航空伽马能谱地形改正新方法及应用   总被引：5，自引：2，他引：5  

范正国  于长春 《物探与化探》2005,29(1):28-30,33

针对航空伽马能谱测量特点,推导了基于二维地形影响系数的航空伽马能谱测量地形逐点改正的理论公式。通过模型试验,总结了不同地形上不同飞行方式时的航空放射性异常特征,给出实测数据处理与野外异常查证对比结果,地形改正效果较好。  相似文献   

三维地震数据的方位角时差校正及其应用     

侯爱源  曾锦光 《物探化探计算技术》1998,20(3):270-273

三维地震数据的同一共中心点道集是由不同方位角的地震道组成的。当地下地层倾斜时,共中心点道集的反射同相轴就存在方位角时差。本文根据方位角时差校正（ＡＭＯ）的基本原理,从ｆ－ｋ域的正、逆ＤＭＯ出发,通过稳相法得到积分法ＡＭＯ脉冲响应的时间、振幅因子公式。把ＡＭＯ应用于一束实际三维地震数据处理,经ＡＭＯ处理后的剖面绕射波和断面反射波得到了加强,其效果是令人满意的。  相似文献   

Weak-contrast approximation of the elastic scattering matrix in anisotropic media     

Bjørn Ursin  Geir U. Haugen 《Pure and Applied Geophysics》1996,148(3-4):685-714

The plane-wave reflection and transmission coefficients at a plane interface between two anisotropic media constitute the elements of the elastic scattering matrix. For a 1-D anisotropic medium the eigenvector decomposition of the system matrix of the transformed elasto-dynamic equations is used to derive a general expression for the scattering matrix. Depending on the normalization of the eigenvectors, the expressions give scattering coefficients for amplitudes or for vertical energy flux.Computing the vertical slownesses and the corresponding polarizations, the eigenvector matrix and its inverse can be found. We give a simple formula for the inverse, regardless of the normalization of the eigenvectors. When the eigenvectors are normalized with respect to amplitudes of displacement (or velocity), the calculation of the scattering matrix for amplitudes is simplified.When the relative changes in all parameters are small, a weak-contrast approximation of the scattering matrix, based on the exactly determined polarization vectors in an average medium, is obtained. The same approximation is also derived directly from the transformed elasto-dynamic equations for a smooth vertically inhomogeneous medium, proving the consistency of the approximation.For monoclinic media, with the mirror symmetry plane parallel to the interface, the approximative scattering matrix is given in terms of analytic expressions for the non-normalized eigenvectors and vertical slownesses. For transversely isotropic media with a vertical axis of symmetry (VTI) and isotropic media, explicit solutions for the weak-contrast approximations of the scattering matrices have been obtained. The scattering matrix for amplitudes for isotropic media is well known. The scattering matrix for vertical energy flux may have applications in AVO analysis and inversion due to the reciprocity of the reflection coefficients for converted waves.Numerical examples for monoclinic and VTI media provide good agreement between the approximative and the exact reflection matrices. It is, however, expected that the approximations cannot be used when the symmetry properties of the two media are very different. This is because the approximation relies on a small relative contrast between the eigenvectors in the two media.Presented at the Workshop Meeting on Seismic Waves in Laterally Inhomogeneous Media, Castle of Trest, Czech Republic, May 22–27, 1995.  相似文献   

Comparison between a radiative wind model for be stars and high angular resolution data from the GI2T interferometer     

Ph. Stee 《Astrophysics and Space Science》1995,224(1-2):561-562

I present theoretical line profiles and intensity maps from an axi-symmetric radiative wind model from a rapidly rotating Be star. The introduction of a viscosity parameter in the latitude-dependent hydrodynamic code enables us to consider the effects of the viscous force in the azimuthal component of momentum equations (Araújo et al. 1994). Both velocity field and density law derived from the hydrodynamic equations have been used for solving the statistical equilibrium equations. By adopting the Sobolev approximation, we could easily obtain a good estimate of both electronic density and hydrogen level populations throughout the envelope. The numerical calculation was performed for parameters characterisic of the Be star Cassiopeiae.  相似文献   

