共查询到20条相似文献，搜索用时 109 毫秒
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《地质科学》2001,(2)
(按影响因子为序 ,摘引自中国科技信息研究所信息分析中心 1 999年 1 2月引证报告 )期刊名总被引频次影响因子期刊名总被引频次影响因子地学前缘 2 4 4 1 .0 0 8海洋地质与第四纪地质 2 2 0 0 .346岩矿测试 373 0 .959地震 2 0 4 0 .345地质学报 50 90 .948高校地质学报 580 .340地球化学 41 7 0 .935地质地球化学 92 0 .339第四纪研究 30 6 0 .82 9古生物学报 3480 .333地质科学 3790 .80 8中国地震 1 92 0 .32 3地理学报 51 0 0 .80 2山地研究 880 .31 8冰川冻土 344 0 .679地壳形变与地震 1 32 0 .31 3测绘学报 1 61 0 .679地震地磁观测… 相似文献
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南京台位于南京市中山陵风景区，见图1。现有体应变、短水准测量、地磁、地电、大地电场、测震等观测手段。体应变观测项目是“九五”数字化改造项目，于1998年4月lO日安装观测，仪器型号：TJ-2B型体积式应变仪，灵敏度：2．30mV／10^-8，钻孔岩性是石英砂岩，钻孔深度为62．3m。2004年度仪器工作正常，全年M2波潮汐因子平均值为0．8654、潮汐因子中误差为0．0173、相对中误差为0．0199，记录固体潮较为清晰稳定。 相似文献
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地磁无源导航是利用地磁场信息来限制惯性导航系统的误差增长,满足潜艇自主性、隐蔽性和高精度的要求。笔者介绍了地磁无源导航的发展,分析了以往研究存在的问题并指出:①潜艇无源导航必须利用小尺度的、实测的地磁图,而不能直接用国际地磁参考场IGRF;②利用地磁场导航必须考虑地磁日变的影响。阐述了利用卡尔曼滤波进行地磁无源导航的原理和算法,同时作了仿真试验,结果表明达到了用地磁场辅助惯性导航的效果,并叙述了地磁日变特征,讨论了消除日变影响的方法,在无连续磁暴日出现的前提下,提出了解决方案,通过均值日变校正,在一定程度上减小了日变干扰,最后以小尺度的东海某区海洋地质调查中的地磁异常数据库资料对潜艇无源导航过程进行了仿真试验,修正了潜艇的导航定位。 相似文献
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根据沙河、正定、商丘、东营四测站三天同步测量所获取的地磁日变数据,提出了三种局部地区地磁日变的拟合方法;井通过对四测站三天地磁日变曲线的分析发现了时差对日变曲线的非均衡影响以及东营日变具比较明显的海岸效应之影响。 相似文献
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据福建数字遥测地震台网测定 ,2 0 0 1年 1月 1日至 1 2月 3 1日福建及其近海地区共发生ＭＬ≥ 2 0级地震 82次 ,其中 2 0～ 2 9级地震 71次 ,3 0～ 3 9级地震 1 0次 ,最大地震为 8月 6日漳浦海外 4 2级 ;台湾海峡地区发生ＭＬ≥ 3 0级地震 4次 ,最大地震为 1 0月 1 3日海峡南部 4 2级 ;台湾地区共发生ＭＳ≥ 5 0级地震 1 3次 ,最大地震为 6月 1 4日苏澳以东海中的 6 1级。对比 1 991年以来闽台地区年度地震活动水平 ,今年各区地震活动在去年较为平静的基础上 ,继续呈现减弱态势。 1 999年 9月 2 1日台湾南投 7 6级强震群活动前后 ,福… 相似文献
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李忠平 《物探化探计算技术》2009,31(5):434-436
通过收集某地区地磁台记录的磁场,和当天另一地区地磁日变场数据,以某地的地磁台记录磁场作为参考地磁场,以另一地当天地磁日变场作为主要地磁场,采用傅立叶变换对时变地磁异常进行频谱分析。计算出二地的地磁场水平导数和某地磁响应参数及视电阻率,并对其进行了一维电磁测深反演,与在同一测深剖面施测的可控源音频大地电磁测深（CSAMT）反演结果对比分析,效果基本一致。采取这种计算方法,可有效地提取磁异常深部信息,为危机矿山深部找矿增加一种新的解释手段。 相似文献
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《Russian Geology and Geophysics》2014,55(9):1138-1145
Global geomagnetic data are inverted for detecting a high-conductivity layer at depths of 1500–2000 km to test the hypothesis of a magnesiowüstite phase transition in the lower mantle. We present the results of processing of both synthetic and global data—average monthly values of the geomagnetic field from 1920 to 2009. The inverted global data are consistent with the possible existence of a high-conductivity layer at great depths in the lower mantle. 相似文献
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This paper presents relative secular variations of the total intensity of the geomagnetic field against a background of results of magnetic anomaly interpretation along seismic profile P4. Profile P4 crosses a Variscan folding zone in the Paleozoic Platform (PLZ), the Trans-European Suture Zone (TESZ), and the Polish part of the East European Craton (EEC). Secular geomagnetic field variations
measured in 1966–2000 along a line adjacent to seismic profile P4 were analysed. The study of secular variations, reduced to the base recordings at the Belsk Magnetic Observatory, showed that the growth of geomagnetic field at the East European Craton was slower than in the Trans-European Suture Zone and the Paleozoic Platform.A 2D crustal magnetic model was interpreted as a result of magnetic modelling, in which seismic, geological and geothermal data were also used. The modelling showed that there were significant differences in the magnetic model for geotectonic units, which had been earlier determined based on deep seismic survey data. It should be noted that a fundamental change of trend of the relative secular variations was observed at the slope of the Precambrian Platform. After analysing the geomagnetic field observed along profile P4, the hypothesis that the contact between Phanerozoic and Precambrian Europe lies in Poland's territory can be proven. 相似文献
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《Atmósfera》2014,27(3):227-237
