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1.
Analytical models of the palaeomagnetic field have been constructed for a number of geological periods (Quaternary Neogene, Jurassic, Triassic, Permian and Permo-Carboniferous) by spherical harmonic analysis using the present-day world map as a basis and (for the earlier periods) using also a palaeogeographic reconstruction. The use of the palaeogeographic chart for the earlier periods simplifies the models, and its use appears to be valid. The low accuracy, small number and uneven distribution of palaeomagnetic data severely limit the conclusions which can be drawn from the analyses. Nevertheless the results for all periods indicate that throughout the past 300 million years the geomagnetic field has maintained its global structure, and has remained similar to the field of a dipole slightly shifted from the Earth's centre. It appears that there have not been any persistent systematic anomalies or variations in the Earth's magnetic field throughout that time, but rather that the field has been oscillating around a mean level not greatly different from that of the present epoch.  相似文献   

2.

Synchronous annual variations in the geoelectric and geomagnetic field are studied on the basis of long-term electromagnetic monitoring. It is shown that the annual geoelectric variations have intraterrestrial origin and are not related to the annual geomagnetic variations. Temporal variations in the magnetotelluric impedance and magnetic tipper, which characterize the electrical conductivity of the geological environment, are analyzed. It is established that annual variations in the magnetotelluric impedance mainly describe the variations in the electrical conductivity of surface crustal layers and are less sensitive to the deep electrical conductivity of the Earth. The annual variations in the imaginary magnetic tipper at the periods of 1000–3000 s probably reflect the changes in conductivity of a deep transversal low-resistive zone (the fault). It is suggested that annual variations in the geoelectrical and geomagnetic fields, as well as in the electrical conductivity of the geological environment, arise as a response to the changes in the geodynamical processes caused by the revolution of the Earth around the Sun.

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3.
地磁正常场的选取与地磁异常场的计算   总被引:34,自引:8,他引:26       下载免费PDF全文
根据2003年中国地磁观测数据(包括135年地磁测点和35个地磁台)以及我国邻近地区38个IGRF计算点的地磁数据,计算中国地磁异常场的分布。选取两种地磁场模型作为地磁正常场,一是国际参考地磁场的球谐模型,二是中国地磁场泰勒多项式模型。根据各个测点的地磁异常值(观测值减去模型计算值),用球冠谐分析方法计算地磁异常场的球冠谐模型,并绘制2003年中国地磁异常(△D,△I,△F,△X,△Y,△Z)。分析和讨论了中国地磁异常场。  相似文献   

4.
本文概略地介绍了第四纪沉积地层古地磁学研究的基本原理、野外采样及实验方法。文中综合对比了我国近几年来测量的十一个地层剖面和五个钻孔剖面的结果,并对第四系底界(Q_1与N_2)以及Q_1与Q_2年代界限进行了初步讨论  相似文献   

5.
利用玉树地震前玉树周围500 km范围内的地磁观测数据,采用地磁垂直分量加卸载响应比、地磁垂直分量日变化幅度逐日比、地磁垂直分量日变化空间相关、低点位移等方法讨论了震源区地磁场变化与地震的相关性,并发现它们之间有较好的对应关系。  相似文献   

6.
When re-heated to temperatures below the Curie temperature and subsequently cooled in a constant magnetic field (H T), rock samples which contain magnetic minerals can acquire an induced magnetic anisotropy (IMA). As the result of acquiring the IMA, a constriction develops in the hysteresis loop of the magnetization of these rocks at the values of the magnetizing field close or equal to the HT. Thus the IMA is capable of retaining the information on the palaeointensity of the geomagnetic field, i.e., if IMA was created in a rock in the geomagnetic field in a past geological epoch, it preserves the information on the intensity of that field. Investigations have shown, that when IMA is created in a rock under external stress, the stress has an impact on the magnetic memory. Here we also deal with the issue of how stress affects the magnetic memory of IMA. A mathematical model for the effect of stress on magnetic memory phenomena related to induced magnetic anisotropy in rocks containing multidomain magnetite and titanomagnetite grains is proposed herewith. The effect of temperature on the magnetic memory of rocks is discussed also.  相似文献   

