共查询到20条相似文献，搜索用时 15 毫秒
1.
The results of a magnetic study of part of the Younger Granite Province of Nigeria are presented here. Spectral analysis of the magnetic anomalies over the area has been carried out in an effort to estimate the depth to magnetic sources. Average magnetic source depth of 286 m has been obtained for the area and this is thought to be related to the depth to the top of the main anomalous structures in the area. Observed magnetic anomaly profiels taken across the area have been interpreted in terms of arbitrarily shaped bodies—whose existence was confirmed by 3-D Hilbert transformation-using nonlinear optimization techniques. The modelled bodies occur at depths of 200–760 m and have magnetizations of 0.29–0.47 A/m. The results from the analysis of the magnetic field are discussed in relation to the results from previous gravity studies over the area and the mode of emplacement of the Younger Granites. 相似文献
2.
《Journal of Applied Geophysics》2010,72(4):157-161
An intimate mathematical relation between Hartley and Hilbert transforms is given here in contrast with the well known Fourier and Hilbert transform relations. It is interesting to note that the Fourier–Hilbert and Hartley–Hilbert transforms while possessing the same magnitude differ in phase by 270°. The inverse Hartley–Hilbert transform returns the original function unlike the Fourier–Hilbert transform which results the negative of the original function. Further, it may be realized that the envelope defined here of the analytic signal in both Fourier–Hilbert and Hartley–Hilbert domains numerically remain the same while differing in polarity. The feasibility of Hartley–Hilbert transform for a straight forward interpretation, total magnetic anomaly due to a thin plate from Tejpur, India and self potential data of the Sulleymonkey anomaly in the Ergani Copper district, Turkey are illustrated in contrast with the Fourier–Hilbert transform. This pair of transforms have innumerable geophysical applications. 相似文献
3.
Recently observed features in the subsurface geology of the Haifa Bay area (northern Israel) have been evaluated using 3-D forward gravity and magnetic modeling and inversion schemes. The interpretation is based on updated petrophysical data of the Jurassic, Cretaceous and Tertiary sedimentary layers and volcanics. It has been shown that the Bouguer gravity anomalies correspond mainly to thickness variations in the Senonian to Tertiary sediments. The gravity effect of these sediments was calculated using their actual densities and structural setting as interpreted from seismic reflection data. This effect was removed from the Bouguer gravity in order to study the pre-Senonian geological structures. The pattern of residual gravity anomalies (named “stripped gravity”) is essentially different from the pattern of the Bouguer gravity. The prominent Carmel gravity high, clearly seen on the Bouguer gravity map, completely vanishes on the “stripped” gravity map. That suggests that this relatively positive anomaly is caused by the considerable thickness of the low-density young sediments in the surrounding areas and does not correspond to high-density magmatic rocks or crystalline basement uplift as previously suggested. The average densities of the Jurassic and Cretaceous volcanics are generally lower then those of the background sedimentary rocks. Volcanics are the main cause for magnetic anomalies onshore and offshore northern Israel. The magmatic root of the Asher volcanics is, most probably, located close to the Yagur fault. A large, deep-seated gabbroic intrusion is assumed to be located under the Mediterranean abyssal plain in the NW part of the study area. The Atlit marine gravity low appears to be caused by a thick Mesozoic and Tertiary sedimentary accumulation. The results presented should be of considerable assistance in delineating some aspects of hydrocarbon exploration in the area. 相似文献
4.
Jarosław Zawadzki Tadeus Magiera Piotr Fabijańczyk 《Studia Geophysica et Geodaetica》2009,53(1):133-149
The goal of the study was the geostatistical evaluation of quantitative magnetic measures, which can be used for effective
delineation of the extent of the area polluted with heavy metals. Several parameters of magnetic susceptibility, measured
in the soil profile, were proposed as magnetic indicators of soil pollution and analyzed in detail. The following parameters
were calculated: maximum magnetic susceptibility, magnetic susceptibility at the depth of 3 cm and 5 cm, and the area under
the curve of magnetic susceptibility. Measurements were performed at two forested study areas, located in Upper Silesian Industrial
Area (Poland). Analyses were performed using geostatistical methods, and the results were verified using dense chemical measurements.