The O+ ion density measured by the SROSS-C2 satellite during solar minima (year 1995, F10.7 = 77) and maxima (year 2000, F10.7 = 181) has been analyzed for studying diurnal, seasonal, latitudinal and geomagnetic variations. The study region covers an area encompassed between 5-3 5° N latitude and 65-95° E longitude over India at a ~500 km altitude (F2 region). The year 2000 shows significant enhancement in the annual average of O+ ion density and attainment of post sunset secondary enhancement compared to 1995. Attributed to photoionization, daytime shows a maximum ionization compared to nighttime. However, attainment of post sunset secondary maxima is attributed to the strong pre-reversal enhancement in the vertical E x B drift. The effect of geomagnetic activity Kp through the E x B drift dynamic movement on O+ ion density distribution studies indicates periodicities of seven and nine days in 1995 and 2000, respectively, and polynomial dependency of the O+ ion density on geomagnetic activity Kp. Further on, stratification of the O+ ion density according to latitude (5-35° N) indicates high density in mid-latitudes (12-24° N) compared to high and low latitudes, except in the winter of 1995, which shows a distinct trend (i.e., density decreases with increasing latitude). 相似文献
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D. S. V. V. D. Prasad P. V. S. Rama Rao G. Uma S. Gopi Krishna K. Venkateswarlu 《Journal of Earth System Science》2005,114(4):437-441
Using the data of amplitude scintillations recorded at 244 MHz from the geostationary satellite, FLEETSAT (73‡E) at a low
latitude station, Waltair (17.7‡N, 83.3‡E, 20‡N dip), during the increasing sunspot activity period of 1997–2000, the effect
of the geomagnetic storms on the occurrence of ionospheric scintillations has been studied. A total of 60 SC storms studied
during this period, following the Aarons’ criterion, reveals that the local time of onset of the recovery phase of the geomagnetic
storms play an important role in the generation or inhibition of the ionospheric irregularities. Out of the 60 storms studied,
nearly 60 to 70% satisfied the categories I, II and III of Aarons’ criteria. However, in the remaining 30 to 40% of the cases,
no consistent results were observed. Thus, there is a necessity for further investigation of the effect of geomagnetic storms
on ionospheric irregularities, particularly with reference to the altitude variations of the F-layer (h’F) relating to the
changes in the local electric fields. 相似文献
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Fractal dynamics of geomagnetic storms 总被引：1，自引：1，他引：0
Naïma Zaourar Mohamed Hamoudi Matthias Holschneider Mioara Mandea 《Arabian Journal of Geosciences》2013,6(6):1693-1702
We explore fluctuations of the horizontal component of the Earth’s magnetic field to identify scaling behaviour of the temporal variability in geomagnetic data recorded by the Intermagnet observatories during the solar cycle 23 (years 1996 to 2005). In this work, we use the remarkable ability of scaling wavelet exponents to highlight the singularities associated with discontinuities present in the magnetograms obtained at two magnetic observatories for six intense magnetic storms, including the sudden storm commencements of 14 July 2000, 29–31 October and 20–21 November 2003. In the active intervals that occurred during geomagnetic storms, we observe a rapid and unidirectional change in the spectral scaling exponent at the time of storm onset. The corresponding fractal features suggest that the dynamics of the whole time series is similar to that of a fractional Brownian motion. Our findings point to an evident relatively sudden change related to the emergence of persistency of the fractal power exponent fluctuations precedes an intense magnetic storm. These first results could be useful in the framework of extreme events prediction studies. 相似文献
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地磁场模型的计算和评述 总被引：1，自引：0，他引：1
评述了计算地磁场区域模型的各种数学方法,如:利用多项式方法可以计算地磁场的Taylor多项式模型和Legendre多项式模型,利用球冠谐和分析方法可以计算出磁场的冠谐模型。本文指出了建立区域模型各种方法的优缺点,指出球冠谐和分析方法是计算地磁场三维模型的好方法。 相似文献
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在研究磁异常时,习惯将正常地磁场从测得的地磁场值中消除,以便突出上地幔和地壳内的各种磁异常。正常地磁场的选择正确与否,直接影响到人们对磁异常的认识及地质现象的研究。对于大面积的航空磁测编图,正常地磁场的选择尤为重要。 相似文献
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地磁总强度梯度的计算与分析 总被引：2，自引：0，他引：2
不仅要知道地磁场的分布规律,而且要知道地磁场梯度的分布规律。本上根据地磁场的高斯理论和地磁场的球谐模型,计算出中国及其邻近地区地磁总强度的水平梯度(南北方向和东西方向)和垂直梯度,绘制出相应的等值线图,并分析了总强度梯度的分布规律。地磁总强度的水平梯度和垂直梯度,主要随纬度变化,与经度关系不大。值得注意的是在我国的中心地区,地磁总强度的水平梯度值最大。 相似文献