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1.
最新的岩石圈磁场模型及中国磁异常特征的几点认识   总被引:1,自引:0,他引:1  
介绍了最新的地球磁场模型,包括MF5,NGDC-720和WDMAM。模型MF5是由CHAMP卫星测量得来,它的球谐展开阶次为n=16~100,对应的波长段为400~2500km。模型NGDC-720和WDMAM是综合了卫星磁测、航空磁测、海洋磁测与地面磁测得到数据经过处理后得来,它们有不同的球谐阶次和分辨率。NGDC-720模型是由美国国家地球物理数据中心(The National Geophysical Data Center,NGDC)提供,它的球谐阶次从16阶到720阶,对应于由2500km到56km的波带。M.Purucker博士公布的WDMAM参考模型1是一张分辨率为3′,高度位于WGS84上方5km的磁异常图,它向上延拓后的结果与MF5中的岩石圈磁异常保持一致。作者根据国际上公布的CHAMP、NGDC-720与WDMAM Candidate1的最新数据,绘制了中国及毗邻地区的磁异常图,对中国及毗邻地区明显的大地构造,如造山带,盆地等地区的磁异常特征进行了描述和分析,塔里木、四川、松辽等盆地地区及华北平原部分地区模型中均表现为正异常,西藏高原、天山造山带等地区表现为负异常,而一些深大断裂表现为磁异常高梯度带。通过四川盆地和西藏高原地区三个模型的相互对比,我们发现模型阶次越高,它所反映的磁性体(尤其是浅部地质体)的情况越丰富,不同的是四川盆地的结果随着阶次的增高就越接近航磁结果,而西藏高原随着阶次的增高却和航磁结果差别越来越大。  相似文献   

2.
Zhao  SK 许惠平 《世界地质》1991,10(3):39-50
由磁卫星(MAGSAT)资料绘制了中国区域磁异常图。资料首先分为拂晓和黄昏二组且对每一组分别进行处理。这二组数的各阶相关系数表明短波(≤540km)特征以非壳噪声为主。根据这二组数据中波长在540~2300km谐波得出了磁异常图。它代表了在卫星高度约400km处中国地壳磁异常,其幅值在—6~7nT之间。研究区域处于中、低磁纬度,磁异常并直不同接发因源相关。为克服这一困难,把磁异常图转化成反映地磁化率横向变化的地壳磁化率图。在反演中老虑了地磁场方向和强度的变化。该磁化率异常图呈现了区域构造,前寒武克拉通为强磁性,而山脉和缝合带为低磁性区。  相似文献   

3.
岩石圈磁场模型及其应用   总被引:1,自引:0,他引:1  
评介了一些重要的地球岩石圈磁场模型,包括根据CHAMP卫星数据制作的MF系列模型、综合模型CM、POMME系列模型、EMAM2网格数据集等.大力推荐Px Maule博士制作的全球磁性地壳厚度图和侯重初等人制作的中国大陆居里温度等温面图.建议充分利用卫星磁测数据和已开发的方法技术开展研究工作.  相似文献   

4.
划分重磁区域异常与局部异常的一种方法泛克立格法   总被引:2,自引:0,他引:2  
在重(磁)资料的分析处理中,经常需要划分区域异常与局部异常。本文对用于矿床品位预测的方法—泛克立格法加以改进、完善,使其适合于求重(磁)资料的区域异常与局部异常。根据某点周围若干个信息点上的重(磁)观测数据估计出该点处的区域异常值,而且这种估计是在满足线性、无偏、最小估计方差条件下求得的。从重(磁)观测数据中减去区域异常就可得到局部异常,这就是泛克立格法。它比经常用来划分区域异常与局部异常的方法—趋势分析方法有许多优点。趋势分析方法只是泛克立格法的一个特例。在本文中,作者还提出在小范围内,重力区域异常适合于用一次多项式拟合;而磁法区域异常适合于用二次多项式拟合的观点  相似文献   