7.
The works on paleomagnetic observations of the dipole geomagnetic field, its variations, and reversals in the last 3.5 billion years have been reviewed. It was noted that characteristic field variations are related to the evolution of the convection processes in the liquid core due to the effect of magnetic convection and solid core growth. Works on the geochemistry and energy budget of the Earth’s core, the effect of the solid core on convection and the generation of the magnetic field, dynamo models are also considered. We consider how core growth affects the magnetic dipole generation and variations, as well as the possibility of magnetic field generation up to the appearance of the solid core. We also pay attention to the fact that not only the magnetic field but also its configuration and time variations, which are caused by the convection evolution in the core on geological timescales, are important factors for the biosphere.  相似文献   

8.
安宁河断裂带晚第四纪活动的基本特征及强震危险性分析   总被引:7,自引:0,他引:7  
通过影像解译,结合野外地质调查,利用第四纪地貌填图、样品采集和差分GPS地貌面的测量等研究手段,对安宁河断裂带及其附近地区第四纪地貌特征与断层活动关系进行了研究,分析了安宁河断裂带晚第四纪以来的活动特征,探讨了该断裂上强震的危险性。结果表明,晚第四纪以来,安宁河断裂带有强烈左旋走滑和逆冲的双重运动特征,由此可将其划分为南、北两段,北段最后一次活动时间大约在公元15世纪,南段最后一次活动时间为1536年。安宁河断裂带北段的强震危险性大于南段,且未来地震的强度在7.5级左右。  相似文献   

9.
Recent studies have shown that, in addition to the role of solar variability, past climate changes may have been connected with variations in the Earth??s magnetic field elements at various timescales. An analysis of variations in geomagnetic field elements, such as field intensity, reversals, and excursions, allowed us to establish a link between climate changes at various timescales over the last millennia. Of particular interest are sharp changes in the geomagnetic field intensity and short reversals of the magnetic poles (excursions). The beginning and termination of the examined geomagnetic excursions can be attributed to periods of climate change. In this study, we analyzed the possible link between short-term geomagnetic variability (jerks) and climate change, as well as the accelerated drift of the north magnetic pole and surface temperature variations. The results do not rule out the possibility that geomagnetic field variations which modulate the cosmic ray flux could have played a major role in climate change in addition to previously induced by solar radiation.  相似文献   

10.
磁线圈对地磁场的物理模拟及对地磁导航研究的意义   总被引:1,自引:0,他引:1  
利用磁线圈对地球基本磁场开展动态模拟,将地磁场随空间的变化转化为在实验室中随时间的变化,能够为地磁导航系统的匹配试验提供物理仿真的地磁场环境。本项研究依照虚拟仪器技术思路,对磁线圈、恒流电源、磁通门磁力仪(或Overhauser磁力仪)和工控机进行数字化连接,并采用LabVIEW编程进行驱动控制,通过自动调节线圈绕组中的电流大小来实现对磁场的物理模拟并进行实时监测,尝试组建了地磁场动态模拟系统,并分别开展了对地磁场总强度和三分量信号的动态模拟实验。模拟系统可以实现天然地磁场和人工编制两种动态信号的输出模拟,且拟合效果良好。地磁场动态模拟系统的初步建立为今后地磁匹配试验等研究提供了仿真磁场环境。  相似文献   

11.
实地调查表明,山西长治断裂由三段组成,南段和中段为西倾正断层,北段为东倾正断层,总体走向北东25o,长达65km,控制着附近山地与第四纪山间盆地的构造演化和地貌发育;第四纪早期,断裂发生强烈的垂直差异活动,最大垂直活动幅度可达400m左右;第四纪晚期,断裂活动性明显减弱,中段仍有活动,至少发生过两期活动,第—期活动发生于距今10.88万年左右或以后、1.49万年以前,第二期活动发生于距今1.49万年以后,垂直错距0.65m。  相似文献   

