共查询到19条相似文献，搜索用时 190 毫秒
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2D磁异常分步反演方法是利用二维(剖面)磁测数据确定场源几何参数以及物性参数的一种反演方法,该方法的优点是构造的形态函数S不受场源磁化特征的影响,因此可以在未知场源物性参数的前提下,通过拟合依次反演得到磁性源形体横截面几何参数、磁化强度以及磁化方向.本文阐述了2D磁异常分步反演方法的原理及步骤,对形态函数S的特征及求取方法进行了讨论,分析了区域背景干扰(正常场)对反演结果的影响并提出了初步解决方案.在方法研究的基础上,进行了单一理论模型及组合理论模型的试算,得到了较好的反演结果.为了验证该方法的效果,对实测剖面进行了试算,得到了场源的边界及场源埋深信息,为进一步反演提供了有用的参考. 相似文献
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谱矩方法可以对数据的表面形貌做较为细致的描述.它以随机过程为理论基础,用各阶谱矩及统计不变量等具体的参数表征表面的几何形态,算术平均顶点曲率是一种基于四阶谱矩的统计不变量.通常,埋深不同的场源所引起的磁异常尺度不同,从曲率的角度来理解即为磁异常曲面的弯曲程度不同.因此,本文应用算术平均顶点曲率提取磁异常的几何信息,并将所提取的信息用于场源深度的反演.理论上推导了基于谱矩的球状磁源体和板状磁源体的反演公式,得到了场源深度与磁异常、曲率之间的关系式.结合理论模型计算验证了方法的有效性,并与欧拉反褶积方法进行对比.与传统的方法相比,该方法快速简单,无需调节参数,且有较好的反演精度.最后,将该方法用于塔里木盆地航磁异常的反演和解释中,反演出的磁源体深度可满足区域磁异常数据分析和解释的要求,为克拉通沉积盆地磁异常源的深度划分提供丰富的信息. 相似文献
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《地球物理学进展》2020,(4)
本文提出了一种基于航磁垂向分量数据提取磁性场源体深度的方法.从垂直磁化条件下球体模型垂向分量的正演理论出发,给出了利用垂向分量极大值获取异常体埋深的关系式,并在此基础上推导了约束条件下垂向分量深度识别关系式.该关系式简化了场源深度识别的复杂度,充分利用先验信息且无需进行复杂反演运算,能够较为精确地计算异常体的埋深,为磁性场源体深度的提取提供了一种新的解决方案.理论模型试验证明,利用本文提出的深度识别方法进行深度估算的相对误差绝对值均小于1%,相较于常规的垂向分量极大值方法具有更高的估算精度.将该方法应用于中国北部某地区实测航磁垂向分量数据,获取的深度结果与钻孔资料相一致,深度相对误差绝对值小于10%,验证了本文方法对于实际资料的有效性. 相似文献
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Theta图是利用位场(重磁)数据识别边界的常用方法,其表达式为重磁异常水平变化与垂直变化的比值函数.该方法计算浅源地质体边界的效果较好,而由于深源位场数据在换算过程中会产生趋同效应,在深源地质体识别应用中计算结果不准确,为此,本文提出Theta-Depth法并进行地质体埋深的计算.首先给出直接利用Theta图像进行场源体深度估算的方法,然后推导出基于Theta导数的线性方程来自动估算场源位置参数,本文方法可有效地利用Theta图像的特征为约束条件来提高反演结果的精度.理论模型试验证明本文提出的Theta-Depth法能有效地计算出场源体位置和深度.将该方法应用于满都拉地区实测磁数据的解释,帮助圈定了矿脉的分布. 相似文献
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《应用地球物理》2016,(2)
Tilt-depth法可以用于快速反演磁源的上顶埋深,但其无法反演磁源底部深度,同时该方法的反演解过于单一。针对于此,本文在有限厚度台阶磁异常导数公式基础上,推导出了可以同时反演地质体上、下界面埋深的改进型Tilt-depth法计算公式,并采用在Tilt梯度图上选取多特征点进行联合反演的计算模式来提高反演解的可靠性。二维及三维组合模型试验均证实了改进型Tilt-depth法可以有效地反演出磁性体的上顶与下底深度,且上顶埋深的反演精度明显高于常规方法的。最后将改进型Tiltdepth法用于松辽盆地长岭断陷航磁数据反演,其上顶埋深的反演结果与钻孔钻遇火山岩的深度基本一致,证实改进型Tilt-depth法相对于常规方法的反演结果更加准确。 相似文献
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《地球物理学报》2021,64(6)
三维磁异常快速反演是磁法勘探进行地质解释的一项重要内容.本文在方向tilt梯度基础上进行导数处理,并进行合理改进,得到了6个改进的方向tilt梯度导数,丰富了不同方向上的磁异常信息.对常规欧拉反褶积方程进行三个方向求导,所构成的方程组与6个改进的方向tilt梯度导数进行结合,从而构建出了两个基于方向tilt梯度导数的快速反演方程组(方向tilt-Euler法),用于反演场源的位置参数.另外,将三个方向导数下的欧拉反褶积进行平方和及均方根处理,得到了场源构造指数的求解公式.单一模型试验表明,6个改进的方向tilt梯度导数异常基本不受磁化方向影响,可从不同方向上反映磁异常信息,方向tilt-Euler能够准确地反演出场源的位置及构造指数.叠加模型试验证实了方向tilt-Euler法相对于tilt-Euler法,具有反演解聚集度更强、连续性更好、反演准确度更高、受噪声影响更小及无虚假反演解等优点.将本文方法应用于内蒙古塔木素航磁资料处理中,获得了丰富的地下磁源分布信息,为了解该地区隐伏断裂构造及岩体分布等提供了有效依据. 相似文献
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南海重磁异常特征及火成岩分布(英文) 总被引：8，自引：1，他引：7
南海火成岩油气藏具有广阔的勘探前景,综合利用地球物理方法圈划与识别火成岩体、研究火成岩分布是火成岩油气藏研究的基础。针对南海重磁场特征,采用低纬度、变倾角化极技术进行了磁异常化极处理,利用优选延拓方法实现重磁异常分离并提取南海海域浅部火成岩重磁异常信息,利用磁异常三维相关成像给出南海火成岩的三维空间等效分布,在重磁梯度突出局部异常边界信息的基础上,通过梯度加权的重磁相关分析勾画不同类型火成岩的平面展布,火成岩的分布特征显示出受地壳深部结构及断裂构造的控制与影响。 相似文献
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The inversion of density structure by graphic processing unit (GPU) and identification of igneous rocks in Xisha area 
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下载免费PDF全文 Organic reefs, the targets of deep-water petroleum exploration, developed widely in Xisha area. However, there are concealed igneous rocks undersea, to which organic rocks have nearly equal wave impedance. So the igneous rocks have become interference for future exploration by having similar seismic reflection characteristics. Yet, the density and magnetism of organic reefs are very different from igneous rocks. It has obvious advantages to identify organic reefs and igneous rocks by gravity and magnetic data. At first, frequency decomposition was applied to the free-air gravity anomaly in Xisha area to obtain the 2D subdivision of the gravity anomaly and magnetic anomaly in the vertical direction. Thus, the distribution of igneous rocks in the horizontal direction can be acquired according to high-frequency field, low-frequency field, and its physical properties. Then, 3D forward modeling of