5.
卫星磁测的过去·现在·未来   总被引:4,自引:2,他引:4  
张昌达 《物探与化探》2003,27(5):329-332
论述了卫星磁测的历史、现状和对未来的展望;介绍并对比了3颗磁卫星(Magsat,Oersted,CHAMP)和由它们测得的与中国大陆和海域大地构造单元有关的6个卫星磁异常.  相似文献   

6.
黑龙江大兴安岭地区航磁异常特征及找矿效果   总被引:1,自引:0,他引:1  
利用大兴安岭地区1:5万高精度航磁资料,结合区域地质背景分析了该区航磁异常特征,依据地物化资料、已知矿(床)点的分布及成矿规律筛选出了一批航磁异常.在最新的高精度航磁图上,已知铁矿异常特征明显,经对比研究及综合查证发现了1处磁铁矿点及多处有色金属、贵金属矿点,在此基础上总结查证经验,指出了今后采用航磁数据在区内的找矿方向.  相似文献   

7.
中国航磁调查已基本覆盖全国,尤其是近二十年来开展了大面积1∶5万高精度航磁调查,为铁矿的成矿规律研究及找矿预测提供了重要的基础数据。文章基于全国航磁编图(1∶100万)和大比例尺(≥1∶5万)航磁数据集,开展区域、矿集区、矿床3个不同尺度的研究,旨在总结4种主要类型铁矿在区域和局部磁场上的响应模式,指导找矿应用。研究表明,不同类型的铁矿在区域磁场上呈现出不同的特征,沉积变质型铁矿主要位于条带状磁异常边部负背景场中的局部高磁异常,岩浆型铁矿主要位于线性磁异常带,接触交代-热液型铁矿(矽卡岩型)主要沿带状或等轴状磁异常边缘分布,火山岩型铁矿通常沿带状磁异常分布。不同的区域磁异常特征通常反映了特定的控矿要素,主要刻画了火山-沉积建造、基性-超基性杂岩、中酸性侵入岩、火山岩由浅部至深部的分布特征,为成矿地质背景研究提供了大量深部信息。岩浆活动强烈的构造带,会导致地壳内基底隆起和较高的地温梯度,呈现出磁性基岩深度和居里面深度较浅的特征,有利于铁矿物的富集成矿。大比例尺航磁资料(≥1∶5万)大都能够直接反映矿体或含矿地质体的特征,磁异常都对应了铁矿体或矿化的中心,但矿体的规模、产状、埋深、品位等特征的变化都会造成磁异常幅值、形状、大小的变化,通过约束条件下2D和3D正反演计算获得深部矿体或含矿地质体的特征,对找矿勘查最具指导意义。概括来讲,中小比例尺航磁资料主要用于成矿地质背景研究,分析成矿控矿要素,达到区域成矿预测的目的。大比例尺航磁资料可用于隐伏矿体或含矿地质体预测,建立深部矿体或含矿地质体二维或三维模型,指导勘探工作。  相似文献   

8.
高精度航磁调查在新疆西天山地区的应用   总被引:2,自引:1,他引:1  
介绍了高精度航磁调查在西天山地区的应用效果,在高精度航磁图上,磁异常信息极为丰富,不仅已知铁矿在图上反映明显,而且还新发现了50余处铁矿异常,在已经进行了查证的5处异常中,有4处见矿,分别为14号、20号、169号和374号。这4处异常的成功发现不仅带来了巨大的经济效益,也为今后利用高精度航磁调查进行找矿提供了典型的实例。根据该区高精度航磁调查实际效果,笔者认为在新疆西天山地区,乃至整个中国西部勘查程度较低的地区,进行高精度航磁测量,并进行快速的地面查证工作,是寻找铁磁性矿产行之有效的方法。  相似文献   

