共查询到20条相似文献，搜索用时 359 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.
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
3.
Sh. R. Bogoutdinov A. D. Gvishiani S. M. Agayan A. A. Solovyev E. Kin 《Izvestiya Physics of the Solid Earth》2010,46(11):1004-1016
The International Real-time Magnetic Observatory Network (INTERMAGNET) is the world’s biggest international network of ground-based
observatories, providing geomagnetic data almost in real time (within 72 hours of collection) [Kerridge, 2001]. The observation
data are rapidly transferred by the observatories participating in the program to regional Geomagnetic Information Nodes (GINs),
which carry out a global exchange of data and process the results. The observations of the main (core) magnetic field of the
Earth and its study are one of the key problems of geophysics. The INTERMAGNET system is the basis of monitoring the state
of the Earth’s magnetic field; therefore, the information provided by the system is required to be very reliable. Despite
the rigid high-quality standard of the recording devices, they are subject to external effects that affect the quality of
the records. Therefore, an objective and formalized recognition with the subsequent remedy of the anomalies (artifacts) that
occur on the records is an important task. Expanding on the ideas of Agayan [Agayan et al., 2005] and Gvishiani [Gvishiani
et al., 2008a; 2008b], this paper suggests a new algorithm of automatic recognition of anomalies with specified morphology,
capable of identifying both physically- and anthropogenically-derived spikes on the magnetograms. The algorithm is constructed
using fuzzy logic and, as such, is highly adaptive and universal. The developed algorithmic system formalizes the work of
the expert-interpreter in terms of artificial intelligence. This ensures identical processing of large data arrays, almost
unattainable manually. Besides the algorithm, the paper also reports on the application of the developed algorithmic system
for identifying spikes at the INTERMAGNET observatories. The main achievement of the work is the creation of an algorithm
permitting the almost unmanned extraction of spike-free (definitive) magnetograms from preliminary records. This automated
system is developed for the first time with the application of fuzzy logic system for geomagnetic measurements. It is important
to note that the recognition of time disturbances is formalized and identical. The algorithm presented here appreciably increases
the reliability of spike-free INTERMAGNET magnetograms, thus increasing the objectivity of our knowledge of the Earth’s magnetic
field. At the same time, the created system can accomplish identical, formalized, and retrospective analysis of large archives
of digital and digitized magnetograms, accumulated in the system of Worldwide Data Centers. The relevant project has already
been initiated as a collaborative initiative of the Worldwide Data Center at Geophysical Center (Russian Academy of Sciences)
and the NOAA National Geophysical Data Center (Unite States). Thus, by improving and adding objectivity to both new and historical
initial data, the developed algorithmic system may contribute appreciably to improving our understanding of the Earth’s magnetic
field. 相似文献
4.
中国地磁观测台网台站配备多种高精度连续观测仪器,获得大量数字化观测数据。为有效监控仪器运行状态、台站观测环境及观测数据质量,地磁观测台网引入多个数据评价指标,参考背景噪声即为其中一个重要指标,分析该指标在国际地磁静、扰日以及不同时间段的分布特征,评估其有效性,并利用观测数据验证其合理性。该指标可有效监控数据质量,及时反映地磁台观测运行中存在的问题,作为评估地磁观测台网对地磁场活动最小分辨能力的指标,尚蕴藏其他变化特征。参考背景噪声指标在数据质量监控和数据分析中具有一定应用价值。 相似文献
5.
The Study of Two Geomagnetic Jerks in China 总被引：1，自引：0，他引：1
This paper analyzes the first differences of the annual means (annual rate) for the Y and Z components of the geomagnetic field from nine magnetic observatories in China, measured from 1985 to 2003. The 1991 jerk was obvious in the Y component measured but not clear for the Z component. Rapid changes in the Z components were ubiquitous around 2000 -2001, but not seen for the Y component. External effects were removed from the monthly means by comparing the monthly mean of the geomagnetic field components at the observatories with the monthly time series of the Ap geomagnetic index. However, some examples were analyzed and showed whether external effects were removed or not, there was no marked distinction in determining the jerks in China for the Y component and the Z component of the geomagnetic field. Finally, the isolines of the first differences of the annual means were used to analyze the spatial and temporal distributions of the jerks. 相似文献
6.
