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针对目前人们所使用的交互式重力剖面拟合软件多以正演布格重力异常为主,在应用效果方面存有欠缺的情况,提出了在作重力剖面布格异常拟合的同时,增加高阶方向导数的拟合。其目的是发挥布格重力异常的高阶方向导数在突出浅部地质体的特征,压制区域性深部地质因素,区分相邻地质体引起的叠加异常等方面的优势。这里采用最小二乘法演算了布格重力异常高阶方向导数的计算过程,对计算程序编制和使用中涉及的相关问题进行了阐述,并例举了在地球物理勘探中,利用高阶方向导数提高重力资料解释效果的实例。并在最后对重力剖面进行可视化拟合解释时应注意的要点做了分析,强调了兼顾布格重力异常及其高阶方向导数二者拟合曲线均基本相似,而不应追求其中某一方面精确拟合的解释原则。 相似文献
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在进行重力异常解释时，根据测区重力地壳模型分析结果，为了分离出由不同深度的地质因素引起的重力异常，根据测区重力地壳模型分析结果，主要采用七种不同边长的正方形窗口平均法进行了重力场的划分试验。结果表明：使用不同边长的窗口平均法可以将布格重力异常分解为由深部场源引起的一级区域异常、中深部场源引起的二级区域异常及浅部场源引起的二级剩余异常等三部分，达到了分离布格重力异常的目的。在深部资料很少的青藏高原地区进行重力异常推断解释时，本文所示划分重力异常方法极具参考价值。 相似文献
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《物探与化探》2017,(5)
南京地质调查中心于2007~2015年间在宁芜北部南门头地区开展了大量的物探测量和地质工作,为长江中下游深部找矿提供了找矿经验和方法指导。南门头地区物探资料的解释存在一定多解性,在分析物性数据的基础上,对南门头地区的重磁异常数据进行了一定的处理和解释,总结了引起重力异常的主要因素,并对本区岩体、火山岩、隐爆角砾岩筒、古火山通道的分布及断裂特征有了新的认识。在验证钻孔的控制下,结合重磁剖面、CR法与CSAMT法剖面特征、钻孔测井曲线特征,对本区深部地质结构有了整体的认识。通过对电法、重磁异常的二次解释及对以往取得的资料进行的综合分析,丰富了物探异常解释的经验,对于长江中下游深部找矿方法技术的研究及应用具有一定的指导意义。 相似文献
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针对利用船舶测量海底地形效率低和成本高的缺点,选取西太平洋板块俯冲菲律宾板块而形成的马里亚纳海沟所在海域作为实验区域,依据重力地质方法（GGM）,利用重力异常数据反演海底地形。采用移去恢复技术确定了重力地质法模型的密度差异常数为2.32 g/cm3。分析比较了GGM海深模型、ETOPO1模型和直接将船测点海深数据格网化（模型1）3种海深模型之间的差异,并依据反演结果对"挑战者深渊"两侧地貌进行了研究。结果表明：GGM模型反演海底地形的结果优于ETOPO1模型,更优于将船测点海深数据直接格网化的结果;模型相对误差与海深的关系不大,受海底地形变化影响明显;在船测数据匮乏或者过于稀疏的海域,模型间海深差值结果较大;"挑战者深渊"海沟两侧的地貌有明显差异,在海沟南侧水深小于5 000 m的浅海部分,坡度平缓（2°~5°）,而在水深大于5 000 m的部分,坡度明显增大（10°~15°）;海沟北侧在整个下降阶段坡度很大（10°~15°）,11°45'N附近出现一个缓冲地带。 相似文献
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在中国境内沿北纬40°截取了长剖面,对布格重力异常和卫星重力异常进行了正演拟合计算,并结合新的大地构造划分作了初步的地质解释。结果表明:古老的陆核、原地台、地台和地块等稳定地区内部的密度值横向变化小,年轻的褶皱带等活动地区内部的密度值横向变化大。各个构造域边界的地壳消减对接带,布格重力异常反映不明显,而卫星重力异常对应较好。布格重力异常与卫星重力异常的正演拟合结果不同的地区,其地壳和上地幔的密度分布有较大的差异。这些重要结论有助于寻求卫星重力异常与布格重力异常的在机制和应用上的共性与差异,以便达到对两种重力异常的本质有更进一步认识的目的。 相似文献
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《矿产与地质》2017,(6)
根据广西西大明山地区1∶5万重力资料,并在地质资料的约束下,对广西西大明山地区隐伏岩体三维形态进行了细致的模拟推断。西大明山地区1∶5万布格重力异常图与地质图的研究表明,局部重力异常主要是由西大明山隐伏岩体引起的,2013年广西第四地质队在该地区布置的ZK31901、ZK40004两个钻孔分别发现了隐伏岩体,证实了重力推断。为了求出西大明山地区隐伏岩体的三维形态,采用重磁异常三维物性反演随机子域法方法,具体步骤为三维重磁异常自动反演→重构模型体和建立反演初始模型→三维重磁异常人机交互反演→输出结果(岩体形态、顶底埋深)。通过重磁反演,比较具体的描述岩体深部的空间展布,对于该地区成矿规律研究及深部成矿预测提供了重要的资料,从而为该地区今后开展第二空间深部地质找矿提供重要资料,具有一定的意义。 相似文献
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高陵－达县剖面位于秦岭中段，斜跨中朝准地台、秦岭褶皱系、扬子准地台三大构造单元。在研究剖面实磁场特征的基础上，综合地质、物性、省内及邻省深部物探资料，建立了剖面地质－地球物理模型，依此对剖面通过地段的地壳结构、断裂带深部特征、三大构造单元的深部格架进行了解释推断。 相似文献
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本文按统一比例尺编制了印度-青藏地区1°×1°重力异常图和地形高程图,并用滑动平均方法得到了本区5°×5°重力异常图。用地改后的1°×1°重力异常,采用组合体模型人一机联作选择法,计算了横跨印度-青藏-蒙古长达4680km的岩石圈剖面,还给出了一个楔形体重力正演公式。基本结果有:(1)MBT、MCT的倾角为10°±5°,ITS、NS、KS的倾角为75°±5°;(2)地壳滑脱面的深度在青藏之下约20km,向高喜马拉雅、MCT、MBT抬升至15km;(3)青藏高原南、北边缘均为岩石圈结构的斜坡带,界面倾角由上向下而增大。在大、小喜马拉雅之下,壳内界面(Ⅰ、Ⅱ)的倾角约12°,Moho倾角为18°,岩石圈底面倾角约36°。在祁连山带所有界面倾角都小于喜马拉雅带,其中壳内界面倾角仅约1°,Moho倾角约2°,岩石圈底面倾角约12°;(4)岩石圈厚度由印度、蒙古向高喜马拉雅和祁连山带逐渐增加,与青藏岩石圈的边缘上翘形成主动俯冲和相对逆冲势态。印度岩石圈厚度(或上地幔顶部低密层埋深)不超过50km,蒙古高原(南)厚约70km,到高喜马拉雅和祁连山下分别增加至145和122km,青藏中心地带(怒江两侧)岩石圈厚135km,向南,北边缘各减小到120和90～102km,在高喜马拉雅和祁连山下面形成25和10km的断差;(5)在青藏Moho之下厚5km的高密薄层和软流层之间有一密 相似文献
