重磁数据的线性滤波与反演失真问题     

汤悦林  陈元平 《物探与化探》2002,26(3):225-231

文中对国内研制的4种主要线性滤波方法进行了对比分析。选出一种具代表性的滤波方法,用计算机模拟观测场,探讨了在复杂干扰下重磁异常因滤波引起的失真,并就重磁异常在因滤波而引起失真的情况下如何反演解释,提出了可行的办法和建议。  相似文献   

东马珠穆沁旗中铁陨石表面的角砾状橄榄石的特征     

陶克捷  杨主明等 《岩石学报》2001,17(2):321-324

东乌珠穆沁旗中铁陨石中有二种橄榄石。一种是陨石中基质橄榄石，另一种是镶嵌在陨石表面的角砾状橄榄石。电子探针成分分析结果表明，两种橄榄石中的FeO和MnO比值，包体矿物种类，包体铁纹石和镍纹石中Fe,Ni的含量等，均有较大区别。陨石中基质橄榄石矿物是本陨石中原物质，而角砾状橄榄石是宇宙中物质。他们是两块自由翱于宇宙中的物质碰撞混合而形成的东乌珠穆旗陨石中这种现象。  相似文献   

全球气侯长期振动的Fokker-Planck方程及其求解     

封国林  曹鸿兴  邵耀椿  曹永忠 《气象学报》1996,54(6):753-758

假定行星反照率为温度的平方关系，导出了零维随机动力气候模式。对相应的ＦｏｋｋｅｒＰｌａｎｃｋ方程用矩阵连分法求解，得到了１０万年，４万年，２万年气候周期的本征值和本征向量。数值计算表明，在随机噪声强度Ｄ＝１．９５时，１０万年气候振动具有最大的振幅，即Ｍｉｌａｎｋｏｖｉｔｃｈ理论无法解释的１０万年周期。  相似文献   

不同大地坐标系大地坐标求解转换参数模型的应用和权阵的选取     

朱华统 《测绘学院学报》1992,(3)

本文介绍了布尔莎(L,B,H)公式求解转换参数模型的应用,重点是讨论权阵的选取。其结果表明,按最小二乘平差求转换参数时,必须使用相关权阵。  相似文献   

长周期地震观测中的环境干扰     

邱国荣 《地震地磁观测与研究》1992,13(2):61-66

文章根据长周期地震观测的理论和我国763长周期台网的观测实践,分析了长周期观测中的环境干扰。认为长周期观测对环境干扰(主要指温、湿度)敏感,但影响长周期仪器正常工作的关键是潮湿,尤其是记录室的潮湿。文章以763台网优秀台站的观测实践为例,认为只要掌握了环境干扰的规律,在防潮问题上采取有效措施,长周期地震观测是完全可以做到仪器工作稳定,管理得心应手。  相似文献   

多罗山钨矿床黑钨矿晶体形貌学研究     

王文魁  甘正梅 《地球科学》1992,17(6):638-646

简要论述了典型热液裂隙充填钨—铋—钼石英脉矿床地质及其以黑钨矿—辉铋矿—辉钼矿为主的矿物组合纵向逆分带现象。重点测量研究了黑钨矿晶体的宏观形态特征和微形貌,及其成因演化机制。以现代光学微分干涉(DIC)显微镜观察测量了黑钨矿端面(102)等的螺旋生长及[010]晶带等的层生长现象。提出黑钨矿晶体的螺—层混合生长概念。  相似文献   

层次分析法（AHP法）在金矿勘查中的应用—新疆金窝子金矿床为例     

贺连顺 《矿产与地质》1992,6(6):420-424

应用层次分析法（Analystical Hierarchy Process,简称AHP法）确定金窝子金矿床合理的工业品位指标。将影响工业品位的因素及各因素间的隶属关系构成系统的多层次分析结构模型，进行层次排序，制订工业品位指标的总目标，通过分析和计算，确定工业品位指标的最佳方案，取得了较满意的结果。  相似文献   

偏光显微镜聚敛光系统光路分析   总被引：1，自引：0，他引：1  

包相臣 《矿物岩石》1995,15(2):73-77

通过实验和计算，文章证明了勃氏镜进入显微光路后，可使整个显微镜系统变成望远系统，望远系统接收平行光信号，形成干涉图或偏光图像，而显微系统接收非平行光信号形成矿物像，文章不仅对偏光图和干涉图在显微镜筒中的光路变化及成像机理进行了深入讨论，并且对如何保持干涉图和偏光图像清晰提出了调试意见。  相似文献   

Detection, excision and statistics of interference at the Mauritius radio telescope     

S. Sachdev  N. Udaya Shankar 《Journal of Astrophysics and Astronomy》2001,22(2-3):213-227

A technique to detect man-made interference in the visibility data of the Mauritius Radio Telescope (MRT) has been developed. This technique is based on the understanding that the interference is generally ‘spiky’ in nature and has Fourier components beyond the maximum frequency which can arise from the radio sky and can therefore be identified. We take the sum of magnitudes of visibilities on all the baselines measured at a given time to improve detectability. This is then high-pass filtered to get a time series from which the contribution of the sky is removed. Interference is detected in the high-pass data using an iterative scheme. In each iteration, interference with amplitudes beyond a certain threshold is detected. These points are then removed from the original time series and the resulting data are high-pass filtered and the process repeated. We have also studied the statistics of the strength, numbers, time of occurrence and duration of the interference at the MRT. The statistics indicate that most often the interference excision can be carried out while post-integrating the visibilities by giving a zero weight to the interference points.  相似文献   

Application of matrix analysis in delineating sinkhole risk areas along highway (I-70 near Frederick,Maryland)     

Wanfang?ZhouEmail author  Barry?F.?Beck  Angela?L.?Adams 《Environmental Geology》2003,44(7):834-842

Sinkhole collapse in the area of Maryland Interstate 70 (I-70) and nearby roadways south of Frederick, Maryland, has been posing a threat to the safety of the highway operation as well as other structures. The occurrence of sinkholes is associated with intensive land development. However, the geological conditions that have been developing over the past 200 million years in the Frederick Valley control the locations of the sinkholes. Within an area of approximately 8 km², 138 sinkholes are recorded and their spatial distribution is irregular, but clustered. The clustering indicates the existence of an interaction between the sinkholes. The point pattern of sinkholes is considered to be a sample of a Gibbsian point process from which the hard-core Strauss Model is developed. The radius of influence is calculated for the recorded sinkholes which are most likely to occur within 30 m of an existing sinkhole. The stochastic analysis of the existing sinkholes is biased toward the areas with intensive land use. This bias is adjusted by considering (1) topography, (2) proximity to topographic depressions, (3) interpreted rock formation, (4) soil type, (5) geophysical anomalies, (6) proximity to geologic structures, and (7) thickness of overburden. Based on the properties of each factor, a scoring system is developed and the average relative risk score for individual 30-m segments of the study area is calculated. The areas designated by higher risk levels would have greater risk of a sinkhole collapse than the areas designated by lower risk levels. This risk assessment approach can be updated as more information becomes available.  相似文献