活动星系核与类星体中致密天体的形成与并合：伽玛爆发与引力辐射     

王建民 《紫金山天文台台刊》1999,18(3):271-273

频繁的超新星爆发可用以解释活动星系核与类星体的超高金属丰度。星团中的恒星与吸积盘相互作用导致致密天体中子星和黑洞的形成率很高,这些致密天体与红巨星很容易形成双星系统,而后形成（ＮＳ／ＢＨ,ＮＳ／ＢＨ） 双星由于引力辐射最终导致并合而形成伽玛射线爆发。我们估计了伽玛射线爆的爆发频率,发现与观测相符。  相似文献   

地面网与空间网联合平差中起算边长和起算方位角权的确定     

徐正扬 《测绘学院学报》1995,(1)

本文全面分析了拉普拉斯方位角和起算边长的精度，指出了联合平差中这两类元素不能作为固定值，而应视为变量且赋予相应的权，并对权的取法进行了探讨。  相似文献   

铀矿层真实厚度的确定和最佳测井点距          下载免费PDF全文

秦积庚  谭庆江 《地球物理学报》1990,33(4):468-479

本文讨论了最佳测井点距的选择原理,其最佳值大致为8-12.5cm.并从原理上分析了矿层解释厚度增大的主要原因:根据离散测量值所作的分层解释结果必然导致矿层解释厚度的增大.大量的模型测量结果完全证实了理论分析的正确性,并且还提出了合适的解决办法.  相似文献   

西天山卡拉达湾地区铀及多金属综合找矿方向研究          下载免费PDF全文

陈江源  段晨宇  牛家骥  陈志鹏  尚景武 《地质找矿论丛》2020,35(1):25-32

卡拉达湾地区位于新疆北天山西段,属于中亚造山区,是在前寒武纪基底陆壳裂解的基础上发展起来的陆间型造山带,是铀及多金属成矿的重要区域。本文在前人工作的基础上,依据地面磁测、地面伽玛总量测量结果,总结分析了卡拉达湾地区磁场、放射性场、构造、矿化蚀变特征与铀及多金属成矿的关系,并圈定了铀及多金属找矿有利地段各2处,为西天山卡拉达湾地区的铀及多金属矿找矿工作提供方向。  相似文献   

铁路隧道GPS网布设的精度分析     

姚连璧  沈云中  胡丛玮  刘大杰 《武汉大学学报(信息科学版)》1997,(2)

探讨了隧道ＧＰＳ网在设计阶段估算横向贯通误差的基本理论，对按该理论编制的软件进行了计算正确性的验证。结合铁路测量规则对不同长度的隧道ＧＰＳ网横向贯通误差进行了计算分析，提出了分设隧道ＧＰＳ网的一些基本原则和隧道ＧＰＳ网横向贯通误差的近似估算方法  相似文献   

柴达木盆地第四纪古气候变化在物理测井自然伽玛曲线上的记录   总被引：7，自引：2，他引：7  

陈晔  袁林旺  周春林  刘泽纯 《古地理学报》2001,3(2):29-37

利用物理测井曲线分析古气候变化，是近年发展起来的新领域。本文在对取芯井涩中6井多种气候指标分析的基础上，建立了涩中6井GR曲线古气候反演模式，将该模式引进到盆地东部唯一贯穿第四纪的钻孔---达参1井，利用该井高分辨率自然伽玛曲线建立了盆地东部地区2.85Ma以来的时间标尺，据此讨论盆地东部地区2.85Ma以来的古气候变化，表明盆地气候变化在大阶段上明显受到天文轨道周期的控制，但也具有明显的区域性特征。此外还与盆地西部大浪滩ZK-336孔进行了对比。表明柴达木盆地同时包含了高原隆升与全球性气候变化的信息，是古环境变迁的良好的信息载体。也证明了自然伽玛曲线是反映内陆干旱盆地气候与环境变化良好的代用指标。  相似文献