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以宁芜北火山岩覆盖区南门头工区为例,利用地质、物探等综合找矿方法进行深部矿勘查方法技术的探索。通过研究岩石物性特征,综合分析研究区重力、航磁异常、1:10000面积性高精度磁法测量和重力测量、电法(CR法)综合剖面测量资料,对异常进行综合分析和解释,并对成矿有利部位进行钻探验证,辅以井中物探,取得了较好的应用效果。以南门头工区勘查工作为例,总结了火山岩覆盖区勘查过程中制约找矿的干扰因素,为今后类似覆盖区开展深部找矿工作提供参考。 相似文献
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依据大量的矿床(点)地质勘查成果以及航磁、重力等异常资料,结合本区层控热液叠加改造型金硫矿床成矿模式,分别对铜官山铜金矿田主要金、硫、铜矿床深部资源潜力进行预测分析,为该区指明了深部找矿方向。 相似文献
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《China Geology》2021,4(4):553-570
The southern part of the Kyushu-Palau Ridge (KPR) is located at the conjunction of the West Philippine Basin, the Parece Vela Basin, the Palau Basin, and the Caroline Basin. This area has extremely complex structures and is critical for the research on the tectonic evolution of marginal seas in the Western Pacific Ocean. However, only few studies have been completed on the southern part, and the geophysical fields and deep structures in this part are not well understood. Given this, this study finely depicts the characteristics of the gravity and magnetic anomalies and extracts information on deep structures in the southern part of the KPR based on the gravity and magnetic data obtained from the 11th expedition of the deep-sea geological survey of the Western Pacific Ocean conducted by the Guangzhou Marine Geological Survey, China Geological Survey using the R/V Haiyangdizhi 6. Furthermore, with the data collected on the water depth, sediment thickness, and multichannel seismic transects as constraints, a 3D density model and Moho depths of the study area were obtained using 3D density inversion. The results are as follows. (1) The gravity and magnetic anomalies in the study area show distinct zoning and segmentation. In detail, the gravity and magnetic anomalies to the south of 11°N of the KPR transition from high-amplitude continuous linear positive anomalies into low-amplitude intermittent linear positive anomalies. In contrast, the gravity and magnetic anomalies to the north of 11°N of the KPR are discontinuous and show alternating positive and negative anomalies. These anomalies can be divided into four sections, of which the separation points correspond well to the locations of deep faults, thus, revealing different field-source attributes and tectonic genesis of the KPR. (2) The Moho depth in the basins in the study area is 6–12 km. The Moho depth in the southern part of KPR show segmentation. Specifically, the depth is 10–12 km to the north of 11°N, 12–14 km from 9.5°N to 11°N, 14–16 km from 8.5°N to 9.5°N, and 16–25 km in the Palau Islands. (3) The KPR is a remnant intra-oceanic arc with the oceanic-crust basement.which shows noticeably discontinuous from north to south in geological structure and is intersected by NEE-trending lithospheric-scale deep faults. With large and deep faults F3 and F1 (the Mindanao fault) as boundaries overall, the southern part of the KPR can be divided into three zones. In detail, the portion to the south of 8.5°N (F3) is a tectonically active zone, the KPR portion between 8.5°N and 11°N is a tectonically active transition zone, and the portion to the north of 11°N is a tectonically inactive zone. (4) The oceanic crust in the KPR is slightly thicker than that in the basins on