12.
陈化然  蒋邦本 《中国地震》1998,14(2):131-139
本文利用1950-1995年长达45年的地磁资料,建立了中国地磁基本场时空变量统一模式。然后,又以此模式场作为正常场,计算出1970年中国地磁异常场,并与地质构造相比较,发现二者有着密切的关系。  相似文献   

13.
Preliminary paleointensity results are presented from 36 sites with virtual geomagnetic pole (VGP) latitudes of about 30–90° normal polarity in the Quaternary West Eifel volcanic field. A strong correlation between VGP latitude and the Earth's virtual magnetic dipole moment (VDM) is observed, with low intensities for low VGP latitudes indicating possibly an emplacement during an excursion or event of the Brunhes epoch. The age distribution of the West Eifel volcanics is, as yet, poorly known. Also, the mean VDM value for sites with high VGP latitudes is considerably lower than the present day dipole moment of the Earth.  相似文献   

14.
The sources of geomagnetic disturbances during 1999–2003 are discussed. The relation between geomagnetic activity and the rate of coronal mass ejections (CMEs), their parameters, and the dynamics of solar photospheric magnetic fields is considered. It is shown that during the reorganization of unipolar regions of the photospheric magnetic field, the number of CMEs increases and their parameters change. The geomagnetic disturbance level also increases in these periods.  相似文献   

15.
1690~2000年地磁场能量的三维分布及其长期变化   总被引:1,自引:0,他引:1       下载免费PDF全文
利用Bloxham & Jackson 地磁场模型和国际参考地磁场模型(IGRF),研究了1690~2000年地磁总能量及其北向、东向和垂直向分量的能量以及非偶极子磁场的能量在地球内部的分布及长期变化.结果表明,地表和地核以外地磁场总能量及其北向和垂直向的能量是持续衰减的,垂直向的磁场能量占总能量的64%以上,对总能量的贡献起主要作用;东向分量的能量随时间的变化以增加为主.地磁场的能量变化率存在56年的周期,主要是由偶极子磁场产生的.地表以外的非偶极子磁能从减小到增大转折出现在1770年,比地核以外滞后40年.地球内部磁能随时间的变化显示,偶极子磁能逐渐减小,非偶极子磁能增加,越靠近核幔边界增加越快;偶极子和非偶极子磁能的变化量相等的分界面在距地心3780km处.从核幔边界到地表,磁能变化的衰减非偶极子比偶极子快,表明偶极子磁场比非偶极子磁场有更深的场源.  相似文献   

16.
利用重磁反演软件,对2017年8月冀鲁豫交界区流动地磁总强度数据进行处理并解析延拓,研究该区岩石圈磁场及其深部、浅表磁场异常分布特征与地下介质磁化率结构的性质。结果表明:冀鲁豫交界区岩石圈磁场异常分布是岩石圈浅表与深部磁异常综合叠加的结果,岩石圈地下介质的浅表与深部磁化率结构具有一定差异性,且受断裂控制呈分段性特征,可能与该区域复杂的岩石圈磁化率结构及地质构造有关。  相似文献   

17.
地磁场磁力线切割海水和电磁感应两种方式的共同作用影响着海水介质中变化地磁场的时空特征.虽然近些年的野外实践、数值模拟和理论研究都表明,海面和深海海底的变化磁场存在差异,但极少有实测数据揭示在海水介质不同深度位置地磁场的时空特征.本文主要介绍在南海西南次海盆4366 m深度处布放和回收了一个4000 m长深海地磁观测潜标的科学实验;重点分析垂直方向不同水深位置上地磁场观测记录中总强度的变化幅度及相位的时空特征.并通过建立地磁场太阳静日变化模型,将观测结果与南海周缘的三个地磁台站观测记录进行对比分析.研究结果表明,地磁场总强度在深海水体的不同深度存在着显著差别.在地磁扰动较小或平静期间,深海潜标处的日变形态与同纬度邻近台站的观测结果较为一致;而在地磁扰动期间,由于所处位置处地下电性介质的差异会对感应磁场产生不同的影响,观测到的总强度在幅度和相位变化中也出现相应的不同.本文的分析结果不仅为海水介质不同深度地磁场时空特征的研究提供了科学实验依据,也为海洋磁测中地磁日变观测站的布设提供建议.  相似文献   