9.
王亮  张应文  杨建辉 《贵州地质》2009,26(3):209-214,217
对1:5万高精度磁异常原始资料数据处理,进行化极、延拓计算7个不同上延高度异常,分析对比所有资料,结合地物化资料,对磁异常平面进行特征分区。又根据已知的白马洞(区内)-杉树林(区外)铅锌矿床成矿带及区内异处的铅锌、铜、锰等矿床(点)的成矿规律和分布特点,圈定了8个异常成矿靶区,19个大型的浅层局部负磁异常,均为有一定找矿意义的磁异常,并推测它们可能为岩体与矿致磁异常(铅锌、铜、锰、铁)等综合引起,在岩体(浅表隐伏的花岗岩珠或岩枝)与围岩接触带、层间破碎带上,应是赋矿的有利部位。  相似文献   

10.
通过对新疆卡克地区上石炭统别根他乌组105个岩石薄片进行显微镜下观察,识别出6种微相:MF1灰泥灰岩微相、MF2含生物碎屑灰泥灰岩、MF3生物碎屑粒泥灰岩、MF4含生物碎屑亮晶似球粒灰岩、MF5生物碎屑亮晶灰岩和MF6生物碎屑砾屑灰岩。根据微相组合类型,推断该地区在罗苏期至达拉期经历了台地-台地边缘浅滩及礁-台地边缘斜坡3种环境,整体为一个完整海侵-海退的过程。  相似文献   

11.
A new composite map of magnetic surface (MAGSURF) anomaly for Italy and its adjacent region has been derived from sea and ground surveys on the basis of an improved definition of the Italian Magnetic Reference Field and its temporal change. Spectral analysis of the MAGSURF anomaly field shows a regional scale energy in the wavelength range 145–500 km, due to the presence of various crustal sources. The regional MAGSURF anomaly map shows poor correlation with the corresponding MAGSAT scalar anomaly map, whose power spectrum reveals wavelength components in the range 300–700 km. The MAGSURF data are upward-continued to an elevation of 100 km for comparison with MAGSAT satellite data, downward-continued to the same altitude of 100 km and low-pass filtered for wavelengths larger than 500 km. Upward-continued surface data and downward continued satellite data show good morphological similarity for wavelengths in the range 300–500 km at an altitude of 100 km. Satellite data permit the characterization of magnetic signatures due to sources located in the middle-lower crust of Sardinia, Lombardia, Molise and Dalmatia, while further surface regional anomalies are connected with upper crust bodies of Mid Tyrrhene and East Sicily.  相似文献   

12.
Based on the MAGSAT magnetic anomaly fields over Europe and the adjacent areas spherical cap models have been derived. The method of spherical cap harmonic analysis, due to Haines (1985), has been applied for the modelling of the MAGSAT magnetic anomalies. The data set used in the analysis included the 1 ° × 1 ° gridded values of the MAGSAT anomaly fields between latitudes ϑ = 6 ° to 60 °N and longitudes λ = 19 °W to 70 °E. The pole of the cap is at ϑ = 33 °N and λ = 26 °E and its half-angle is 40 ° . The maximum index (Km) of the model is 18 and the total number of model coefficients is 361. A minimum wavelength corresponding to this index at the Earth's surface is ~ 1000 km. The RMS deviations between the calculated and observed values are ~ 4 nT for δX, ~ 3 nT for ΔY and 3,5 nT for ΔZ respectively. The spherical cap harmonic model was used for the construction of magnetic anomaly maps for all components and at different altitudes.  相似文献   