The results showed that the area under curve of magnetic susceptibility was the most effective magnetic indicator of soil
contamination with heavy metals. It was possible to detect the entire polluted area, and only about 16% of the study area
was assumed to be contaminated while being unpolluted. The results obtained with maximum magnetic susceptibility and magnetic
susceptibility at the depth of 3 cm and 5 cm were less effective in comparison with the area under curve of magnetic susceptibility. 相似文献
5.
G.R.J. Cooper 《Geophysical Prospecting》2017,65(1):316-323
A new method for the calculation of the depth, location, and dip of thin dykes from pole‐reduced magnetic data is introduced. The depth can be obtained by measuring the distance between chosen values of a tilt angle that is based upon the ratio of the magnetic field and its Hilbert transform over the dyke. Alternatively, it can be obtained from the horizontal derivative of the ratio of the Hilbert transform of the field to the field itself, over the dyke. The latter method also allows the dip of the dyke to be estimated from the gradient of the depth estimates. 相似文献
6.
磁异常的反演是地球物理勘探的重要手段,三维磁化率反演是磁异常定量解释中的一种重要方法.由于剩磁的存在使得磁化方向与地磁场方向产生偏差,从而影响了磁异常反演与解释的精度.本文基于磁异常模量反演和磁化强度矢量反演方法得到了一种新的磁化强度矢量反演方法.与以往的磁化强度矢量反演方法相比,该方法以磁异常模量反演得到的磁化率模型为约束,采用Lp范数正则化方法求解,提高了磁化强度矢量反演的精度和效率.本文通过模拟试验的反演计算,验证了这种磁化强度矢量反演方法的有效性.最后,将本文方法应用于新疆东天山卡拉塔格地区航磁数据的解释,获得了地下空间不同磁性差异的磁性体的空间分布特征,为进一步分析研究区隐伏矿床提供了重要信息. 相似文献
7.
伊犁盆地中部区域地处多个构造单元的交汇区,构造复杂,缺乏高精度地质资料,制约了对盆地构造演化的进一步认识.本文联合使用多种先验信息作为约束条件,利用高精度重磁数据反演获得了研究区地下海拔-10 km以浅的三维密度和磁性结构,增强了反演结果的可靠性.结果揭示以白石墩次凸为中心发育了一个"北断南超"的南西-北东向不对称型凹陷,北部沉积厚度大于南部;区内主要断裂具有高角度特征,生烃中心受断裂控制,阿吾拉勒山前凹陷浅部可能发育逆掩断裂;火成岩以侵入的基性火成岩为主,伴有部分喷出火成岩和中酸性火成岩. 相似文献
8.
Using aeromagnetic data acquired in the area from the Cerro Prieto geothermal field, we estimated the depth to the Curie point isotherm, interpreted as the base of the magnetic sources, following statistical spectral-based techniques. According to our results the Curie point isotherm is located at a depths ranging from 14 to 17 km. Our result is somewhat deeper than that obtained previously based only in 2-D and 3-D forward modeling of previous low-quality data. However, our results are supported by independent information comprising geothermal gradients, seismicity distribution in the crust, and gravity determined crustal thickness. Our results imply a high thermal gradient (ranging between 33 and 38 °C/km) and high heat flow (of about 100 mW/m2) for the study area. The thermal regime for the area is inferred to be similar to that from the Salton trough. 相似文献
9.
