共查询到20条相似文献，搜索用时 921 毫秒
1.
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
2.
IGRF（国际地磁参考场）是有关地球 主磁场与长期变化的模型，IGRF的误差主要来源于：忽略外源场、球谐级数的截断、台站分 布的不均匀、测量、忽略地壳磁异常场等. 分析我国大陆地区IGRF的误差，有利于我国地磁 研究 人员在工作中合理地应用IGRF资料. 如果不计磁异常与环境干扰都比较大的北京台，29个基 准台的IGRF的误差(均方根差)为146.9nT. 相似文献
3.
Igor Mandić Eugen Vujić Balázs Heilig Izidor Pelajić Davorka Herak 《Acta Geophysica》2016,64(5):1311-1339
More than ten years ago, the Geophysical Institute initiated the installation of a geomagnetic observatory in Croatia. Over the past decade, extensive surveys and studies have been conducted in order to determine the proper location for the observatory. Finally, in 2012, the observatory was established in Lonjsko Polje. This paper presents the first data recorded in the period 2012.5-2015.0. Also presented are the technical aspects and data processing techniques of this remotely operated observatory. Analysis of data quality and comparison with data from the surrounding INTERMAGNET observatories is discussed in detail. Although remote observatories cannot provide the ideal environment for magnetometers, the obtained results accentuate the potential of the new observatory to provide high-quality data. The establishment of this observatory paves the way for scientific and professional development of geomagnetism in Croatia. 相似文献
4.
The hourly data of nine geomagnetic observatories situated in Central Europe have been analyzed using the generalized magnetovariation
(GMV) method designed recently for induction soundings of inhomogeneous media. In this method, impedance is one of transfer
functions in the differential relation between spectra of the magnetic components and their derivatives. The peculiarity of
this impedance is its correspondence to the magnetotelluric one estimated from the linear relations. Three transfer functions
have been estimated simultaneously for data of geomagnetic observatories, using three different routines working in the period
range from three hours up to two days. Noises in the source field components have been compared with noise in the estimated
plane field divergence. The multivariate errors-in-variables method was used to extract spatially and temporally coherent
geomagnetic field structure from the partially incoherent geomagnetic variations. This method allows estimating reliably impedances
and gradient tippers for each observatory, taking into consideration the Earth’s sphericity. The obtained responses have been
used for induction soundings and for detecting a deep inhomogeneity in the region. 相似文献
5.
中国部分地磁台站年均值与IGRF模型一致性分析 总被引：1，自引：0，他引：1
利用中国部分地磁台站1990～2003年的年均值资料,研究了台站年均值与IGRF模型计算值的一致程度,结果表明：①我国地磁台站的长期变速度与IGRF模型的长期变速度有差异：总体来讲,我国台站磁偏角D和垂直强度Z的长期变速度低于IGRF模型的相应速度;水平强度H的长期变速度在1990～1995年间高于IGRF模型的相应速度,在1995～2000年间低于IGRF模型的相应速度;②台站年均值与IGRF模型值的差值曲线中,H和Z有明显的起伏,反映了地磁场长期变的非线性;③虽然有上述长期变上的差异,但对于同一个台站,各地磁要素年均值与IGRF模型值的差值的标准偏差均低于IGRF模型的误差水平,说明IGRF模型与台站年均值的一致性比较好;④对于同一地磁要素,不同台站的年均值与IGRF模型值的差值的平均值相差较大,反映出台站所在位置地壳磁异常的巨大差异。通过总结上述工作,文中还讨论了地磁台站保持长期可靠运行的重要性以及地磁台网历史观测资料抢救的紧迫性。 相似文献
6.
7.
《地震科学（英文版）》2010,(4)
By calculating the hourly standard deviation of the first-order differences of the horizontal geomagnetic component minute data,a new index Vr to represent the variation rate of the geomagnetic field was introduced.Vr-indices show similar trends in the temporal change at different observatories and have simultaneous peak values at the observatories covering a large span geographically,which reveals that the source of geomagnetic disturbances represented by Vr is in the magnetosphere.Based on the comparison among Vr,Kp and ap,it is found that generally Vr changes linearly with Kp and ap,which means that the rapid changes of magnetic field usually exist together with magnetic disturbances.But there are exceptions.As Vr can be easily produced by individual observatory in quasi real time and is more sensitive to the variation rate of geomagnetic field rather than the field itself,it can be expected to serve for monitoring or predicting the geomagnetic-induced event in a quick and intuitive way. 相似文献
8.