both sides of the ridge, and it is inferred that the KPR formed from the thickening of the oceanic crust induced by the upwelling of deep magma in the process of rifting of remnant arcs during the Middle Oligocene. In addition, it is inferred that the thick oceanic crust under the Palau Islands is related to the constant upwelling of deep magma induced by the continuous northwestward subduction of the Caroline Plate toward the Palau Trench since the Late Oligocene. This study provides a scientific basis for systematically understanding the crustal attributes, deep structures, and evolution of the KPR.©2021 China Geology Editorial Office. 相似文献
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The Jiza' basin is located in the eastern part of Yemen, trending generally in the E–W direction. It is filled with Middle Jurassic to recent sediments, which increase in thickness approximately from 3,000 m to more than 9,000 m. In this study, block-35 of this sedimentary basin is selected to detect the major subsurface geological and structural features characterizing this basin and controlling its hydrocarbon potentials. To achieve these goals, the available detailed gravity and magnetic data, scale 1:100,000, were intensively subjected to different kinds of processing and interpretation steps. Also, the available seismic reflection sections and deep wells data were used to confirm the interpretation. The results indicated three average depth levels; 12.5, 2.4, and 0.65 km for the deep, intermediate, and shallow gravity sources and 5.1 and 0.65 km for the deep and shallow magnetic sources. Accordingly, the residual and regional anomaly maps were constructed. These maps revealed a number of high and low structures (horsts and grabens and half grabens), ranging in depth from 0.5 km to less than 4.5 km and trending mainly in the ENE, NW, and NE directions. However, the analytical signal for both gravity and magnetic data also showed locations, dimensions, and approximate depths of the shallow and near surface anomaly sources. The interpretation of the gravity and magnetic anomalies in the area indicated that the NW, NNW, ENE, and NE trends characterize the shallow to deep gravity anomaly sources; however, the NE, NW, and NNE trends characterize the magnetic anomaly sources, mainly the basement. Two-dimensional geologic models were also constructed for three long gravity anomaly profiles that confirmed and tied with the available deep wells data and previously interpreted seismic sections. These models show the basement surface and the overlying sedimentary section as well as the associated faults. 相似文献
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Magnetic anomalies of offshore Krishna-Godavari basin,eastern continental margin of India 总被引：1，自引：0，他引：1
K. V. Swamy I. V. Radhakrishna Murthy K. S. Krishna K. S. R. Murthy A. S. Subrahmanyam M. M. Malleswara Rao 《Journal of Earth System Science》2009,118(4):405-412
The marine magnetic data acquired from offshore Krishna-Godavari (K-G) basin, eastern continental margin of India (ECMI),
brought out a prominent NE-SW trending feature, which could be explained by a buried structural high formed by volcanic activity.