南海北部陆架西区盆地地质、地球物理场特征及其深部结构 总被引：8，自引：6，他引：8
分析了南海北部陆架西区盆地的地质、地球物理场特征，计算了研究海域重、磁资料的1阶小波细节、4阶小波逼近变换。根据分析与计算可知，研究区的布格重力异常以北西低的负值，东南高的正值为特征。在东部及东南部异常等值线走向为北东；西部异常等值线以北西走向为特征；西北地区异常以北东东、北东走向的局部等值线圈闭为特征。磁场的展布十分复杂，按磁异常的变化程度可分为三个变化区，即磁异常平静区、剧变区及缓变区。磁异常的平静区位于研究区的西部，即莺歌海盆地所在位置，这一带磁异常等值线极为稀疏，异常值为负背景异常。剧变区位于海南岛，该地区的磁异常变化极为剧烈，异常特征以局部小圈闭为特征，等值线分布密集。磁异常的平缓区位于平静区及剧变区之外的其它地区。琼东南盆地、北部湾盆地的磁异常具有此特征。根据重、磁场资料以及南海北部盆地钻井取样的测试结果、同时参考穿越南海地学断面的结果，对研究区的地壳结构进行了反演计算，计算表明南海陆架盆地区域地壳结构较为复杂，研究区的地壳厚度在22－33km之间，总的趋势由陆向洋地壳厚度逐渐减薄，反映出该区域地壳具有陆壳、拉伸陆壳、过渡壳的性质，同时存在有上地幔隆起区及凹陷区。磁性底界面厚度在17－24km之间变化，其中在莺歌海盆地较深，在海南岛地区磁性界面较浅。 相似文献
10.
Aeromagnetic anomalies measured over the three relict andesite volcanoes (Paritutu, Kaitake and Pouakai) in Taranaki are largely dominated by topographic effects. Three-dimensional magnetic modelling, well constrained by both contrasting levels of exposure and previous gravity models, shows that the bulk magnetization of the andesite edifice and edifice core of both Kaitake and Pouakai is 2.5–3.5 A m-1 in a direction close to that of the present earth's field. However, the large andesite dyke/stock complexes below all three edifices and a localized area of the Kaitake edifice directly above the centre of the subedifice complex have anomalously low bulk magnetizations of 0.3–1.0 A m-1 in the same direction. These subsurface complexes represent dyke injection from magma chambers situated in the basement, probably below 6 km depth. Here, we deduce that heat from these magma chambers drove hydrothermal convection systems causing widespread demagnetization, especially in the subedifice complexes, but also locally within the edifices themselves. A lesser degree of demagnetization at Pouakai, the youngest of the three volcanoes, may indicate a shorter and consequently more intense period of activity at this centre. 相似文献
11.
An alternative approach in establishing relation between vertical and horizontal gradients of 2D potential field 
下载免费PDF全文
下载免费PDF全文 Indrajit G. Roy 《Geophysical Prospecting》2017,65(6):1687-1693
The relation in which the vertical and horizontal gradients of potential field data measured along a profile across a two‐dimensional source are a Hilbert transform pair is re‐established using complex domain mathematics. In addition, a relation between the measured field and its vertical gradient in terms of a closed‐form formula is also established. The formula is based on hypersingular or Hadamard's finite‐part integral. To estimate the vertical gradient directly from the field data, Linz's algorithm of computing Hadamard's finite‐part integral is implemented. Numerical experiments are conducted on synthetically generated total magnetic intensity data with a mild level of noise contamination. A model of a magnetically polarised vertical thin sheet buried at a finite depth within a non‐magnetic half‐space was considered in generating the synthetic response. The results from numerical experiments on the mildly noise‐contaminated synthetic response are compared with those from using classical Fourier and robust regularised Hilbert transform‐based techniques. 相似文献
12.
