatories we analyzed. They
occur in quiet days, which suggests that their source is in the ionosphere. 相似文献
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陈伯舫 《地震学报(英文版)》1994,7(3):457-464
ＩｎｖｅｓｔｉｇａｔｉｏｎｓｏｆｔｈｅｓｅｉｓｍｏｍａｇｎｅｔｉｃｅｆｆｅｃｔｉｎｔｈｅｇｅｏｍａｇｎｅｔｉｃｄｉｕｒｎａｌｖａｒｉａｔｉｏｎｓＰｏ－ＦａｎｇＣＨＥＮ（陈伯舫）（ＤｅｐａｒｔｍｅｎｔｏｆＰｈｙｓｉｃｓａｎｄＤｅｐａｒｔｍｅｎｔｏｆＧｅ... 相似文献
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D. R. Barraclough T. D. G. Clark S. W. H. Cowley F. H. Hibberd R. Hide D. J. Kerridge F. J. Lowes S. R. C. Malin T. Murphy H. Rishbeth S. K. Runcorn H. C. Soffel D. N. Stewart W. F. Stuart K. A. Whaler D. E. Winch 《Surveys in Geophysics》1992,13(1):47-88
A joint Discussion Meeting of the Royal Astronomical Society and the Royal Irish Academy, held on January 11th, 1991, commemorated the establishment of some early magnetic observatories, discussed recent research using global geomagnetic data and described the present status of magnetic observatories in the United Kingdom. The observatory and instruments at the Dublin magnetic observatory; the origins of the Greenwich magnetic observatory, and why it eventually had to be resited; and the history of the Munich magnetic observatory formed the historical part of the proceedings. Current research topics discussed were the geomagnetic secular variation and deep Earth structure and dynamics; fluid flow patterns near the top of the core; the origin of the annual variation of the geomagnetic field; results of an analysis of monthly means from some British observatories; a new theory of the geomagnetic daily variation; and the interactions between ionospheric science and geomagnetism. The present-day observatory scene was described in terms of the information that can be derived from the almost 40 year series of data from Hartland magnetic observatory; of the methods used to process data from the three UK magnetic observatories, which nowadays are operated automatically and remotely; and (a look into the future) of a new project, INTERMAGNET, which aims to make available, in near real time, data from the world-wide network of magnetic observatories. 相似文献