gravitational field was carried out to establish the density model of this area by reference to physical properties of rocks based on former researches. Furthermore, 3D inversion of gravity anomaly by genetic algorithm method of the graphic processing unit (GPU) parallel processing in Xisha target area was applied, and 3D density structure of this area was obtained. By this way, we can confine the igneous rocks to the certain depth according to the density of the igneous rocks. The frequency decomposition and 3D inversion of gravity anomaly by genetic algorithm method of the GPU parallel processing proved to be a useful method for recognizing igneous rocks to its 3D geological position. So organic reefs and igneous rocks can be identified, which provide a prescient information for further exploration. 相似文献
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The inversion of density structure by graphic processing unit （GPU） and identification of igneous rocks in Xisha area 总被引：1，自引：0，他引：1
Organic reefs, the targets of deep-water petroleum exploration, developed widely in Xisha area. However, there are concealed igneous rocks undersea, to which organic rocks have nearly equal wave impedance. So the igneous rocks have become interference for future exploration by having similar seismic reflection characteristics. Yet, the density and magnetism of organic reefs are very different from igneous rocks. It has obvious advantages to identify organic reefs and igneous rocks by gravity and magnetic data. At first, frequency decomposition was applied to the free-air gravity anomaly in Xisha area to obtain the 2D subdivision of the gravity anomaly and magnetic anomaly in the vertical direction. Thus, the distribution of igneous rocks in the horizontal direction can be acquired according to high-frequency field, low-frequency field, and its physical properties. Then, 3D forward modeling of gravitational field was carried out to establish the density model of this area by reference to physical properties of rocks based on former researches. Furthermore, 3D inversion of gravity anomaly by genetic algorithm method of the graphic processing unit(GPU) parallel processing in Xisha target area was applied, and 3D density structure of this area was obtained. By this way, we can confine the igneous rocks to the certain depth according to the density of the igneous rocks. The frequency decomposition and 3D inversion of gravity anomaly by genetic algorithm method of the GPU parallel processing proved to be a useful method for recognizing igneous rocks to its 3D geological position. So organic reefs and igneous rocks can be identified, which provide a prescient information for further exploration. 相似文献
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本文提出了能提高异常体分辨能力,同时得到绝对电导率的地面磁电阻率数据三维反演方法.磁电阻率响应用准直流的低频磁场代替;数值模拟由频率域电场满足的Helmholtz方程出发,采用三维交错网格有限差分法;长直导线源作为发射源,其中源的计算包含在背景场中;结合地面磁电阻率数据各分量的特点,选择y分量进行反演研究;反演采用三维非线性共轭梯度反演技术,为了提高异常体的深度分辨能力,进行迭代重构反演;用印模法对初始模型进行重构,采用的是辅模型在浅部,元模型在深部的组合方式.从合成数据和实际数据的反演结果可以得到以下的认识:(1)由频率域麦克斯韦方程组出发,低频磁场数据反演可以直接得到电导率,而不是相对电导率之比;(2)采用印模法组合初始模型,进行迭代重构反演,可以提高地面磁电阻率数据反演对异常体的分辨能力,确定埋深位置,同时不会丧失对于浅部异常体的分辨能力;(3)在结合印模法的地面磁电阻率数据三维反演中,深部异常体的分辨能力受地表不均匀导电体影响较小;(4)确定印模深度可以采用上一次重构反演结束时的模型变化量,通过相邻两次重构反演结束时的模型变化量之差来确定迭代重构是否终止.因为静磁场与重力场在数学上的相似性,本文的反演方法可以被运用到重力场等位场的地面数据的反演中. 相似文献
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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
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Petar Stavrev 《Geophysical Prospecting》2006,54(2):153-166
