地面磁测数据正常场改正现行方法探讨

地面磁测数据正常场改正是地面磁测工作资料整理的一个不可或缺的步骤。正常场改正的好与坏、对与错,改正的程度如何,都直接关系到磁异常的形态,以至于磁测工作的解释结果。本文通过讨论国际地磁参考场的求法、地面磁测工作正常场的改正意义,比较了国际地磁参考场与地磁图的精度,对现行的地面磁测数据正常改正的方法探讨后,通过工作实例说明...     

地磁场模型的计算和评述

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。     

Optimization fitting of the eccentric dipole models to the observed geomagnetic field

We have obtained formulas to calculate the field components of an eccentric dipole (ED) with an arbitrarily directed moment from specified coordinates of the dipole center and from its moment vector. With these formulas, the model dipole position was fitted to the observed geomagnetic field, and the approximation accuracy was estimated according to the standard deviation from IGRF along the X, Y, and Z components; the fitting procedure was checked in several tests.We computed the ED parameters (position and moment orientation) and harmonic coefficients of the ED field for 50 years using surface IGRF components, discovered some changes, and compared them with those according to the Schmidt eccentric dipole model. It was found that the nondipolar contributions to the geomagnetic field increase as the dipole field decays with time, and the dipole center drifts northand eastward away from the Earth's gravity center.The main contribution of the dipole part in the Gaussian spherical harmonic expansion of the geomagnetic field turned out to come from the terms with n of 1 to 5 rather than from two first terms, and the contribution of higher harmonics increases with time. Therefore, the Schmidt ED approximation based on the first eight Gauss coefficients (n ≤ 2) must have only relative significance indicating changes of the parameters. On the other hand, world magnetic anomalies (WMA) show up already in two first Gauss terms rather than since the third term as it has been commonly assumed.     

1600-2000年地球主磁场的全球变化

根据汤普森（Thompson）地磁场模型和第 8代IGRF模型，计算了1600-2000年期间的偶极子磁场、非偶极子磁场、西向漂移和地磁功率谱等反映主磁场变化的主要参数，分析了各个参数的长期变化特征。主要结果是：400年来地磁场的偶极子磁矩持续减小，1800年以来磁心的位置快速离开地心向太平洋方向移动了291km；西向漂移有大约30年左右的周期；非偶极子磁场异常中，南大西洋正磁异常、非洲负磁异常和大洋洲负磁异常是1600年以来一直存在的 3个大型磁异常，东亚正磁异常和北美正磁异常是1700年后逐渐形成的，17世纪北太平洋地区存在强的正磁异常。     

A normal reference field for the Ionian sea area

The area of the Ionian sea, between Albania and the Southern Italian Peninsula, has been taken into account for the production of geomagnetic component maps. Data from the national Albanian and Italian magnetic repeat station networks have been merged, and normal reference fields in latitude and longitude, have been computed. Data processing, reduction procedures and comparisons with IGRF are presented.     

Integrated Geophysical Works on the Kozlovka Anomaly (Kaluga Region)

This work presents integrated geophysical studies that were carried out to identify the nature of the intense magnetic anomaly detected by the results of land surveying on the right bank of the Slushka River in the territory of the Yukhnovskii district of Kaluga Region. The comprehensive interpretation of the geophysical data and the laboratory measurements of the core made it possible to determine the nature and parameters of the anomaly-forming object that is located in the upper part of the section; it consists of loams that contain such magnetic minerals as greigite, pyrrhotite, and magnetite.     

Experimental Verification and Research for the Distortion in the Integrated Frequency Responses of the High-Pressure Sealed Cabin and Magnetic Field Sensor

Although magnetotelluric sounding method applied to the land is advanced, there are many difficulties when it is applied to marine environment, one of which is how to lay magnetic field sensors down to the seafloor to complete measurements. To protect the magnetic field sensors from intense erosion and high pressure, suitable high-pressure sealed cabins must be designed to load them. For the consideration of magnetic measurement and marine operation, the sealed pressure cabin should be nonmagnetic and transportable. Among all optional materials, LC4 super-hard aluminum alloy has the highest performance of price/quality ratio to make the sealed pressure cabin. However, it does not mean that the high-pressure sealed cabin made using LC4 will be perfect in performance. In fact, because of its weak magnetism, the pressure cabin made using LC4 has distorting effect on frequency responses of the magnetic field sensors sealed in it. This distorting effect does not affect the use of the magnetic field sensor, but if we want to eliminate its effect, we should study it by experimental measurements. In our experiment tests, frequency sweep magnetic field as excitation signal was used, and then responses of the magnetic field sensor before and after being loaded into the high-pressure sealed cabin were measured. Finally, normalized abnormal curves for the frequency responses were obtained, through which we could show how the high-pressure sealed cabin produces effects on the responses of the magnetic field sensor. Experimental results suggest that the response distortion induced by the sealed pressure cabin appears on mid- andhigh-frequency areas. Using experimental results as standardization data, the frequency responses collected from seafloor magnetotelluric measurements can be corrected to restore real information about the seafloor field source.     