从国际地磁台站分布、地磁信息节点分布、地磁观测技术指标、数据产品及服务应用等5个方面介绍了国际地磁台网的发展现状。通过综合分析,得出地磁场和空间环境的全球性精细化监测及预报已经成为地球科学家关注的焦点。在此基础上,从4个方面预测了国际地磁台网未来发展趋势,以期为我国开展相关工作提供参考和借鉴。 相似文献
9.
Eugen Vujić 《Acta Geophysica》2016,64(2):320-335
A general mathematical tool for expanding vector systems on a sphere into basis functions, spherical elementary current system (SECS) method, was applied for separation of the geomagnetic field variations into external and internal parts, over a limited region of central and southeastern Europe. The registered variations at three Croatian repeat stations were compared to the variations estimated by the SECS method using the variations from the different sets of observatories. The results of the SECS method were also compared to a simple assumption that the variations at repeat station are equal to those at particular observatory. The relevance of this comparison was to get an insight about the possibility of using the SECS method for estimating the geomagnetic field variations over Croatia. The guidelines for the application of the SECS method for the purpose of reducing repeat station data were also given. 相似文献
10.
11.
The geomagnetic field components are periodically measured at repeat stations. The main objective of the repeat stations is to provide data for tracing the secular variation of the geomagnetic field components. Secular variation at the repeat station is generally different from that at geomagnetic observatory used in the data reduction. The effect of the secular variation differences on geomagnetic data reduction was estimated for the regions of Europe, North America (below 60°N) and Australia, respectively, during the period of 2000-2010. These estimations were obtained by using the monthly mean values of north, east and vertical components of geomagnetic field, recorded at geomagnetic observatories. The effects were calculated by using observatories pairs, with distances from 350 km (in Europe) to 3100 km (in North America and Australia). The maximal effects were found to be the smallest in east component in Europe and North America, and vertical component in Australia; the effects increase with time from a central reduction epoch and they are not constant during mentioned eleven years; they were less than 1 nT only in Europe, for distances between the observatories up to 1000 km in all three components and for periods spanning ±1 month from a central epoch. It was found that their year to year variability is mostly due to the non-eliminated external field residuals in the observatories monthly means; their effect is up to 3 nT for ±3 months from a central epoch. Further, the real effects were compared to those modeled by IGRF-12 model. The maximal differences between the real and the modeled values are below 4.5 nT in all three components, for ±3 months from a central epoch. 相似文献
12.
A. A. Soloviev R. V. Sidorov R. I. Krasnoperov A. A. Grudnev A. V. Khokhlov 《Geomagnetism and Aeronomy》2016,56(3):342-354
In 2011 Geophysical Center RAS (GC RAS) began to deploy the Klimovskaya geomagnetic observatory in the south of Arkhangelsk region on the territory of the Institute of Physiology of Natural Adaptations, Ural Branch, Russian Academy of Sciences (IPNA UB RAS). The construction works followed the complex of preparatory measures taken in order to confirm that the observatory can be constructed on this territory and to select the optimal configuration of observatory structures. The observatory equipping stages are described in detail, the technological and design solutions are described, and the first results of the registered data quality control are presented. It has been concluded that Klimovskaya observatory can be included in INTERMAGNET network. The observatory can be used to monitor and estimate geomagnetic activity, because it is located at high latitudes and provides data in a timely manner to the scientific community via the web-site of the Russian–Ukrainian Geomagnetic Data Center. The role of ground observatories such as Klimovskaya remains critical for long-term observations of secular variation and for complex monitoring of the geomagnetic field in combination with low-orbiting satellite data. 相似文献
13.
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
14.
流动地震地磁矢量观测是一种获取地震前兆异常的方法,试验研究和观测实例表明,地震孕育引起的地磁场异常变化量级较小,因此在观测、数据处理过程中都要尽可能消除误差提高精度.本文主要从地磁矢量数据日变通化精度方面开展讨论,首先使用反距离加权插值法由泰安、武汉、崇明、杭州4个地磁台观测资料计算出蒙城地磁台相应的虚拟地磁数据,其磁偏角、水平分量、垂直分量三个要素与真实观测值的相关系数分别高达0.9987、0.9946和0.9806,验证了反距离加权插值方法对地磁观测数据空间插值的有效性.其次,选择东部和西部测区分别使用反距离加权插值方法建立各地磁矢量测点位置的虚拟日变台并用其进行通化,实例计算结果表明,该方法可有效提高日变通化精度,对于地磁台站稀疏地区更具实际应用价值. 相似文献
15.
