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利用屯溪地区重磁、地质和矿产资料,阐述了屯溪地区航磁、重力异常特征,并结合物性特征,分析了航磁、重力异常的地质成因及其对地质构造和矿产的反映。屯溪地区重磁异常特征十分清晰,反映了屯溪盆地地基底、盖层和侵入岩分布规律,标明屯溪盆地是古生代基底,这一认识大大扩展了屯溪地区找矿空间,说明在红层盆地古生代基底中有寻找朱溪式超大型矽卡岩钨铜矿床的可能性。 相似文献
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杨桥孜铜金矿是皖北覆盖区以地质理论为指导通过综合物探手段发现的一处中型矽卡岩型矿床。该矿床是皖北地区迄今为止发现的规模最大金矿床,对三铺岩体成矿预测、皖北地区找矿、研究华北陆块找金方向具有重要意义,为覆盖区综合找矿方法提供了成功经验。重磁勘探在该矿床的发现过程中发挥了重要作用,重磁组合异常特征倍受关注。杨桥孜金铜矿位于重力梯级带的次级鼻状重力高异常区,重力二阶导数异常与矿体分布相吻合;地磁场以正异常为背景,局部叠加明显的强磁异常,强磁异常与铁矿体分布一致,铜金矿体对应于磁力梯级带。重高磁高、重高磁梯组合异常在矿床普查过程中发挥了作用。 相似文献
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南海西北部海南岛幅重磁场特征分析 总被引：1，自引：0，他引：1
海南岛幅重力异常基本特征是自由空间异常呈现北高、南低的变化趋势，布格重力异常表现为随着水深加大，异常值增大，由西北向东南方向（南海海盆）逐渐增高。海南岛幅磁异常基本特征是以负值为主，东部磁异常走向主要为北东和东西向，西部磁异常走向主要为北西向。陆架区为低缓负异常，陆坡区为局部负异常及正负伴生异常，深海盆地为急剧变化的条带状异常，而西沙群岛为局部急剧变化的异常。依据重磁场异常，结合相关的地形、地貌、地质构造等资料对海南岛幅进行合理分区，并初步进行地质因素分析。 相似文献
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东海地区重磁场特征及其地质意义 总被引：1，自引：0，他引：1
重磁方法是地球物理研究中的重要分支,其以位场理论为基础,具有在水平方向上的高分辨率能力并能够提供地壳深部结构的信息,从而对于研究沉积盆地的形成演化过程起着经济有效的作用.文章以东海地区近年的重磁数据为基础,分析了重磁场特征,布格异常值介于-160～460 mGal,在正值背景上发育一些局部的重力低圈闭,布格重力异常的主体走向为NE向,磁力异常值介于-200～+ 500 nT,磁力异常的主体走向为NE向.同时,利用磁异常数据计算了东海的磁性基底界面,磁性基底深度在4～12 km之间变化,各个地区磁性基底深度起伏变化不同,结合前人研究成果,认为东海地区广泛存在中生界地层. 相似文献
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重磁异常结合其他地质、地球物理资料进行相关分析,有利于提高位场异常地质解释的质量。利用等效点源反演绘制的图件,来研究北美及相邻海域的地面自由空间重力异常、POGO(线轨道地球物理观测)卫星磁异常,以及区域热流和构造信息间的视一空间相关关系。在卫星高度上相关异常的区域位场,也用泊松理论在重、磁场导数异常之间,移动窗口线性回归作定量分析。在大陆地区观测到长波长重磁异常之间的一种反相关关系。重力异常为负、磁力异常为正的地区,其特点是地壳相对较厚,磁化强度较高。例如:一个突出的磁力高与爱那达科盆地向辛辛那堤穹窿延伸的重力低相对应。磁力异常为负、重力异常为正的地区,其特征是地壳较薄,区域热流值较高。如:北美和中美洲的科迪勒拉地区,以及黄石地热区。虽然,海洋区域的重磁异常显示弱相关,但统计相关的符号一般为正。 相似文献
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近期的川西地区深层火山岩勘探成果表明该地区二叠系火山岩具有巨大勘探潜力,但目前以地震为主的勘探手段在精细刻画火山岩分布范围等方面尚存在困难,本研究尝试通过重磁方法为火山岩勘探提供更多有利证据。利用川西地区最新的重磁资料,结合现有地质认识分析川西地区重磁物性特征;根据不同模型的重磁正演模拟结果,总结川西地区深层火山岩重磁响应特征。通过实测重磁资料处理,分析研究区断裂分布特征和高磁异常分布规律。研究表明:(1)正演结果显示磁力异常对火山岩的反应敏感,重力异常对断裂构造反应明显,但对火山岩无明显反应;(2)磁力异常对火山岩的刻画能力较为突出,能够识别出厚度大于45 m的火山岩,但对于火山岩埋深、岩性变化的识别存在困难;(3)通过研究区重力异常解译出的断裂构造与研究区已知断裂构造吻合度较高,同时利用磁力异常刻画的火山岩分布情况与现有认识也具有可比性。重磁勘探在四川盆地火山岩勘探中具有重要作用,重力勘探可探明控制火山岩分布的深大断裂的发育情况,磁力勘探能够识别出火山岩平面分布特征,快速圈定有利靶区,进而为火山岩勘探提供有力的重磁依据。 相似文献
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梅岩辉 《物探化探计算技术》2007,(Z1)
根据重力位、重力异常、磁位和磁异常公式,应用泊松关系,通过严格的公式推导,给出了重力位、重力异常、磁位和磁异常之间的数学关系,从而使重磁异常正演计算表达式包含于简单的规则之中,揭示出均质多面体重磁异常正演理论的一致性。 相似文献
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利用区域物探重磁资料圈定黔东金刚石母岩钾镁煌斑岩的尝试 总被引：2，自引：2，他引：0
本文试图据镇远马坪一带分布的钾镁煌斑岩露头,及与之对应的1∶20万区域重磁异常的特征响应值（剩余重力异常值（1～4）×10-5m/s2、航磁异常值（2～12）nT）为线索,以辉石重砂异常点分布、金刚石砂矿出土点分布、金刚石指示矿物铬尖晶石发现点分布、有限物性资料及局部重磁异常分布特征为基础,对台江-剑河-锦屏-黎平一带... 相似文献
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A re-compilation of magnetic data in the Weddell Sea is presented and compared with the gravity field recently derived from retracked satellite altimetry. The previously informally named ‘Anomaly-T,’ an east–west trending linear positive magnetic and gravity anomaly lying at about 69°S, forms the southern boundary of the well-known Weddell Sea gravity herringbone. North of Anomaly-T, three major E–W linear magnetic lows are shown, and identified with anomalies c12r, c21–29(r) and c33r. On the basis of these, and following work by recent investigators, isochrons c13, c18, c20, c21, c30, c33 and c34 are identified and extended into the western Weddell Sea. Similarly, a linear magnetic low lying along the spine of the herringbone is shown and provisionally dated at 93–96 Ma. Anomaly-T is tentatively dated to be M5n, in agreement with recent tectonic models.Although current tectonic models are generally in good agreement to the north of T, to the south interpretations differ. Some plate tectonic models have only proposed essentially north–south spreading in the region, whilst others have suggested that a period of predominantly east–west motion (relative to present Antarctic