X地磁垂直分量日变幅逐日比及其与地震关系的探讨   总被引：8，自引：1，他引：8  

冯志生  王建宇  蒋延林  吴晶  梅卫萍 《华南地震》2001,21(2):20-27

分析了地城关垂直分量日变幅逐日比值的高值异常与其后地震的关系，发现它们之间有良好的对应，通过分析地磁垂直分量谐波幅度的逐日比，作者认为这种高值变化可能与其间地下介质电阻率下降有关，但也有可能是是外场变化所致。  相似文献   

地磁场模型和冠谐分析   总被引：4，自引：2，他引：4  

安振昌 《地球物理学进展》1992,(3)

地磁场是由内源场(地核场和地壳场)和外源场(电离层场和磁层场)组成的,地磁场模型是表示地磁场时空分布的数学表达式.本文简述了地磁场全球模型和区域模型的计算方法和应用;评述了冠谐分析方法及其在地磁学中的应用;介绍了地磁场模型误差的主要来源.  相似文献   

中低纬地区地磁脉动的研究   总被引：1，自引：0，他引：1  

杨少峰 《地震地磁观测与研究》1992,13(1):50-57

近年来我们对中低纬地区地磁脉动进行了大量的观测和研究。本文不仅介绍了观测仪器的设计、台网设置及数据处理方法。而且还简要地介绍了一些主要科研成果,如低纬Pc3脉动特点,低纬Pi2脉动偏振特性。南极地区的地磁脉动观测结果,以及在磁暴和太阳耀斑期间在低纬地区观测的地磁脉动。这对于进一步认识中低纬地区地磁脉动是十分有益的。  相似文献   

中国地磁台环境场的计算与分析   总被引：1，自引：0，他引：1  

安振昌  李家发  吴一柱  王月华  谭东海 《地震地磁观测与研究》1992,(6)

根据国际参考地磁场(IGRF)模型,计算出1945年5月—1990年5月中国部分地磁台的计算年均值,并与相应观测年均值比较,计算出地磁台各个地磁要素的磁异常值以及地磁台异常场的模量,本文的计算结果将为认识地磁台的地磁场环境、地磁台站资料评比提供依据。  相似文献   

地磁场水平梯度的计算与分析   总被引：4，自引：0，他引：4  

安振昌 《地球科学进展》1992,7(1):39-43

In this paper，based on the Gauss theory of geomagnetism and the spherical harmonic mi}del of the geomagnetic field，the horizontal gradients of the geomagnetic field in north一south and west-;east dlrections were calculated in Chinese and"its surrounding regions, the contour maps of the horizontal gradients of the geomagnetic components were constracted，and its regularities of distributions were analysed.
The horizontal gradients of the total intensity (F)，horizontal intensity (H) and vertical intensity (Z ) vary mainly with lat相似文献   

Equatorial and low latitude ionosphere during intense geomagnetic storms   总被引：1，自引：0，他引：1  

G.A. Mansilla   《Journal of Atmospheric and Solar》2006,68(18):2091-2100

An investigation is made in order to analyse the role of neutral gas composition in the equatorial and low latitude ionosphere during intense geomagnetic storms. To this end data taken by the Dynamic Explorer 2 satellite at 280–300 km (molecular nitrogen N₂ and atomic oxygen O concentrations, electron density and vertical plasma drifts) are used. The sudden commencements of the events considered occurred at 11:38 UT on March 1, 1982, 18:41 UT on November 20, 1982 and 16:14 UT on February 4, 1983. Vertical plasma drifts are the most important contributor to the initial storm time response of the equatorial F region. Neutral composition changes (expressed as an increase in the molecular species, mainly N₂) possibly play a predominant role in the equatorial and low latitude (10–20°) decreases of electron density at heights near F2-region maximum during the main and recovery phases of intense geomagnetic storms. Delayed increases of electron density observed at daytime during the recovery phase may be also attributed to increases in atomic oxygen. At low latitudes possibly a combined effect of O increase and upward plasma drift due to enhanced equatorward winds is the responsible mechanism for the maintenance of enhanced electron density values.  相似文献   

