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采用递推矩阵方法计算各向异性介质的磁流源并矢Green函数,并利用上述并矢Green函数对层状各向异性倾斜地层中多分量感应测井的响应进行数值模拟,分析了线圈距、层厚、倾角和围岩对多分量感应测井响应的影响.计算发现,共面视电导率比共轴视电导率变化规律复杂,不能反映地层电导率的真实情况.各向异性地层共轴视电导率随井眼相对倾角的增加而减小,而共面视电导率随井眼相对倾角的增加而增加.仪器的垂向分辨率、围岩各向异性对目的层响应的影响程度取决于线圈距,围岩各向异性对高电导率目的层中测井响应的影响大于对高电阻率目的层中测井响应的影响. 相似文献
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本文采用广义反射系数法推导了水平层状各向异性地层中电磁场的积分解析解,并利用快速汉克尔变换技术实现了三维感应仪器测井响应的快速计算.三维感应测井响应与地层水平电导率、垂直电导率和井斜角及仪器方位角同时有关,单一分量的测井曲线不能满足资料解释的需要.通过对仪器测量分量响应特征的考察,本文提出了一种基于组合量测井曲线的资料直观解释方法.数值模拟显示,交叉分量相关组合量可准确划分地层纵向边界,并可直观识别各向异性层;与单独分量相比,主分量相关组合量提高了纵向分辨率、减弱了与地层电导率参数的非线性关系. 相似文献
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《地球物理学进展》2015,(4)
地层电阻率是影响油气或煤层气评价的重要参数,水平井中常利用感应测井确定地层电阻率,由于水平井与直井测量环境有较大差异,响应方式势必与直井不同.水平井测井响应的环境影响复杂,不能使用基于几何因子的信号处理,必须通过三维正演数值模拟方法研究响应特征.本文利用基于有限元方法的COMSOL Multiphysics软件对三层对称地层模型中的水平井感应测井响应进行了数值模拟分析.通过分析比较源距为0.3m、0.6m、0.9m、1.2m的四个水平线圈系的响应特征发现,不同源距的线圈系测得的电导率值受仪器位置、上下围岩电导率、目的层厚度和仪器偏心的影响规律不同.数值模拟结果对水平井的解释工作及仪器研发具有指导性意义. 相似文献
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随着复杂油气田的广泛勘探,对测井技术提出了新的要求,阵列感应电阻率的出现可得到较准确的地层真电阻率,但我国的阵列感应电阻率测井仪主要依赖进口,限制了我测井不能在与仪器供给商有利益冲突的国家或地区进行同类作业服务.本文介绍了5频等参数阵列相位感应电阻率测井仪器原理、设计流程,与常规感应电阻率、俄罗斯VIKIZ测井资料的对比.阵列相位差感应电阻率测井仪较好的解决了常规感应测井仪器中存在的纵向分辨率差、径向探测深度浅、井眼影响大、不能解决复杂侵入剖面等问题,具有较好的分辨能力,适合于水淹层测井、薄层测井、剩余油测井. 相似文献
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《地球物理学进展》2016,(2)
本文提出的瞬态感应测井是一种以瞬变电磁激发为基础的感应测井方法.其工作波形是瞬态的:有一个主频并有一定的带宽.发射探头是线圈,激发的感应电动势与感应测井一样沿圆周方向.具体激发频谱取决于与其配合的声波测井压电换能器参数.当换能器是宽带时,激发的瞬变电磁场是宽带的,激发波形的电震荡周期比较少,测量的电磁感应波形的震荡周期也比较少.这些震荡波形从激发时刻便开始出现,只能够用同轴的线圈进行接收.同样,接收信号中也包含直接耦合信号和二次场信号,两者相差90°.当地层的电导率随频率改变时,接收波形中二次场的响应波形幅度和相位均发生改变.对接收波形可以参考感应或阵列感应测井的处理方法,用Doll几何因子进行设计.但是,需要面对不同频率的幅度和相位,增加解耦处理方法.相对于阵列感应测井,该测井方法有两个优点:能够测量一个频带内地层的电阻率,能够与阵列声波测井从探头结构上进行组合,便于测井系统的集成. 相似文献
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为了提高随钻电磁波测井仪器的抗震能力,仪器传感器中所有发射与接收线圈均安装在柱状金属钻铤上的环状刻槽中,同时槽中充填高磁导率的铁氧体,以提高发射和接收效率.本文针对多环状刻槽钻铤中发射与接收线圈分布,研究建立一套随钻电磁响应的混合模拟算法.首先,根据环状刻槽几何尺寸以及轴向边界,将整个钻铤与外部的井眼和地层划分成多个不同电导率和磁导率分布的轴对称非均质各向同性层状模型,并应用混合法建立层状非均质地层中电磁场的半解析解与各个线圈上感应电动势的计算方法.其次,利用摄动原理给出随钻电磁测井中振幅比与相位差的空间灵敏度计算公式.然后,通过数值结果考察铁氧体磁导率和地层电导率变化对发射线圈的发射功率和接收线圈上感应电动势的影响,并确定各个接收线圈上感应电动势的动态变化范围,为仪器设计过程中选择合适的铁氧体提供理论依据.最后,通过空间灵敏度分布特征考察振幅比与相位差在探测特征上的差异. 相似文献
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应用模式匹配算法研究建立水平层状非均质横向同性地层中多分量感应测井响应的快速算法.首先,利用Fourier级数展开法将多分量感应响应的数值模拟转化为三个轴对称问题,并利用电阻率径向导数的奇异表达式,引入两个附加奇异微分算子,用于描述柱状分界面上的积累面电荷对共面线圈系电磁响应的影响.然后通过模式匹配算法求解轴对称问题,得到水平层状非均质横向同性地层中多分量感应磁场的半解析解以及测井响应计算方法,最后通过数值模拟结果对该算法进行检验并进一步考察阵列多分量感应仪器的响应特征. 相似文献
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本文针对中国石油集团测井有限公司(CPL)三维阵列感应测井仪器(Three Dimensional Induction Tool,TDIT)的真实结构与参数,利用2.5维数值模式匹配技术研究建立水平层状非均质TI地层中仪器偏心情况下三维感应测井响应的高效数值模拟算法.首先,利用2.5维数值模式匹配技术给出水平层状非均质TI模型中偏心磁流源并矢Green函数的半解析解.在此基础上,结合三维阵列感应测井仪器参数以及测量过程中出现的仪器偏心与旋转等实际情况,通过叠加原理推导出该仪器响应的有效计算公式.最后,通过数值模拟结果分析考察仪器偏心、仪器自旋角等参数对测井响应的影响以及变化特征,为多分量感应资料处理与解释提供理论基础. 相似文献
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用有限差分法计算各向异性介质中多分量感应测井的响应 总被引：16，自引：5，他引：11
感应测井电阻率是砂泥岩储层中定量评价含油气性的主要参数之一,然而由于储层电各向异性的存在,传统的感应测井仪得到的电阻率主要响应地层的水平电阻率,比地层的垂直电阻率小,由此计算的含水饱和度偏高．多分量感应测井则可以通过不同方向的发射和接收,测量多个分量,弥补上述缺陷,为储层的含油气性评价提供准确信息．本文用交错网格有限差分法导出了主轴各向异性介质中Maxwell方程的离散化关系式,计算了三维各向异性介质中多分量感应测井的电磁响应．利用三层模型的数值模拟,分析了不同磁场分量对各向异性介质的响应特性,用多层模型和倾斜各向异性地层的响应计算检验了所编制的交错网格有限差分法程序． 相似文献