Analysis of geomagnetic field along seismic profile P4 of the International Project POLONAISE'97

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.     

New data on the structure of the Kas Block in the basement of the West Siberian Plate

A new concept concerning the structure and stages of evolution of the Kas Block of the West Siberian Plate is stated in this paper. The Kas Block is traditionally considered to be a subsided western margin of the Siberian Platform. The new concept is based on the results of the interpretation of the geophysical data recently obtained along the reference and regional profiles in this territory. The geological interpretation of the deep dynamic sections obtained by reprocessing of the CDP seismic reflection records has been performed for the first time. The structural features of the Kas Block, as well as the character of its junction with the Siberian Platform and the Paleozoic framework, are discussed. The tectonic scheme of the territory and the scheme of the pre-Late Devonian surface of the Kas Block have been compiled. The Baikalian age of the basement of the Kas Block is substantiated. The Salairian allochthonous ophiolite-basalt tectonic nappe is localized for the first time within the sedimentary cover of the Kas Block. The available information allowed us to reconstruct the development of the western margin of the Siberian continent in the Riphean and Early Paleozoic before and after the Baikalian Orogeny, respectively. The informational background of the geological and geophysical interpretation involves the results of the CDP seismic reflection profiling, including the deep dynamic seismic sections and parameters of the P-wave velocities along the reference 1-SB seismic line and the regional Vostok 10, 12, 15, and 16 seismic lines; the results of the deep seismic and magnetotelluric soundings; the gravity measurements; the magnetic exploration; and the new coherent physical geological models.     

高压密封舱与磁场传感器的综合频响变异及其实验验证

大地电磁测深在陆地上的方法技术成熟, 但将其移植到海洋中却遇到了较多的技术问题.其中之一是如何将磁场传感器运抵海底实施测量.为抵御海水的侵蚀和抗衡海下的环境压力, 需要研发装载磁场传感器的密封舱.该舱体需满足测磁的技术要求, 即制造材料的非磁性, 且兼顾海洋作业设备轻便的特点.LC4超硬铝合金在可选的材料中性价比居高, 然而用它制成的高压密封舱并非十分完美.因它的弱磁性, 使得磁场传感器装入舱体后, 整体频率响应发生了部分变异.这种变异虽不影响磁场传感器的使用, 但要对其规律特征予以测定, 方能剔除由此产生的对磁场测量的不良影响.在所构思的实验装置中, 通过人为产生扫频磁场, 对密封和非密封条件下的磁场传感器进行激励.在响应输出端, 测取幅频特性和相频特性, 获得归一化的对比资料和频响异常曲线, 从而对密封前后磁场传感器的性能变化有较清楚的认识.实验结果揭示, 由高压密封舱引起的频响变异发生在中高频区段.实验数据可作为标定资料, 对海底大地电磁探测的实测信号进行校正后, 即可还原出真实的海底场源信息.      

EMM2010模型在中国大陆的精度评估及其适用性

基于我国大陆最新观测所得的1 302个地磁测点和32个地磁台站磁偏角D、磁倾角I、总强度F的1 334组准确数据,并结合地壳磁异常能谱变化特征,对增强地磁模型(EMM2010)在我国大陆的精度及其适用性进行了定量分析。结果表明：EMM2010模型(D、I、F)在我国大陆的总体精度分别为10.45′、8.08′、112.85 nT  ;东北、华北与新疆地区模型的精度为13.07′、8.90′、130.89 nT ;华南、青藏高原及其东缘地区模型的精度为7.07′、6.65′、81.84 nT;其精度是受模型有限的截断阶数、各区域的磁异常状况和磁测数据的误差等因素共同影响的。EMM2010模型的精度在我国大陆表现出显著的地域分布特征,与磁异常的分布形态及其复杂程度、梯度密切相关,异常越突出,形态越复杂,模型的精度越低。与世界地磁模型(WMM2010)、第11代国际参考地磁场(IGRF11)相比,EMM2010模型在我国大陆的总体精度平均提高了50%,主要原因是模型不仅包含了地球主磁场,同时还包含了地壳磁场。EMM2010模型应用于我国大陆的实例及精度分析表明,模型具有一定的适用性,但有其局限性,不能准确反映出我国大陆的地磁场信息,鉴于模型的精度,建议在EMM2010模型基础上,结合我国最新的各部门的高精度磁测数据,构建我国高精度的地磁场模型。     

The hungarian magnetic network and the processing of the obtained data

In 1994–1995 a geomagnetic survey was carried out on the territory of Hungary and the neighbouring regions on 195 stations. Magnetic declination, inclination and total field were directly observed. Some of the stations were measured jointly with Istituto Nazionale di Geofisica (ING), Roma. The results were reduced to the epoch of 1995.0. Normal fields for the magnetic components were determined as second order functions of the geographic coordinates. The polynomial coefficients have been computed in three different ways: by means of simple and weighted least squares procedure and using the adjustment according to the “most frequent value”. In the present paper the mathematical foundation of these methods and the comparison between the obtained results will be presented.     