13.
Based on the CHAMP Magsat data set, spherical cap harmonic analysis was used to model the magnetic fields over China continent. The data set used in the analysis includes the 15′×15′ gridded values of the CHAMP anomaly fields (latitude φ=25°N to 50°N and longitude λ=78°E to 135°E). The pole of the cap is located at φ=35°N and λ=110°E with half-angle of 30°. The maximum index (Kmax) of the model is 30 and the total number of model coefficients is 961, which corresponds to the minimum wavelength at the earth's surface about 400 km. The root mean square (RMS) deviations between the calculated and observed values are ~ 4 nT for ΔX, ~ 3 nT for ΔY and ~ 3.5 nT for ΔZ, respectively. Results show that positive anomalies are found mainly at the Tarim basin with ~6- 8 nT, the Yangtze platform and North China platform with ~4 nT, and the Songliao basin with ~4-6 nT. In contrast, negative anomaly is mainly located in the Tibet orogenic belt with the amplitude ~ (-6)-(-8) nT. Upward continuation of magnetic anomalies was used to semi-quantitatively separate the magnetic anomalies in different depths of crust. The magnetic anomalies at the earth's surface are from -6 to 10 nT for upper crust, middle crust -27 to 42 nT and lower crust -12 to 18 nT, respectively. The strikes of the magnetic anomalies for the upper crust are consistent with those for the middle crust, but not for the lower crust. The high positive magnetic anomalies mainly result from the old continental nucleus and diastrophic block (e.g. middle Sichuan continental nucleus, middle Tarim basin continental nucleus, Junggar diastrophic block and Qaidam diastrophic block). The amplitudes of the magnetic anomalies of the old continental nucleus and diastrophic block are related to evolution of deep crust. These results improve our understanding of the crustal structure over China continent.  相似文献   

14.
Airborne and marine magnetic observations in East Antarctica and adjacent seas of the Indian Ocean were compiled for a magnetic anomaly map of the Antarctic. For East Antarctica, over 260,000 line km of Russian reconnaissance magnetic data were used that had been collected since 1955 mainly at line spacings of about 5, 20 and 50 km. For the offshore areas, magnetic data from American, Australian, German, Japanese, and Russian marine expeditions were incorporated. Digitally recorded data and data digitized from published and unpublished maps and profiles were included in the compilation. Local grids of these data were developed and merged into a regional grid at an interval of 5 km. The prime product of this compilation is a shaded-relief map that shows the most complete and coherent perspective to date of the region's magnetic character. In combination with other types of data, the compilation provides new insight on the tectonic features and history of this largely inaccessible region of the world. It maps out approximately 4300 km of the Antarctic Continental Margin Magnetic Anomaly (ACMMA) related to Gondwana breakup, new cratons and mobile belts, and large submarine igneous provinces.  相似文献   

15.
蒋虎  黄珹 《地球科学进展》2001,16(3):394-398
CHAMP计划是由德国的波茨坦地球科学研究中心 (GFZ)提出 ,而且 ,目前已经付诸实施的科学计划之一。其目的在于通过获取大量近地观测资料来精化地球重力场模型 ,同时开展地球电磁场及地球大气重要参数的确定等研究。详细而全面地介绍该计划的科学目标 ,并评述了它将在建立地球重力场模型、地球电场模型、地球磁场模型和监测地球大气等方面所起的作用。  相似文献   

16.
在前人工作的基础上提出了“多频段的磁异常”的概念.并通过对目前流行的一些滤波方法进行比较,提出使用小波滤波和插值切割法滤波分频的工作思路.探讨了分频段磁异常与地质岩性的关系.认为:①分频以后信息量成倍地增加,读到了许多原始数据(包括常规数据处理)无法读到的信息;②分频提出的信息,不同频率有着不同宏观特征;③不是一种岩性只相关一种频率段异常;④原始数据的结构特点对分频结果起决定性作用;⑤分频有4~5个频段就可以得到许多新的信息;⑥同常规磁异常解释一样,信息提取以后的人工分析是异常解释中非常值得关注的一环;⑦利用插值切割分频的原则是,切割次数是起圆滑作用的因子,因子的大小取决于原始数据的干扰水平(圆滑水平);⑧分频磁异常可以区分不同的岩性.  相似文献   