geographic coordinates) occurred during the mid-Mesozoic spreading between East and West Gondwana. We identify an area immediately to the south of T which appears to be the southerly extent of N–S spreading in the herringbone. Following recent work, the extreme southerly extent of the N–S directed spreading of the herringbone is provisionally dated M9r/M10. In the oldest Weddell Sea, immediately to the north and east of the Antarctic shelf, we see subtle features in both the magnetic and gravity data that are consistent with predominantly N–S spreading in the Weddell Sea during the earliest opening of East and West Gondwana. In between, however, in a small region extending approximately from about 50 km south of T to about 70°S and from approximately 40° to 53°W, the magnetic and gravity data appear to suggest well-correlated linear marine magnetic anomalies (possible isochrons) perpendicular to T, bounded and offset by less well-defined steps and linear lows in the gravity (possible fracture zones). These magnetic and gravity data southwest of T suggest that the crust here may record an E–W spreading episode between the two-plate system of East and West Gondwana prior to the initiation of the three-plate spreading system of South America, Africa and Antarctica. The E–W spreading record to the east of about 35°W would then appear to have been cut off at about M10 time during the establishment of N–S three-plate spreading along the South American–Antarctic Ridge and then subducted under the Scotia Ridge. 相似文献
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The movement of Antarctica with respect to South America has a number of implications for paleocirculation as well as for the reconstructions of Gondwanaland. Recent papers on the Southwest Indian Ridge have published new or revised poles of opening for Africa and Antarctica which can be combined with the poles of opening between South America and Africa to give resultant motions between South America and Antarctica.The first indication of a complete closure between South America and the Antarctic Peninsula is at anomaly 28 time (64 Ma) as the two continents are now configured. Between anomaly 28 time (64 Ma) and anomaly M0 time (119 Ma) the amount of closure does not change greatly, and the small computed overlap can be explained by minor uncertainties in the rotation poles used for the reconstructions or some slight extension between East and West Antarctica. By 135 Ma some rotation or translation of the Antarctic Peninsula with respect to East Antarctica must be postulated in addition to any presumed extension between East and West Antarctica in order to avoid an overlap of South America with the Antarctic Peninsula.Having determined what we feel to be a viable reconstruction of Western Gondwanaland and holding South America fixed, we rotated Africa and Antarctica, with respect to South America, for eight different times during the past. Africa moved away from South America in a more or less consistent manner throughout the time period, closure to present, while Antarctica moved away from Africa in a consistent manner only between 160 Ma and 64 Ma. At 64 Ma its motion changed abruptly: it slowed its north-south motion with respect to Africa and began slow east-west extension with respect to South America. This change supports the hypothesis that a major reorganization of the triple junction between Africa, Antarctica and South America occurred between 60 and 65 Ma. The triple junction changed from ridge-ridge-ridge to ridge-fault-fault at the time of the major westward jump of the Mid-Atlantic Ridge just south of the Falkland-Agulhas Fracture Zone.The Mesozoic opening of the Somali Basin moved Madagascar from its presumed original position with Africa in Gondwanaland. The closure of Sri Lanka with India produces a unique fit for India and Sri Lanka with respect to Africa, Madagascar and Antarctica. This fit juxtaposes geological localities in Southeast India against similar localities in Enderhy Land. East Antarctica. The late Jurassic opening in the Somali Basin is tied to opening of the same age in the Mozambique Basin. Since this late Jurassic movement represents the initial break-up of Gondwanaland, it is assumed that similar movement must have occurred in what is now the western Weddell Sea and may also explain the opening evidenced by the Rocas Verdes region of southern South America. 相似文献