磁性地层学是界定沉积物地质年代的一种重要方法,该方法的应用建立在沉积物记录了可靠的特征剩磁基础上.红层的磁性地层年代学研究对于我国华南地区晚中生代以来古环境、古气候的演化具有极为重要的意义.但是,目前对于红层古地磁可靠性的解释存在广泛的争议,为更好地理解并尝试解决具体红层剖面的古地磁可靠性问题,迫切需要综合岩石磁学和其他非磁学手段对沉积物中的载磁矿物性质进行系统厘定.本文通过对赣南地区两个典型晚白垩纪红层剖面(信丰XF剖面和留车LC剖面)进行详细的岩石磁学分析,并结合扫描电镜和沉积相特征,判定出磁性矿物以赤铁矿为主,含有少量针铁矿、磁赤铁矿和磁铁矿.其中,赤铁矿是最主要的剩磁载体,且与钛铁矿共存,综合磁学与非磁学结果判定其记录了原生的沉积剩磁.在获得了可靠的古地磁信息基础上,结合前人对该区域生物地层学和年代学研究并与邻区地层比对,初步判断出LC剖面与XF剖面地质年代分别为晚白垩纪早期Cenomian期和晚白垩纪晚期Maastrichtian期.XF剖面依据ESR测年、南雄盆地地层比对和沉积相的判断,地层极性时段初步界定为C30n,即68.196~66.398 Ma,这为进一步探讨该地区的古环境和古气候演化提供了可参考的年龄标尺. 相似文献
13.
东海陆架盆地及其周边海域地质、地球物理场特征 总被引：7，自引：5，他引：7
分东海陆架盆地及其周边海域的重、磁场特征、对研究区域的地球物理场资料进行了小波变换与多尺度分布与计算，计算了研究了海域重，磁资料的1－4阶小波变换逼近、细节、根据分析与计算可知，在东海陆架盆地及其周边域，重、磁异常的主要特征没有内陆盆地那样明显，但盆地内的绝大部分地区均位于异常相对缓变区，在盆地内部有时有局部异常的圈闭及剧变区，但总的特征为缓变的，而周边区域多为相对剧变区，但也存在局部区域的缓变, 、磁场特征表明，盆地基底相对盆地周边区域主要由密度较大，磁性中的岩石组成，因此盆地中部以高正磁异常为主，布格重力异常 对周边地区高，东海陆架盆地及其周边海域的重力场的主要走向为NNE向，局部重力异常较为平缓，磁异常走向没有重力异常明显，但主要也为NNE向，重、磁场的分布特征表明，东海陆架盆地及其邻域的地质构造为大陆架构造的延伸。 相似文献
14.
Study on coupling between deep and shallow structures of Xingtai area and some significant questions
IntroductionIn order to gain a clear idea of the deep tectonic environment of Xingtai earthquake area,three wide-angle deep seismic renectionlrefraction profiles have been conducted through the are4they are Yuanshi--Ji'nan profile, Renxian--Wuqing profile and Tat' an--LongyaM inzhou profi I e.The Yuanshi--Ji'nan profile passes through the epicenter of the Ms=7.2 main shock andTat' ~ongyaO--X inzhou profi ie passes through the ep icenter of the Ms=6. 8 earthquake. Duringthe "Eighth Five-… 相似文献
15.
Based on the Hilbert–Huang spectral analysis, a method is proposed to identify multi‐degree‐of‐freedom (MDOF) linear systems using measured free vibration time histories. For MDOF systems, the normal modes have been assumed to exist. In this method, the measured response data, which are polluted by noises, are first decomposed into modal responses using the empirical mode decomposition (EMD) approach with intermittency criteria. Then, the Hilbert transform is applied to each modal response to obtain the instantaneous amplitude and phase angle time histories. A linear least‐square fit procedure is proposed to identify the natural frequency and damping ratio from the instantaneous amplitude and phase angle for each modal response. Based on a single measurement of the free vibration time history at one appropriate location, natural frequencies and damping ratios can be identified. When the responses at all degrees of freedom are measured, the mode shapes and the physical mass, damping and stiffness matrices of the structure can be determined. The applications of the proposed method are illustrated using three linear systems with different dynamic characteristics. Numerical simulation results demonstrate that the proposed system identification method yields quite accurate results, and it offers a new and effective tool for the system identification of linear structures in which normal modes exist. Copyright © 2003 John Wiley & Sons, Ltd. 相似文献
16.