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The determination of the coefficient of viscosity of eruptive products gives useful elements to the knowledge of possible variations of composition and physical conditions of the magmas. 相似文献
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As is known, the secular deceleration of the Earth's diurnal rotation is explained mainly by the tidal friction in the ocean. Below we consider this mechanism in some detail, taking into account also elastic deformations of the mantle under the action of ocean loading and the interaction between the tide-generating body, ocean tidal wave, liquid outer core, and solid inner core. It is shown that elastic displacements of the core-mantle boundary under the action of ocean loading are of about the same amplitude and phase as the elastic loading displacements of the Earth's outer surface. As a result, side by side with the mechanism of secular deceleration of diurnal rotation of the mantle, there are also (1) the opposite mechanism of secular acceleration of diurnal rotation of the outer liquid core and of the solid inner core and (2) the mechanism of excitation of differential rotation in the liquid core. Taking these effects into account, we compare theoretical and modern observed data on the eastward drift of the solid inner core. It is shown that the best agreement may be obtained if the turbulent viscosity of the liquid core is about 2 × 10
3
Poise 相似文献
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The nutations of the planets Mars andEarth are investigated and compared. Alarge number of interior structureparameters are involved in the nutationcomputations. The comparison between the observations and the computationsprovides several constraints on these parmeters andtherefore allows a better understanding of the physics of the interior of theplanet. For the Earth, the high precision of the observations of the nutationshas led to a very good determination of interior properties of the planet. ForMars, observations of nutations are not yet available, and we review how theamplitude of the Martian nutations depends on the hypotheses consideredfor its interior. Although Mars is very similar to the Earth, its interior is not well known;for example, we don't knowif its core is liquid or solid. Only if the core is liquid,the Free Core Nutation (FCN) normal mode exists and can alter the nutationswhich are close to the resonance. From the observed geoids, it is known thatboth planets are not in hydrostatic equilibrium. The departure is larger forMars than for the Earth, and consequently, the implication of considering a convective mantle instead of a mantle in hydrostatic equilibrium described byClairaut's equation for the initial equilibrium state of the planet is largeron the Martian nutations than on the Earth nutations. The consequences of theuncertainty in the core dimensions are also examined and shown to be of a veryhigh influence for Mars if the core is liquid, due to the potential changes inthe FCN resonance. The influence of the presence of an inner core, which isknown to exist for the Earth, could be more important for Mars than for theEarth if the inner core is large. Due to the presence of Tharsis on Mars, thetriaxiality of this planet has, additionally, larger effects than on Earth. 相似文献