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Ten years after the USAC (U.S.–Argentina–Chile) Project, which was the most comprehensive aeromagnetic effort in the Antarctic Peninsula and surrounding ocean basins, questions remain regarding the kinematics of the early opening history of the Weddell Sea. Key elements in this complex issue are a better resolution of the magnetic sequence in the western part of the Weddell Sea and merging the USAC data set with the other magnetic data sets in the region. For this purpose we reprocessed the USAC data set using a continuation between arbitrary surfaces and equivalent magnetic sources. The equivalent sources are located at a smooth crustal surface derived from the existing bathymetry/topography and depths estimated by magnetic inversions. The most critical area processed was the transition between the high altitude survey over the Antarctic Peninsula and the low altitude survey over the Weddell Sea that required downward continuation to equalize the distance to the magnetic source. This procedure was performed with eigenvalue analysis to stabilize the equivalent magnetic source inversion.The enhancement of the Mesozoic sequence permits refining the interpretation of the seafloor-spreading anomalies. In particular, the change in shape and wavelength of an elongated positive in the central Weddell Sea suggests that it was formed during the Cretaceous Normal Polarity Interval. The older lineations in the southwestern Weddell Sea are tentatively attributed to susceptibility contrasts modeled as fracture zones. Numerical experimentation to adjust synthetic isochrons to seafloor-spreading lineations and flow lines to fracture zones yields stage poles for the opening of the Weddell Sea since 160 Ma to anomaly 34 time. The corresponding reconstructions look reasonable within the known constraints for the motions of the Antarctic and South America plates. However, closure is not attained between 160 and 118 Ma if independent published East Antarctica–Africa–South America rotations are considered. The lack of closure may be overcome by considering relative motion between the Antarctic Peninsula and East Antarctica until 118 Ma time, an important component of convergence. 相似文献
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Thick (∼800 m) basaltic successions from the eastern Antarctic Peninsula have been dated in the interval 180–177 Ma and preserve a transition from a continental margin arc to a back-arc extensional setting. Amygdaloidal basalts from the Black Coast region of the eastern margin of the Antarctic Peninsula represent a rare onshore example of magmatism associated with back-arc extension that defines the early phase of Weddell Sea rifting and magmatism, and Gondwana breakup. The early phase of extension in the Weddell Sea rift system has previously been interpreted to be related to back-arc basin development with associated magnetic anomalies attributed to mafic-intermediate magmatism, but with no clearly defined evidence of back-arc magmatism. The analysis provided here identifies the first geochemical evidence of a transition from arc-like basalts to the development of depleted back-arc basin basalts in the interval 180–177 Ma. The exposed Black Coast basaltic successions are interpreted to form a minor component of magmatism that is also