The Central Sichuan Block(CSB) is the hardest block between the deep faults of Pujiang-Bazhong and Huaying Mountain in the central part of Sichuan Basin, which lies in the northwestern part of the upper Yangtze Craton. The CSB has long been considered as the oldest and most stable core area of Yangtze Craton, with the uniform basement and high level of hardening. Here we present a detailed interpretation of deep structures in the CSB by integrating high-resolution seismic data(approx. 50000 km2) with large-scale aeromagnetic data. Results show that eight Neoproterozoic extensional structures of different scales are nearly EW-, NEE-, and NW-trending in the CSB. Discovery of these extensional structures changes previous understanding of the CSB as a unified block. The extensional structures experienced one or two stages of extension in the longitudinal section, and filled with 3000–5000-m-thick weakly magnetic materials. Development of basal A-type granite in Weiyuan, Sichuan Basin and bimodal volcanic rocks of the Suxiong Formation, Western Sichuan confirms the CSB's Neoproterozoic extensional tectonic setting. The newly discovered Neoproterozoic extensional structures are of great significance for source rock and favorable sedimentary facies distribution, reservoir development, and gas accumulation. 相似文献
17.
C. Prior 《地球物理与天体物理流体动力学》2016,110(5):432-457
We study the emergence of braided magnetic fields from the top of the solar interior through to the corona. It is widely believed that emerging regions smaller than active regions are formed in the upper convection zone near the photosphere. Here, bundles of braided, rather than twisted, magnetic field can be formed, which then rise upward to emerge into the atmosphere. To test this theory, we investigate the behaviour of braided magnetic fields as they emerge into the solar atmosphere. We compare and contrast our models to previous studies of twisted flux tube emergence and discuss results that can be tested observationally. Although this is just an initial study, our results suggest that the underlying magnetic field structure of small emerging regions need not be twisted and that braided field, formed in the convection zone, could suffice. 相似文献
18.
Relationship between the regional tectonic activity and crustal structure in the eastern Tibetan plateau discovered by gravity anomaly 下载免费PDF全文
下载免费PDF全文 The eastern Tibetan plateau has been getting more and more attention because it combines active faults, uplifting, and large earthquakes together in a high-population region. Based on the previous researches, the most of Cenozoic tectonic activities were related to the regional structure of the local blocks within the crustal scale. Thus, a better understanding of the crustal structure of the regional tectonic blocks is an important topic for further study. In this paper, we combined the simple Bouguer gravity anomaly with the Moho depths from previous studies to investigate the crustal structure in this area. To highlight the crustal structures, the gravity anomaly caused by the Moho relief has been reduced by forward modeling calculations. A total horizontal derivative (THD) had been applied on the gravity residuals. The results indicated that the crustal gravity residual is compatible with the topography and the geological settings of the regional blocks, including the Sichuan basin, the Chuxiong basin, the Xiaojiang fault, and the Jinhe fault, as well as the Longmenshan fault zone. The THD emphasized the west margin of Yangtze block, i.e., the Longriba fault zone and the Xiaojiang fault cut through the Yangtze block. The checkboard pattern of the gravity residual in the Songpan-Garze fold belt and Chuandian fragment shows that the crust is undergoing a southward and SE-directed extrusion, which is coincident with the flowing direction indicated from the GPS measurements. By integrating the interpretations, the stepwise extensional mechanism of the eastern Tibetan plateau is supported by the southeastward crustal deformation, and the extrusion of Chuandian fragment is achieved by Xianshuihe fault. 相似文献
19.
20.
Either the magnetic anomaly or the horizontal gradient of gravity, if plotted against its Hilbert transform and then joined by a smooth curve, the relation figure is obtained. Properties of relation figures for some two-dimensional sources of simple geometry are shown to be useful in distinguishing the source geometry and also in estimating the source parameters, even in the presence of remanence. 相似文献