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
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.
The results of the analysis of geomagnetic data synchronously recorded by the INTERMAGNET magnetic stations are presented. The goal of this research was to distinguish internal correlations between the data and to determine the optimal spatial interval of the geographical coordinates within which the efficient operation of only one magnetic observatory would be satisfactory in most occasions. The results of the observation of correlations between the geomagnetic data on a global scale are summarized and presented. Possible regions of application of these results are determined. 相似文献
9.
Geomagnetism and Aeronomy - The results of instrumental observations of variations in the Earth’s magnetic field conducted at a number of observatories of the INTERMAGNET network and the... 相似文献
10.
The decadal variation in the length of day and in the Earth's magnetic field is analyzed by empirical mode decomposition (EMD). The existence of a periodicity of about 60-years in the Earth's angular velocity has often been inferred and is confirmed here, with a new estimate of approximately 62 years. The existence of a similar periodicity in the geomagnetic field has been controversial. From the time series analyses presented here of the magnetic declination at 10 observatories, it is concluded that a geomagnetic periodicity of about 62?±?3 years does exist. A similar analysis of the magnetic inclination at five observatories gives a period of 58?±?5 years. The declination data from four observatories is found to correlate with the length of day signal, with a correlation coefficient of approximately 0.6. 相似文献
11.
Pc3 geomagnetic pulsations at near-equatorial latitudes at the initial phase of the magnetic storm of April 5, 2010 总被引：1，自引：0，他引：1
N. G. Kleimenova N. R. Zelinskii O. V. Kozyreva L. M. Malysheva A. A. Solov’ev Sh. R. Bogoutdinov 《Geomagnetism and Aeronomy》2013,53(3):313-320
An analysis of sampled 1-s observational data on geomagnetic pulsations within the Pc3 range on the INTERMAGNET network of near-equatorial and low-latitude observatories spaced over longitude during the initial phase of a moderate magnetic storm (April 5–7, 2010) was carried out for the first time. The obtained results were compared with magnetic observations at the low-latitude Chambon-la-Foret (CLF) and subauroral Kerguelen (PAF) observatories, as well as with observations at six Australian observatories located at low and middle latitudes. Two time intervals were studied in detail: the sudden commencement (SC) of the storm and the onset of the great global substorm. In the first interval, maximal amplitudes of near-equatorial pulsations were observed in the near-noon sector; in the second interval, in the near-midnight sector. The dynamics of the spectral structure of Pc3 pulsations in the considered events was shown to be different in spite of the fact that in both cases an amplification of waves was observed in two close spectral bands of the Pc3 spectrum: ～20–30 and ～30–40 mHz. The considered Pc3 pulsations were characterized by very small azimuthal wavenumbers (0.5 and less). Possible generation mechanisms for the observed Pc3 pulsations are discussed. 相似文献
12.
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
13.
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
14.
ＴｈｅＢｅｉｊｉｎｇｎｅｔｗｏｒｋｏｆｄｉｇｉｔａｌｇｅｏｍａｇｎｅｔｉｃｐｕｌｓａｔｉｏｎｏｂｓｅｒｖａｔｏｒｉｅｓＪｕｎ－ＣｈｅｎｇＺＨＯＵ（周军成）；Ｋｅ－ＬｉＨＡＮ（韩克礼）；ＹｕｅＬＵ（鲁跃）（ＩｎｓｔｉｔｕｔｅｏｆＧｅｏｐｈｙｓｉｃｓ，Ｓ... 相似文献
15.