defined by onshore sub-ice magnetic anomalies, as well as the extensive magnetic anomalies of the southern Weddell Sea. Back-arc magmatism is also preserved on the Falkland Plateau where intrusions postdating 180 Ma are associated with early phase rifting in the Weddell Sea rift system. Back-arc extension was probably short-lived and had ceased by the time the northern Weddell Sea magmatism was emplaced (<175 Ma) and certainly by 171 Ma, when an episode of silicic magmatism was widespread along the eastern Antarctic Peninsula. Previous attempts to correlate mafic magmatism from the eastern Antarctic Peninsula to the Ferrar large igneous province, or, as part of a bimodal association with the Chon Aike silicic province are both dismissed based on age and geochemical criteria. 相似文献
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The purpose of the present study was to study the tectonics of the Yellow Sea. Although oil- gas exploration has been undertaken for more than 30 years in the southern Yellow Sea, the exploration progress has achieved little. There are three tectonic periods with near N–S trending shortening and compression (260–200 Ma, 135–52 Ma and 23–0.78 Ma) and three tectonic periods with near E–W trending shortening and compression (200–135 Ma, 52–23 Ma and 0.78 Ma) at the Yellow Sea and adjacent areas during the Mesozoic and Cenozoic. The Indosinian tectonic period is the collision period between the Sino-Korean and Yangtze Plates, which formed the basic tectonic framework for the Yellow Sea area. There were strong intraplate deformations during the Yanshanian (200–135 Ma) and Sichuanian (135–52 Ma) periods with different tectonic models, which are also the main formation periods for endogenic metallic mineral deposits around the Yellow Sea. The three tectonic periods during the Cenozoic affect important influences for forming oil-gas reservoirs. The Eocene–Oligocene (52–23 Ma) is the main forming period for oil-gas sources. The Miocene–Early Pleistocene (23–0.78 Ma) was a period of favorable passage for oil-gas migration along NNE trending faults. Since the Middle Pleistocene (0.78 Ma) the NNE trending faults are closed and make good conditions for the reservation of oil-gas. The authors suggest that we pay more attention to the oil-gas exploration at the intersections between the NNE trending existing faults and Paleogene– Neogene systems in the southern Yellow Sea area. 相似文献
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大中条地区重磁场特征及其断裂分布与构造单元 总被引：1，自引：0，他引：1
大中条地区是我国著名的铜、金、铁矿集区,区内各类矿床的分布与该区的构造演化有关,并受构造体系、岩浆活动等地质因素控制。因此,系统研究本区的断裂分布和构造单元是预测隐伏矿床的基础。本文通过对大中条地区重、磁场特征研究,系统推断了该区断裂分布并划分了构造单元。对重、磁场特征的研究表明,布格重力异常与化极磁力异常均呈现东西分带的特征,这是大中条地区前寒武纪、中生代和新生代三期构造演化的综合反映。研究中利用重、磁位场边缘识别技术推断出11条断裂,对断裂的研究表明,大中条地区断裂以NE向和NW向为主,大多形成于元古代和中生代,多数断裂表现出多期活动的特点。综合重、磁场特征,构造演化特征及断裂分布,大中条地区可划分为4个一级构造单元和7个二级构造单元,构造单元控制了矿床的成因和分布。上述研究成果对大中条地区构造划分和矿产资源勘查提供了地球物理依据。 相似文献
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基于区域地质-地球物理综合研究, 利用最新实测的航空重磁综合测量数据, 结合野外踏勘与物性测量结果, 采用化极、向上延拓、垂向导数等场源分离或异常提取技术, 研究了大杨树盆地南部及周边不同类型岩浆岩的重磁异常响应, 圈定了其空间分布范围, 揭示了区域岩浆岩发育特征、分布规律及其控制因素。研究表明, 研究区不同类型的岩浆岩具有迥然不同的航磁异常特征; 本次采用的突出局部重磁异常的地球物理方法可以有效识别酸性、中酸性、中基性等岩浆岩; 本次系统圈定了具有地质意义的岩浆岩百余处, 多数岩浆岩沿北东向与北西向断裂及其两侧分布, 尤以断裂交汇部位最为发育, 说明断裂对岩浆活动具有明显的控制作用; 航空重磁揭示研究区发育较大规模的隐伏中基性火山岩, 为区域基础地质研究和火山岩盆地油气藏资源评价提供了重要的地质-地球物理依据。 相似文献
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红海是地球上最年轻的大洋,其板块构造活动正处于威尔逊旋回的幼年期。红海南北两端分别连接着威尔逊旋回的胚胎期和终结期,即东非大裂谷和地中海。这一独特的地理位置和构造部位使其成为板块构造理论研究的圣地。本文通过对已有的地质、地球物理和地球化学资料进行综合分析,了解了红海地区的地形、重磁异常和沿脊的玄武岩地球化学组成等地质构造特征,探讨了红海裂谷的洋壳分布、地幔源区不均一性以及扩张演化历史等问题。红海地形中间深、南北两端浅,可以分为北、中北、中南、南等四段。重磁异常的条带主要出现在中南段,其他段不明显,因而限制了以往对红海扩张历史的认识。目前认为红海全段存在洋壳,红海两岸的沿岸悬崖是共轭扩张陆缘,呈向南开口的喇叭型扩张,而非对应红海岸线的梭子型。红海裂谷沿脊的地幔源区具有明显的不均一性,南段玄武岩显示E-MORB特征,表现为阿法尔地幔柱的影响。红海的发育经历了裂谷前火山作用(31~29Ma)、大陆张裂(29~13Ma)和洋底扩张(<13Ma)三个主要阶段。红海裂谷的形成演化与非洲大陆的裂解、阿法尔地幔柱的活动、新特提斯洋的闭合等密切相关,了解红海的地球动力学过程将为揭示区域大地构造演化以及板块运动规律提供依据。 相似文献
19.