西安地区部分古遗址考古地磁研究          下载免费PDF全文

孟昭秦 《地质科学》1998,33(4):489-493

通过对陕西耀州窑遗址内4个古窑,临潼兵马俑一号坑,西铜一级公路经过黄堡工地开挖的两个五代窑,以及耀州窑博物馆仓库工地内开挖的一个金代窑和一个春秋窑遗址的古地磁研究,初步得出了西安地区古地磁场变化的规律,为鉴定从春秋到金代西安地区的古遗址、古文物提供了考古地磁学上的一个粗略的标准。  相似文献   

60年代末与70年代末中国4个地磁台处Jerk的分析   总被引：5，自引：0，他引：5       下载免费PDF全文

陈伯舫 《地球物理学报》1998,41(1):71-78

外场的影响可以通过一定的方法从地磁月均值中消除,本文用通日月均值资料分析了广州、余山、兰州和北京的Jerk的大小．结果显示,上述4台的X和Y分量都存在二次寻数阶跃．Z分量上Jerk不明显,只有兰州和北京台较易看出60年代末的Jerk．由于本文结果是尽量消除外场影响后的结果,又是中低纬度地区的结果,所以作者认为它可支持Jerk是源于地核的推论,而且认为应将60年代末的Jerk与70年代末的Jerk一并研究．  相似文献   

The Dependence of the Geoeffectiveness of Interplanetary Flux Rope on Its Orientation,with Possible Application to Geomagnetic Storm Prediction     

Yuming Wang  Pinzhong Ye  S. Wang 《Solar physics》2007,240(2):373-386

Interplanetary magnetic clouds (MCs) are one of the main sources of large non-recurrent geomagnetic storms. With the aid of a force-free flux rope model, the dependence of the intensity of geomagnetic activity (indicated by Dst index) on the axial orientation (denoted by θ and φ in GSE coordinates) of the magnetic cloud is analyzed theoretically. The distribution of the Dst values in the (θ, φ) plane is calculated by changing the axial orientation for various cases. It is concluded that (i) geomagnetic storms tend to occur in the region of θ<0°, especially in the region of θ≲−45°, where larger geomagnetic activity could be created; (ii) the intensity of geomagnetic activity varies more strongly with θ than with φ; (iii) when the parameters B ₀ (the magnetic field strength at the flux rope axis), R ₀ (the radius of the flux rope), or V (the bulk speed) increase, or |D| (the shortest distance between the flux rope axis and the x-axis in GSE coordinates) decreases, a flux rope not only can increase the intensity of geomagnetic activity, but also is more likely to create a storm, however the variation of n (the density) only has a little effect on the intensity; (iv) the most efficient orientation (MEO) in which a flux rope can cause the largest geomagnetic activity appears at φ∼0° or ∼ 180°, and some value of θ which depends mainly on D; (v) the minimum Dst value that could be caused by a flux rope is the most sensitive to changes in B ₀ and V of the flux rope, and for a stronger and/or faster MC, a wider range of orientations will be geoeffective. Further, through analyzing 20 MC-caused moderate to large geomagnetic storms during 1998 – 2003, a long-term prediction of MC-caused geomagnetic storms on the basis of the flux rope model is proposed and assessed. The comparison between the theoretical results and the observations shows that there is a close linear correlation between the estimated and observed minimum Dst values. This suggests that using the ideal flux rope to predict practical MC-caused geomagnetic storms is applicable. The possibility of the long-term prediction of MC-caused geomagnetic storms is discussed briefly.  相似文献   

Similarity of new palaeomagnetic data from the Santa Rosa Mountains with those from Steens Mountain gives wide regional evidence for a two-stage process of geomagnetic field reversal     

Neil Roberts  Mike Fuller 《Geophysical Journal International》1990,100(3):521-526

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