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121.
利用新近获得的子午面磁盔-电流片背景太阳风稳态解,对激波从盔底沿电流片方向往外传播时与磁盔间的相互作用进行了数值模拟研究,重要新结果是:1.磁盔的存在使受扰介质速度跃变中央出现下凹,随着激波传出磁盔区并沿电流片方向传播,速度下凹逐渐减弱以致消失;2.激波将磁盔拉长并把盔顶的环形(垂直赤道面)磁场带到行星际空间,成为行星际磁场南向分量的来源之一;3.5个太阳半径(R⊙)内的磁盔部分将出现精细结构,沿盔外边界形成两条高速带,以及马蹄形密度(亮)环形结构等.这些结果表明,太阳附近高速等离子体与磁盔间存在重要的动力学相互作用过程,对行星际空间的太阳风三维结构有重要影响. 相似文献
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地磁偏角实时自动修正技术在油田定向钻井中的应用 总被引:2,自引:1,他引:2
在油田定向钻井的磁导向定位系统中,地磁偏角校正是一个不可缺少的基本要素,同时在磁偏角校正值精度直接影响定向井的导向定位精度。因此,作者提出了提高地磁偏角校正值精度的方法,并试图将地磁偏角实时自动修正技术引入我国油田定向钻井领域。 相似文献
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The time-domain EM induction response of non-magnetic and magnetic targets can be approximated using a conductive permeable prism composed of six faces of conductive plates, each face being composed of a set of conductive ribbons. The effect of magnetic permeability is included by the use of two “apparent flux gathering” coefficients, and two “effective magnetic permeability” coefficients, in the axial and transverse directions. These four magnetic property coefficients are a function of physical properties and geometry of the target, but are independent of prism orientation relative to a transmitter. The approximation algorithm is computationally fast, allowing inversions for target parameters to be achieved in seconds. The model is tested on profiles acquired with a Geonics EM63 time-domain EM metal detector over a non-magnetic copper pipe target, and a steel artillery shell in horizontal and vertical orientations. Results show that this approximation to a permeable prism has a capability of fitting geometric, conductivity and magnetic parameters at both early and late sample times. The magnetic parameters show strong change from early to late times on the EMI decay curve, indicating that the magnetic properties of the target have non-linear characteristics. It is proposed that these magnetic parameters and the nature of their non-linearity may carry additional discrimination information for distinguishing between intact munitions and scrap in UXO studies. 相似文献
128.
J.-F. Girard M. Boucher A. Legchenko J.-M. Baltassat 《Journal of Applied Geophysics》2007,63(3-4):103-116
Karstic conduits play a crucial role for water supply in many parts of the world. However, the imaging of such targets is generally a difficult task for most geophysical methods. Magnetic Resonance Sounding (MRS) is a geophysical method designed for imaging of water bearing structures. Initially, MRS was developed for characterizing horizontally stratified aquifers. However, when applying a 1D MRS measuring setup to the imaging of 2D–3D targets, the size of which may be much smaller than the loop, the accuracy and the lateral resolution may not be sufficient. We have studied the possibility of simultaneously processing several MRS aligned along a profile to perform a Magnetic Resonance Tomography (MRT). This work emphasizes the gain of resolution for 2D–3D imagery of MRT versus the interpolation of 1D inversion results of MRS along the same profile. Numerical modelling results show that the MRT response is sensitive to the size and location of the 2D target in the subsurface. Sensitivity studies reveal that by using the coincident transmitting/receiving (TX/RX) setup and shifting the loop around the anomaly area, the depth, section and position of a single karstic conduit with a size smaller than the MRS loop size can be resolved. The accuracy of the results depends on the noise level and signal level, the latter parameter being linked to the depth and volume of the karstic conduit and the water content in the limestone matrix. It was shown that when applying MRT to the localization of 2D anomalies such as karstic conduits, the inclination of the geomagnetic field, the orientation of the MRT profile and the angle of crossover of the conduit by the MRT profile must be taken into account. Otherwise additional errors in interpretation should be expected. A 2D inversion scheme was developed and tested. Both numerical and experimental results confirm the efficiency of the developed approach. 相似文献
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A Least-squares Window Curves Method for Interpretation of Magnetic Anomalies Caused by Dipping Dikes 总被引:1,自引:0,他引:1
E. M. Abdelrahman E. R. Abo-Ezz K. S. Soliman T. M. El-Araby K. S. Essa 《Pure and Applied Geophysics》2007,164(5):1027-1044
We have developed a least-squares method to determine simultaneously the depth and the width of a buried thick dipping dike
from residualized magnetic data using filters of successive window lengths. The method involves using a relationship between
the depth and the half-width of the source and a combination of windowed observations. The relationship represents a family
of curves (window curves). For a fixed window length, the depth is determined for each half-width value by solving one nonlinear
equation of the form f (z) = 0 using the least-squares method. The computed depths are plotted against the width values representing a continuous curve.
The solution for the depth and the width of the buried dike is read at the common intersection of the window curves. The method
involves using a dike model convolved with the same moving average filter as applied to the observed data. As a result, this
method can be applied to residuals as well as to measured magnetic data. Procedures are also formulated to estimate the amplitude
coefficient and the index parameter. The method is applied to theoretical data with and without random errors. The validity
of the method is tested on airborne magnetic data from Canada and on a vertical component magnetic anomaly from Turkey. In
all cases examined, the model parameters obtained are in good agreement with the actual ones and with those given in the published
literature. 相似文献