通过对同一台站人工观测的地磁场总强度F与连续记录F,及两套连续记录仪记录的地磁场总强度F夜均值的差值分析,发现同一台站两种差值均存在显著的年变化特征。对其他台站同样可以看到类似变化。而各时段的时均值差值也表现出相似的变化特征。由此说明,同一台站地磁观测区的不同点位,地磁场差异在长时间内不断发生变化,在进行绝对观测时,无法通过选择绝对观测时间消除该差值变化。 相似文献
16.
17.
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
18.
19.
ZHANG Yan-hui LI Shi-wen WENG Ai-hua ZHANG Su-qin YANG Yue LI Jian-ping TANG Yu 《地震地质》2019,41(4):979-995
Geomagnetic depth sounding is an effective method for exploring deep structure of the earth. There are dense geomagnetic observatories in China, which lays a foundation to obtain the electrical structure of the transition zone and the upper part of the lower mantle beneath China. However, the corresponding C-responses estimation methods which are applied now cannot get the stable C-responses for many observatories. Thus, a large amount of geomagnetic data is wasted. Therefore, in order to make full use of the geomagnetic data, the estimation of C-responses needs to be systematically studied. Because of the heterogeneous characteristics of the data quality of China's geomagnetic observation data, such as the quality of the data, the length of the record, the types of data(absolute and relative observation)and data discontinuity condition, many geomagnetic data are abandoned, this limits the resolution of mantle electrical structure studies. In this paper, the following techniques are used to improve the stability of the data and increase the number of the available geomagnetic observatories, in the meantime, the stability of the C-responses curves can be effectively improved:1)obtaining the stable spectrums of the different components for each frequency by the BIRRP(Bounded Influence, Remote Reference Processing)software, and using the global smoothing technique to suppress data noise on geomagnetic data; 2)As for the geomagnetic data which only records the relative variation of the D, H and Z components and doesn't have the baseline value, the horizontal component is decomposed by the approximate estimation method to obtain the C-responses of the relative variation data, and then the relative variation data is used directly for the C-responses estimation; 3)the effects of discontinuous data and short-record data on C-responses estimation are discussed. Under normal conditions, the discontinuity of the data has little influence on C-responses, and when the data length is shorter than 5 years, we can hardly get the available C-responses whose periods are longer than 40 days. All these experiments can provide a basis for the data processing of these kinds of observation data; 4)for coastal observatories, the ratio method is used to eliminate the influence of ocean effect on the C-responses functions. After carefully processing the data of more than 100 geomagnetic observatories in China by the above techniques, the stable C-responses function of 42 observatories is finally obtained, among them, the number of the observatories with C-responses ranging from 1.3 to 113.7 days is 24, and the observatories with C-responses ranging from 1.3 to 42.6 days are 18. The techniques of this paper can process heterogeneous data well and obtain more stable C-responses, which provides more basic data for high-resolution geomagnetic depth sounding inversion researches in China. 相似文献
20.
Surveys of the geomagnetic declination, inclination and total field intensity were carried out at eight stations of the Croatian
Geomagnetic Repeat Stations Network in 2004 and 2007. The total field time series at repeat stations and observatories were
compared by use of the multi-linear regression and linear correlation coefficients. The surveys’ data were reduced to 2004.5
and 2007.5 epochs by a simple method proposed here, assuming the secular variations at the repeat station and observatory
are equal or different, respectively. These reductions, obtained in reference to L’Aquila, Fürstenfeldbruck and Tihany observatories,
and corresponding weighted as well as non-weighted averages, were compared. The preferred geomagnetic field elements as well
as the corresponding annual changes between 2004.5 and 2007.5 epochs, were compared to the latest International Geomagnetic
Reference Field. Additionally, the Croatian Geomagnetic Normal Reference Fields for 2004.5 and 2007.5 epochs were presented. 相似文献