A. E. Levitin L. I. Gromova S. V. Gromov L. A. Dremukhina 《Geomagnetism and Aeronomy》2014,54(3):292-299
A new method for determining geomagnetic activity based on calculation of the hourly amplitudes of geomagnetic field variations at ground-based observatories has been developed. Observations performed in 2009, when unusually low solar and geomagnetic activity was registered, were used as a reference level. The described method was used to estimate the energy of local geomagnetic activity; such energy is estimated for observatories in the Earth’s Northern and Southern hemispheres, and a total estimation is made for both hemispheres and for the entire Earth’s surface during large magnetic storms. These are used to compare characteristics of magnetic storm intensity based on the classical Kp and Dst indices and calculated energy estimate. 相似文献
16.
This paper describes the pattern of geomagnetic solar quiet day, Sq, variations recorded at the Indian geomagnetic observatories. The extent to which the high and low latitude ionosphere is
interlinked electromagnetically during periods of quiet geomagnetic conditions is a point of debate. The concept of Gabriel
graph is applied to derive the boundaries for the variations of horizontal, vertical, and declination components of the earth’s
magnetic field during geomagnetically quiet periods. Data of the six Indian geomagnetic observatories (Alibag, Hyderabad,
Nagpur, Pondicherry, Visakapatnam, and Trivandrum) are considered for this analysis. This graph theoretical model is complementary
to the classical data analysis techniques. Analytical method and the results of the analysis are presented in the paper. 相似文献
17.
用中国地磁台站的资料,研究了S_q逐日变化的形态学特征,用理论模型计算了磁层环电流、部分环电流、场向电流、磁尾电流、Chapman-Ferraro电流的地磁效应.在消除了这些磁层电流体系的影响之后,得到了电离层潮汐风发电机电流产生的磁场S_q变化.对1973年的资料研究表明,S_q发电机电流的逐日变化主要表现在强度上,即使在磁扰期间,也可以分离出形态稳定的S_q变化.由此提出了一种新的地磁指数——S_q指数,用来描述S_q发电机电流强度的逐日变化. 相似文献
18.
国际地磁台网计划INTERMAGNET 总被引：1，自引：1，他引：1
本文介绍了国际地磁台网计划（INTERMAGNET）的目的、意义、提出、发展过程及未来趋势，强调指出它对地磁台站现代化建设，地磁学研究，地球物理学发展以及空间天气预报的影响及作用．地磁场和空间环境的全球性质越来越迫切地要求各国学术团体和组织进行大规模国际合作，而作为地学研究的基础—台站建设与观测，资料收集与交换，资源共享与扩展—更应成为地球科学家关心的重要问题与焦点。 相似文献
19.
During magnetic active periods, disturbances in the geomagnetic field can act as natural noise masking other magnetic variations of small amplitude. In this paper, the influence of these perturbations on the observation of the effects on Earth of solar flares (sfe) has been studied. The diurnal and monthly values of detected sfe have been obtained, as well as the temporal variation of the relative occurrence of events. These numbers show how the irregular distribution of the magnetic observatories is an important limitation in the efficiency of the detection method. Some considerations about the actual method used at the International Service on Rapid Magnetic Variations are finally presented. 相似文献
20.
本文使用2008-2010年三年内的国内41个地磁台站和国外4个地磁台站的地磁水平分量H和磁偏角D的分钟值数据,研究了H和D的Vr指数(以下简称VrH和VrD)与Kp指数的关系及其时空分布特征,发现在时间变化上,VrH和VrD均具有27天太阳自转周变化;VrD呈现出显著的季节变化,而VrH却无,但与太阳风速度(SWS, Solar Wind Speed)变化密切相关,其三年的相关系数分别是0.97、0.70、0.88;去除季节变化后的VrD也表现出与SWS的相关,相关系数分别是0.96、0.77、0.5(2010年相关系数低主要受3月份Vr指数不明原因异常变化影响).在空间变化上,在我国大陆范围内,VrH和VrD均随纬度的增高而增大,并且具有地方时效应和显著的晨-昏不对称性,这种地方时效应和晨昏不对称性可能与部分环电流和场向电流有关系.研究认为Vr指数可以反映地磁场的快速变化,并可以间接反映SWS、部分环电流和场向电流对地磁场变化的影响和控制作用. 相似文献