The calculable magnitudes of the anomalous magnetic field from simple 2D sources and their gradients and Laplacians appear as ratios that can be synthesized in functional forms, corresponding to the different source shapes. Field components and first‐order derivatives are involved in the inversion procedures presented. The structural index and source depth are estimated independently of each other. The applied functions allow magnetic profiles and magnetic maps to be shape‐ and depth‐converted with immediate imaging of the inversion results. The contours of these functions outline elongated loops around the 2.5D anomaly axis on magnetic maps. The width of the loops reflects the depth and structural index N of the source in the scale units of the inverted map. Model and field tests illustrate the effectiveness of this approach for fast automatic inversion of large sets of magnetic data for depth, shape, length and location of simple sources. 相似文献
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We presented a new method for interpreting 2D magnetic data, called direct analytic signal (DAS) method, which directly used the analytic signal of magnetic anomaly to compute the depth and the structural index of the source. The DAS method needs only the computation of the first order derivatives of magnetic anomaly, so that the inversion results are more stable than the results obtained by the other existing analytic signal methods. The DAS method is tested on synthetic magnetic data with and without noise, and the DAS method can successfully obtain the depth and the structural index of the source. We also applied the DAS method to interpret a real magnetic data over a shallow geological source whose source parameters are known from closely drilling information, and the inversion results are in accord with the true values. 相似文献
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This paper presents a new inversion method for the interpretation of 2D magnetic anomaly data, which uses the combination of the analytic signal and its total gradient to estimate the depth and the nature (structural index) of an isolated magnetic source. However, our proposed method is sensitive to noise. In order to lower the effect of noise, we apply upward continuation technique to smooth the anomaly. Tests on synthetic noise-free and noise corrupted magnetic data show that the new method can successfully estimate the depth and the nature of the causative source. The practical application of the technique is applied to measured magnetic anomaly data from Jurh area, northeast China, and the inversion results are in agreement with the inversion results from Euler deconvolution of the analytic signal. 相似文献
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The interpretation of the Jarrafa magnetic and gravity highs, NW Libyan offshore, suggests that it may be caused by a body of high-density and high magnetization. Analysis of their power spectra indicates two groups of sources at: (1) 2.7 km depth, probably related to the igneous rocks, some of which were penetrated in the JA-1 borehole, (2) 5 km depth, corresponding to the top of the causative body and (3) 10 km depth, probably referring to the local basement depth. The boundary analysis derived from applied horizontal gradient to both gravity and magnetic data reveals lineaments many of which can be related to geological structures (grabens, horsts and faults).The poor correlation between pseudogravity fields for induced magnetization and observed gravity fields strongly suggests that the causative structure has a remanent magnetization (D = −16°, I = 23°) of Early Cretaceous age, fitting with the opening of the Neo Tethys 3 Ocean.Three-dimensional interpretation techniques indicate that the magnetic source of the Jarrafa magnetic anomaly has a magnetization intensity of 0.46 A/m, which is required to simulate the amplitude of the observed magnetic anomaly. The magnetic model shows that it has a base level at 15 km.The history of the area combined with the analysis and interpretation of the gravity and magnetic data suggests that: (1) the source of the Jarrafa anomaly is a mafic igneous rock and it may have formed during an Early Cretaceous extensional phase and (2) the Jarrafa basin was left-laterally sheared along the WNW Hercynian North Graben Fault Zone, during its reactivation in the Early Cretaceous. 相似文献