南薇西盆地重磁场特征及油气资源远景 总被引：1，自引：1，他引：0
结合南薇西盆地及邻区的重、磁力异常特征分析与综合反演,文章对该区油气有利远景区进行了预测。南薇西盆地北部坳陷和北部隆起以高重高磁特征为主,火山活动强烈。中部坳陷、南部隆起及南部坳陷的北部表现为整体低重、低磁背景上的局部团块状高重、高磁异常,为火山岩与碳酸盐台地的综合反映。南薇西盆地新生界厚度呈北东向条带状薄厚相间的特征,南部坳陷新生界厚度最大,中部坳陷次之。盆地北部处于莫霍面隆起区,而南部莫霍面相对较深,为减薄型陆壳的特征。北部坳陷和北部隆起居里面整体较浅,可能与南海扩张引起岩石圈的强烈伸展减薄、地幔物质上侵有关。中部坳陷和南部隆起的居里面明显浅于南部坳陷,表明中部坳陷和南部隆起的热活动强于南部坳陷。重磁场特征及其反演结果与石油地质特征表明,南薇西盆地的中部坳陷、南部隆起及其西南盆地外围的区域应为盆地最好的油气远景区,其次为南部坳陷,北部坳陷和北部隆起油气潜力不大。在油气远景区内,局部团块状、等轴状的重力高异常区部分可能为碳酸盐台地,生物礁较为发育,应为未来的勘探目标。 相似文献
20.
Fan Zhang Xubo Zhang Weiwei Ding Tingting Wang Jian Zhu 《International Geology Review》2020,62(7-8):840-858
ABSTRACT We investigated the oceanic crustal structure and lithospheric dynamics of the South China Sea (SCS) basin through a comprehensive analysis of residual gravity anomaly and bathymetry combined with seismic constraints and interpretation from geodynamic modelling. We first calculated the residual mantle Bouguer anomaly (RMBA) of the oceanic crustal regions of the SCS by removing from free-air gravity anomaly the predicted gravitational attractions of water-sediment, sediment-crust, and crust-mantle interfaces, as well as the effects of lithospheric plate cooling, using the latest crustal age constraints including IODP Expedition 349 and recent deep-tow magnetic surveys. We then calculated models of the gravity-derived crustal thickness and calibrated them using the available seismic refraction profiles of the SCS. The gravity-derived crustal thickness models correlate positively with seismically determined crustal thickness values. Our analysis revealed that the isochron-averaged RMBA are consistently more negative over the northern flank of the SCS basin than the southern conjugate for magnetic anomaly chrons C8n (~25.18 Ma) to C5Dn (~17.38 Ma), implying warmer mantle and/or thicker crust over much of the northern flank. Computational geodynamic modelling yielded the following interpretations: (1) Models of asymmetric and variable spreading rates based on the relatively high-resolution deep-tow magnetic analysis would predict alternating thicker and thinner crust at the northern flank than the southern conjugate, which is inconsistent with the observed systematically thicker crust on the northern flank. (2) Models of episodic southward ridge jumps could reproduce the observed N-S asymmetry, but only for crustal age of 23.6–20 Ma. (3) Southward migration of the SCS ridge axis would predict slightly thinner crust at the northern flank, which is inconsistent with the observations. (4) Models of higher mantle temperatures of up to 25–50°C or >2% less depleted mantle sources on the northern flank could produce large enough anomalies to explain the observed N-S asymmetries. 相似文献