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Geomagnetism and Aeronomy - The magnetic evolution of the active region of the Sun at the level of the photosphere has been studied. Magnetic synoptic maps of the 2007 Kitt Peak Observatory were... 相似文献
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Studia Geophysica et Geodaetica - 相似文献
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地震激励下处于深水中的桥墩和周围水体的相互作用将对桥梁结构的动力响应产生较大影响。首先对地震作用下水-桥墩的相互作用理论做了概括,给出了动水压力对桥墩的作用效应及各自的适用范围;对主要的三种考虑流固耦合效应的分析方法做了对比,探讨了地震作用下影响水-结构相互作用的主要因素,并对今后的研究提出了建议。 相似文献
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Josef Vykutil 《Studia Geophysica et Geodaetica》1968,12(2):217-220
Резюме Дается вывод формул для вычислений длины хорды, длины и азимутов нормаляных сечений и длины геодезической линии эллипсоида.
Применяются тригонометрические функции данных величин и постоянные принятого ргфгргнц-эллипсоида, что является целесообразным
при использовании вычислителQjных машин, особенно автоматов. Рабочие формулы рекомендуются в форме (8–11).
Dedicated to Professor František Fiala on His 85th Birthday
Address: Veveři 95, Brno. 相似文献
Dedicated to Professor František Fiala on His 85th Birthday
Address: Veveři 95, Brno. 相似文献
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V. E. Pavlov T. Yu. Tolmacheva R. V. Veselovskiy A. V. Latyshev A. M. Fetisova I. V. Bigun 《Izvestiya Physics of the Solid Earth》2017,53(5):702-713
Until recently, the existing data prevented the geophysicists from accurately dating the Bysy-Yuryakh stratum, which outcrops in the middle reach of the Kotuy River, constraining the time of its formation to a wide interval from the end of the Late Cambrian to the beginning of the Silurian. The obtained paleomagnetic data unambiguously correlate the Bysy-Yuryakh stratum to the Nyaian regional stage and constrain its formation, at least a considerable part of it, by the Tremadocian. This result perfectly agrees with the data on the Bysy-Yuryakh conodonts studied in this work and yields a spectacular example of the successful application of paleomagnetic studies in solving important tasks of stratigraphy and, correspondingly, petroleum geology. Within the Bysy-Yuryakh stratum, we revealed a large normal-polarity interval corresponding to the long (>1 Ma) period when the geomagnetic reversals were absent. This result, in combination with the data for the Tremadocian and Middle–Upper Cambrian sequences of the other regions, indicates that (1) the rate of occurrence of the geomagnetic reversals on the eve of the Ordovician Moyero superchron of reversed polarity was at most one reversal per Ma; (2) the superchron does not switch on instantaneously but is preceded by a certain gradual change in the operation conditions of the dynamo mechanism which, inter alia, manifests itself by the reduction of the frequency of geomagnetic reversals with the approach of the superchron. This finding supports the views according to which a process preparing the establishment of the superchrons takes place at the core–mantle boundary. 相似文献