Magnetic field observations of the Sabzevar ophiolitic complex of northeast Iran

Surface measurements of the total magnetic field intensity along three sections transverse to the structural trends of the Joghatay Mountains ophiolitic complex extended north and west of Sabzevar, northeast Iran, are analyzed. The observed variations of the magnetic field intensity are compared with the synthetic results computed for a block structure consisting of several east-west oriented vertical parallelepiped down to 10 km depth which is also in agreement with the mapped shallow structural features of the complex. Shoaling of the basement and/or Curie surface may explain the observed northward decrease of the mean field measurements. However, in this study the variations are modeled in terms of magnetic enrichment of southern blocks.     

地面高精度磁法在新疆哈密地区磁铁矿勘查中的应用

利用地面CZM-3质子磁力仪,对新疆哈密某地区进行了1:1万高精度磁法测量.在此基础上,着重阐释哈密某地区磁场结构及其地质意义,编制出这一地区成矿构造地质图.根据磁铁矿与辉绿岩脉的关系,都具有磁性的特点,进行间接找矿.辉绿岩属于基性岩,具有强磁性,这与磁铁矿相同,单一的磁法原本不能解决问题,但从地质上考虑磁铁矿与辉绿岩...     

Variations of the dipole magnetic moment of the sun during the solar activity cycle

Observations of the large-scale solar magnetic field (synoptic maps) and measurements of the magnetic field of the Sun as a star (the total magnetic field) are used to determine the dipole magnetic moment and direction of the dipole field for three successive solar cycles. Both the magnetic moment and its vertical and horizontal components vary regularly during the cycle, but never disappear completely. A wavelet analysis of the total magnetic field shows that the amplitude of the 27-day variations of this field is very closely related to the magnetic moment of the horizontal dipole. The reversal of the global dipole field corresponds to a change in the inclination of its axis and occurs in a series of steps lasting one to two years rather than continuously. Before the onset of the reversal, the dipole axis precesses relative to the solar rotational axis, then shifts in a meridianal plane, reaching very low latitudes, where a substantial shift in longitude then begins. These results are discussed in connection with helioseismological data indicating the existence of oscillations with a period of about 1.3 yr and properties of dynamo processes for the case of an inclined rotator.     

Magnetic and ground probing radar measurements for soil pollution mapping in the industrial area of Val Basento (Basilicata Region, Southern Italy): a case study

The joint application of electromagnetic techniques for near-surface exploration is a useful tool for soil pollution monitoring and can also contribute towards describing the spatial distribution of pollutants. The results of a geophysical field survey that was carried out for characterizing the heavy metal and waste disposal soil pollution phenomena in the industrial area of Val Basento (Basilicata region, Southern Italy) are presented here. First, topsoil magnetic susceptibility measurements have been carried out for defining the spatial distribution of superficial pollution phenomena in the investigated area. Second, detailed and integrated measurements based on a high-resolution magnetic mapping and ground probing radar (GPR) profiling have been applied to investigate the subsurface in two industrial areas located in more polluted sites that were identified during the first phase. Our monitoring strategy discloses the way to rapidly define the zone characterized by high pollution levels deriving from chemical industries and traffic emissions and to obtain the way information about the presence of local buried sources of contamination.     

Discovery of an ancient pharaoh’s temple on the Horus military road, Northern Sinai, Egypt

Detailed geophysical measurements have been carried out in the northwestern part of the Sinai Peninsula. This area was mainly used by the ancient Egyptian army forces to support the trading and mining trips to Sinai and Asia. The geophysical field work aimed to discover new buried archeological remains using the efficient archeogeophysical detailed and nondestructive methods including total magnetic field, vertical magnetic gradient, and very-low-frequency electromagnetic measurements. Results of the field geophysical measurements have led to a discovery of a temple which is located on the Horus military road. This discovery has been verified by an excavation program, under the supervision of the Supreme Council of Egyptian Antiquities, where buried remains of a pharaoh’s temple were detected and photographed. Some other sites were recommended for further excavation in the future.     

Determining the spatial configurations of the coronal magnetic fields of solar active regions

The fundamental possibility of reliably removing the π ambiguity from the transverse magnetic field detected in solar vector magnetographic measurements, independent of the location of the vector magnetograms on the solar disk is demonstrated. The corrected magnetograms are then used as boundary conditions for the reconstruction of the three-dimensional magnetic field. The calculated field lines agree well with observed non-potential magnetic loops. The π ambiguity is removed using a modified Metropolis algorithm adapted to a spherical geometry. The spatial configuration of the magnetic field is calculated in a nonlinear force-free approximation using an optimization method. Tests of the new algorithm for resolving the π ambiguity are demonstrated for various model cases and comparisons with results of the NPFC method.     

亚东—格尔木地学断面区域磁异常数据处理与地体划分

本文首先介绍了航磁数据的预处理；介绍了视磁化率填图方法及对浅层、深层视磁化率进行了综合分析，进行了方向滤波及长波磁异常的分析处理，讨论了航磁数据图象处理及其有关向题，最后提出了地体划分意见：由5条边缘断裂分割成６个地体。