The magnetic anomaly feature is also associated with a distinct negative gravity anomaly similar to the one associated with
85°E Ridge. The gravity low could be attributed to a flexure at the Moho boundary, which could in turn be filled with the
volcanic material. Inversion of the magnetic and gravity anomalies was also carried out to establish the similarity of anomalies
of the two geological features (structural high on the margin and the 85°E Ridge) and their interpretations. In both cases,
the magnetic anomalies were caused dominantly by the magnetization contrast between the volcanic material and the surrounding
oceanic crust, whereas the low gravity anomalies are by the flexures of the order of 3–4 km at Moho boundary beneath them.
The analysis suggests that both structural high present in offshore Krishna-Godavari basin and the 85°E Ridge have been emplaced
on relatively older oceanic crust by a common volcanic process, but at discrete times, and that several of the gravity lows
in the Bay of Bengal can be attributed to flexures on the Moho, each created due to the load of volcanic material. 相似文献
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A family of geophysical lineaments have been identified in ~15,000 km~2 in central Kerala between9 30'N to 10 45'N and 76 00'E to 77°30′E,integrating geophysical data with geological and geomorphological features. The characteristics of these lineaments in the magnetic and gravity fields and their derivatives have been analysed. The evolution of the lineaments has been traced to the temporal phases of global evolution of the region. A group of these faults have formed by reactivation of the deep-seated distensional fractures associated with and accompanying dyke emplacements during the episodic breakup of Gondwana at ~90 and 65 Ma under distinctive mantle thermal regimes. It is possible that reactivation of these distensional faults may have started during the cooling interval of time between the two distensions in the 90 and 65 Ma and post 65 Ma periods and later in the Cenozoic, when the lineaments were enlarged to their present dimension, possibly under the influence of forces that led to the uplift of the western Ghats. These may extend down to the crust-mantle interface. A cluster of youngergeophysical lineaments has been generated by reactivation along the weak planes of transformation of the charnockitic rocks of the Precambrian. They seem to have a strike-slip character. They are devoid of any dyke association and were formed on a cold crust. They may be confined to the upper-middle crust.They were generated in the high intensity intra-plate palaeo-stress fields of the triple forces arising from(1) the back-thrust from the Himalayan Collision;(2) the impact of epeirogenic forces and related isostatic uplift of the Western Ghats and(3) the flexural isostatic uplifts due to surface loads of late Mesozoic basaltic lavas and Cenozoic sedimentation in the coastal rifted basins in late Cenozoic, probably in the time span of 20 Ma to the present, when the palaeostress fields were most intense. 相似文献
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The observed aeromagnetic anomaly map of Southern High Plateaus provides general information about the magnetization variations that are associated with subsurface magnetic sources, but it does not bring clear information about all geological elements of the study area. In this work, we attempt, by analyzing these aeromagnetic data, to determine structures of Paleozoic basement that may indicate the presence of major deep-seated structures in this area. To better understand and outline the basement geological structures, two approaches have been performed. Such analysis includes application of a low-pass filtering and spectral analysis, which permits an enhanced visual interpretation of the magnetization sources and leads to a better knowledge of the geological structures especially basins or intrusive bodies. The results obtained show magnetic anomalies indicating geological features trending NE–SW. They also reveal two depths of magnetic sources in the area. The deeper sources range from 1074 to 4057 m and reflect the Paleozoic basement. However, the shallower sources range from 153 and 596 m reflecting magnetic sources shallower than the basement. The outcomes of this study suggest a new structure and will contribute to better understand the characteristics and organization of the basin as well as the improvement of the geological map of the area for hydrocarbon exploration. 相似文献
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From the data of the geomagnetic survey of the Indian equatorial region conducted during 1971, it has been possible to deduce the subsurface magnetic anomalies at each survey station. The vertical magnetic anomaly profiles seem to reflect some of the known geological structures in the region. The association between magnetic anomalies and the deep-seated structures in this area emphasises the importance of future intensive studies. 相似文献