18.
Reversals and excursions of Earth's geomagnetic field create marker horizons that are readily detected in sedimentary and volcanic rocks worldwide. An accurate and precise chronology of these geomagnetic field instabilities is fundamental to understanding several aspects of Quaternary climate, dynamo processes, and surface processes. For example, stratigraphic correlation between marine sediment and polar ice records of climate change across the cryospheres benefits from a highly resolved record of reversals and excursions. The temporal patterns of dynamo behavior may reflect physical interactions between the molten outer core and the solid inner core or lowermost mantle. These interactions may control reversal frequency and shape the weak magnetic fields that arise during successive dynamo instabilities. Moreover, weakening of the axial dipole during reversals and excursions enhances the production of cosmogenic isotopes that are used in sediment and ice core stratigraphy and surface exposure dating. The Geomagnetic Instability Time Scale (GITS) is based on the direct dating of transitional polarity states in lava flows using the 40Ar/39Ar method, in parallel with astrochronologic age models of marine sediments in which oxygen isotope and magnetic records have been obtained. A review of data from Quaternary lava flows and sediments gives rise to a GITS that comprises 10 polarity reversals and 27 excursions that occurred during the past 2.6 million years. Nine of the ten reversals bounding chrons and subchrons are associated with 40Ar/39Ar ages of transitionally-magnetized lava flows. The tenth, the Gauss-Matuyama chron boundary, is tightly bracketed by 40Ar/39Ar dated ash deposits. Of the 27 well-documented geomagnetic field instabilities manifest as short-lived excursions, 14 occurred during the Matuyama chron and 13 during the Brunhes chron. Nineteen excursions have been dated directly using the 40Ar/39Ar method on transitionally-magnetized volcanic rocks and these form the backbone of the GITS. Excursions are clearly not the rare phenomena once thought. Rather, during the Quaternary period, they occur nearly three times as often as full polarity reversals.  相似文献   

19.
The effects of the dayside and dusk plumes of the plasmasphere during the ring current recovery phase on the disturbance level of the ground geomagnetic field horizontal component have been considered. It has been indicated that the geomagnetic field horizontal component changes specifically and synchronously in the region corresponding to the plasmaspheric dayside plume. Outside the plume the time variations in the geomagnetic field horizontal component pronouncedly differs. A spectral analysis of disturbances in the geomagnetic field horizontal components in the range of geomagnetic pulsations indicated that the intensity in the range of Pc4 pulsations increases at magnetic stations located on field lines corresponding to the dayside and dusk plumes of the plasmasphere. These pulsations detected in the dynamic spectrum of the geomagnetic field horizontal components in the dayside plume region of the plasmasphere, probably reflect the resonance oscillations of magnetic field lines in the region of field-aligned currents at comparatively low altitudes. We assume that this is caused by the instability of field-aligned currents originating as a result of the interaction between the ring current energetic ions and electromagnetic waves in the region with a relatively dense background plasma of the dayside plume.  相似文献   

20.
地球磁场多次发生南北(正负)磁极位置的变换和白垩纪超静磁带(CNS)的异常现象,这已为大家所公认.但造成这种异常现象的原因,则是迄今未能很好解答的一个难题. 应用非线性理论对地球磁极倒转和白垩纪超静磁带进行了分析, 认为超静磁带事件意味着地球核幔相互作用和外核流体运动可能处于能量最低的状态,地球磁场系统通过不断地与外界交换物质和能量,维持一种空间或时间的有序结构.在121~83Ma期间,无外星撞击地球引起地磁极性倒转,可能是白垩纪超静磁带出现的原因之一.地球磁场极性的随机倒转具有混沌运动的自逆转特性,混沌理论给地磁极性倒转提出了一个简明的动力机制解释.  相似文献   

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