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31.
以反解 Stokes公式为数学模型 ,应用由 T/ P测高数据计算的大地水准面高反演了海域平均重力异常 ,并与船测平均重力异常和 OSU91A位模型计算的平均重力异常进行了比对分析 ,得出了一些有益的结论。  相似文献   
32.
In variational problem, the selection of functional weighting factors (FWF) is one of the key points for discussing many relevant studies. To overcome arbitrariness and subjectivity of the empirical selecting methods used widely at present, this paper tries to put forward in optimal objective selecting method of FWF. The focus of the study is on the weighting factors optimal selection in the variation retrieval single-Doppler radar wind field with the simple adjoint models. Weighting factors in the meaning of minimal variance are calculated out with the matrix theory and the finite difference method of partial differential equation. Experiments show that the result is more objective comparing with the factors obtained with the empirical method.  相似文献   
33.
In this study, a series of inverse-analysis numerical experiments was performed to investigate the effect of soil models on the deformations caused by excavation by using the finite element method. The nonlinear optimization technique that was incorporated into the finite element code was used for the inverse-analysis numerical experiments. Three soil models (the hyperbolic model, pseudo-plasticity model, and modified pseudo-plasticity model) were employed in the intended numerical experiments on a well-documented excavation case history. The results indicate that wall deflection due to excavation can be accurately back-figured by each of the three soil models, while the ground surface settlement can be reasonably optimized only by the pseudo-plasticity model and the modified pseudo-plasticity model. Importantly, the modified pseudo-plasticity model can yield more reasonable simulations when the wall deflection and the ground surface settlement are simultaneously back-figured. The results show that selection of an adequate soil model that is capable of adequately describing the stress–strain-strength characteristics of the soils is essentially crucial when predicting the excavation-induced ground response.  相似文献   
34.
马氏距离(Mahalanobis distance)是一种有效的计算样本集间相似度的方法。它不受量纲的影响,可以排除变量之间的相关性的干扰,且通常能夸大变化微小的变量的作用。由于化探数据信息量大,计算繁琐,该方法在实际生产应用较少。借助强大的数学运算软件Matlab,能实现快速计算马氏距离,结合Mapgis等相关的GIS平台,可以快速圈定综合异常并能很好的强化具一定找矿前景的弱小异常,为下一步异常查证起到快速有效的指导作用。依据青海省门源县西河坝地区1∶5万水系沉积物测量的数据成果,通过与传统综合异常圈定方法进行对比,马氏距离圈定综合异常具一定的优势。  相似文献   
35.
局部腐蚀包括缝隙腐蚀、应力腐蚀、腐蚀磨损、氢腐蚀,H2S应力腐蚀和氢腐蚀是长输管道最容易发生的一种局部腐蚀方式。针对长输管道易发生局部腐蚀的特点,参考其他管道评价方法,根据现场管道的安全状况,提出了适用于现场的含局部腐蚀体积型缺陷管道的三步评价法。该方法不需要考虑管道的腐蚀裕量,简化公式,便于现场计算。  相似文献   
36.
针对目前流星雷达测距误差大的问题,本文提出了提高流星雷达测距精度的新方法,即提高采样速率,用相关分析确定回波脉冲参考点的方法。该方法使流星雷达的测距精度提高一个数量级,测距误差降到±14m,使流星雷达不仅可以用来观测研究流星,还可用于监测飞机、火箭的飞行等,扩大流星雷达的应用。  相似文献   
37.
Increased erosion rates during the last 2 Myr of Earth history are commonly associated with widespread glaciation and global cooling. However, whether erosion rates actually increased during that period of time remains debated. This is in part because the respective role of fluvial and glacial erosion is difficult to assess, and because many existing techniques used to estimate erosion rates may be affected by averaging biases that may produce increased erosion rates towards the present. Here, we apply thermoluminescence thermochronometry to granitic bedrock samples of the southern-central Chilean Andes, a region which experienced a full transition from glacial-humid to fluvial-dry conditions during the Quaternary. Inverse modelling of the thermochronological data enables us to extract unbiased time series of erosion rates during the last ∼100 kyr. We find that erosion rates were systematically higher during around the last glacial maximum than at present, with differences exceeding an order of magnitude. Our findings indicate that glacial erosion is probably more efficient than fluvial erosion and imply that erosion has remained transient during the Quaternary.  相似文献   
38.
赞比亚西北省希富玛铜矿床是中矿资源勘探股份有限公司在"走出去"战略背景下取得的一个勘探找矿成果。文章基于Micromine三维矿业软件平台,建立了希富玛铜矿床地质数据库,并对矿体进行了地质解译及圈定,同时结合矿区的一个矿体,介绍了采用距离反比加权法进行资源量估算的原理和流程。  相似文献   
39.
Since the mechanical twinning along calcite e-planes has a critical resolved shear stress, not only principal stress axes but also differential stress can be determined from the orientations of twin lamellae. Based on the five-dimensional stress space that fulfills the principle of coordinate invariance, it is shown in this article that the inversion of twin and untwin data is comparable with fitting a spherical cap to data points on a unit sphere in the space. The principal stress orientations and stress ratio are indicated by the center of the cap, whereas differential stress is denoted by the size of the cap. Based on this geometrical interpretation, the generalized Hough transform was applied to the inversion of the data in this study. The new method is demonstrated to be robust to sampling bias, variability in the critical resolved shear stress. The determination of differential stress was difficult when the differential stress to be detected was ∼10 times larger than the critical resolved shear stress. Stresses were separated by the method from heterogeneous data successfully as long as the spherical caps corresponding to the stresses to be detected had no or a small intersection.  相似文献   
40.
We present the first CCD photometric UBVRI observations of the not-so-well-studied open cluster NGC 1624 (OCl 403, Cr 53; α2000 = 04 h 40 m 36 s; δ2000 = + 50˚ 27 42″ Trumpler class = I 2 p N). This cluster was observed on 01 February 2004 with the 2 m Himalayan Chandra Telescope at Hanle using a LN2 cooled 2k × 2k CCD. The cluster presents differential reddening with E(B-V) values ranging from 0.70 to 0.90 mag, which could be attributed to the presence of the HII region wherein the cluster is embedded. It is found to be at a distance of 6.025 ± 0.5 kpc and the age of this cluster is estimated to be ∼3.98 × 106 years. In view of these parameters, it can be considered as a young enough cluster located in the direction of the Perseus constellation with the galactic coordinates of l = 155˚.35 and b = + 02 ˚.58. Thus it could also be used as a suitable candidate for tracing the Outer Perseus spiral arm of our Galaxy. The initial mass function slope is derived as 1.65 ± 0.25 by applying the corrections for field star contamination and data incompleteness. This is in good agreement with the Salpeter value within the limits of errors.  相似文献   
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