17.
新疆天山某煤炭勘查区,需查明一水平内火烧煤层的下边界及其富水性。在综合分析该区地质资料及物性参数的基础上,采用了以磁法和瞬变电磁法为主的物探方法。磁法勘探测网设计为20m×80m,并在后期对西部测线进行了加长。根据测区实测磁异常分布图、低通滤波后磁异常分布图、向上延拓30m磁异常分布图及垂向二阶导数磁异常分布图,圈定火烧区主要分布在测区的北部。瞬变电磁法勘探测网设计为40m×80m,依据下1、下5及下10煤层底板富水异常分布图,解释下1、下5煤底板的富水性主要集中在测区的北部,与火烧区范围高度一致,而下10煤层底板富水性极不均匀,仅在测区北部煤层露头附近,受砂岩裂隙的影响,接受降水补给形成零星砂岩裂隙富水区。该解释成果经矿方钻孔验证,结论基本可靠。  相似文献   

18.
Extracted from large surveys of France, Italy and Switzerland, airborne magnetic data covering the western Alpine Arc have been compiled into a single homogeneous map of magnetic anomalies at the constant altitude of 3000 m. For this purpose, each data set has been revised thoroughly and accurately to give a single coherent large-scale pattern.

The magnetic contour map reflects the anomaly pattern over the entire length of the Western Alpine collision suture. The distribution of polarities exhibits a large anomalous low located by reduction to the pole over the whole external part of the belt. The observed anomaly suggests a large gap of magnetization between the Adriatic microplate and the European crust. The analysis of the waveband shows that the broadest wavelengths are produced in the lower crust close to the transition zone, in the granulite facies. This highly magnetic layer is used as a marker to describe the geometry of the European and Adriatic deep seated crust. The main results are presented on a composite synthetic profile showing the sloping side of the European slab and an important crustal thinning to the southeast of the Adriatic slab. This feature is emphasized on the magnetic contour map by a linear magnetic low attributed to major transcurrent fault. This trend is called the Sestri-Voghera trend and extends from the Ligurian basin by the Sestri-Voltaggio Zone to the Judicarian system. Sinistral movements can be recognized along the whole axis as well as possible uplift of rift shoulders. The magnetic anomaly pattern over the complete length of the anomalous body of Ivrea as well as the Insubric-Canavese Line limit the extension of the Adriatic microplate by a well defined linear trend. The symmetrical shears deduced from consecutive anomalies are used to propose a structural scheme.  相似文献   


19.
The present geophysical study deals with the ores and crustal demonstration of southeastern Hazara and its adjoining areas of Azad Jammu and Kashmir, Pakistan, on the basis of terrestrial gravity and magnetic data. Tectonically, the study area lies in the Lesser Himalayas as well as to an extent in the sub-Himalaya, more specifically in the western limb of Hazara Kashmir Syntaxis. In this study, 567 gravity and 508 magnetic stations have been measured with CG-5 gravimeter and proton precession magnetometer, respectively. The collected data have been processed by applying standard corrections and then different types of maps were prepared. The ores in the area have been delineated by the qualitative interpretation of residual Bouguer anomaly and reduction to pole total magnetic intensity maps, whereas regional structures are demarcated by the Bouguer anomaly and regional Bouguer anomaly maps. The positive contour closures on the residual Bouguer anomaly map indicate the iron ore and phosphate, whereas negative contour closures are the effects of low-density material which consists of gypsum and soapstone. The pole-reduced total intensity map also shows the negative and positive contour closures almost in the same localities and confirms the residual Bouguer anomaly map. The geological model computed on the basis of Bouguer anomaly demarcated a series of faults between different rock units in the study area. The Kashmir Boundary Thrust cuts the western limb of Hazara Kashmir Syntaxis near the apex in the north of Muzaffarabad and marks the boundary between Murree Formation and carbonates of Abbottabad Formation. The gravity model also suggests that the thickness of the crust increases towards the northeast.  相似文献   

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