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81.
航磁异常的几种计算机分类方法 总被引:1,自引:0,他引:1
韩英杰 《物探化探计算技术》2005,27(1):81-83
目前,应用计算机对航磁异常进行分类存在很大局限性。为克服这些局限性,将航磁异常分类的结果从定性水平提升到定量水平,这里应用三种分类方法在计算机上对航磁异常进行分类。经实例检验,分类结果令人满意,有效地改进和实现了用于航磁异常分类的定量方法。 相似文献
82.
83.
应用航磁数据分维计算推断火成岩的分布 总被引:2,自引:0,他引:2
计算巴彦浩特盆地航磁异常的分维数, 对计算出的分维数绘制等值线图, 并根据分形特征对该地区的火成岩进行划分, 得到了以往直接对航磁异常图进行推断解释所不能得到的良好地质效果。最后讨论如何选取最佳窗口和最佳网格来计算分维数, 并对此提出了2个经验。 相似文献
84.
不同密度采样是否可以获得稳定的和可追索的地球化学模式是检验采样是否具有代表性,分析技术是否成熟的重要依据。笔者选择新疆哈密大南湖地区约6400km^2面积,进行了从超低密度(1个样/100km^2),甚低密度(1个样/25km^2)直到低密度(1个样/4km^2)地球化学采样,对比了3种密度地球化学采样所获得的地球化学数据和异常分布模式。得出如下结论:超低密度、甚低密度、低密度地球化学调查获得的元素含量平均值和背景值非常接近;超低密度、甚低密度、低密度调查所圈定的地球化学省在形态上和变化趋势上非常相似,浓集中心的位置重合,表明不同调查阶段可获得稳定的和可追索的地球化学模式;采样密度越大数据离散程度越高,即最小值更小,最大值更大,表明元素分布的局部不均匀性,正是这种局部的不均匀性才能通过加密采样刻画出地球化学模式的细节变化,为逐步追踪矿化体奠定了基础;超低密度和甚低密度采样可以有效圈定矿集区所形成的大规模地球化学异常,低密度地球化学调查不仅可以圈定矿集区异常,同时可以圈定分散矿化的小规模局部异常。 相似文献
85.
86.
内蒙古中部重、磁场特征与地壳密度结构 总被引:2,自引:2,他引:2
中亚造山带中的古生代——中生代花岗岩普遍具有正εNd值,在世界上是十分独特的。美国西部加利福尼亚中生代-新生代花岗岩同样具有正εNd值,并且其地壳的速度分布特征与内蒙古中部十分相似。本文通过与美国加利福尼亚的地球物理研究成果进行对比,来研究内蒙古中部的地壳密度结构,特别是下地壳的组成,试图探讨产生正£。值花岗岩的深部地质原因。研究结果表明,在大兴安岭-内蒙古造山带下地壳中可能存在与美国加里福尼亚类似的洋壳物质。此外,还对重、磁异常进行了处理,以确定蛇绿岩带的延展情况。由于在西拉木伦河附近存在切割至莫霍面的深断裂,结合地表出现的蛇绿岩带,故提出温都尔庙-西拉木伦河一线可能是内蒙古中部最重要的地质构造界线。 相似文献
87.
M. Kern T. Preimesberger M. Allesch R. Pail J. Bouman R. Koop 《Journal of Geodesy》2005,78(9):509-519
The satellite missions CHAMP, GRACE, and GOCE mark the beginning of a new era in gravity field determination and modeling. They provide unique models of the global stationary gravity field and its variation in time. Due to inevitable measurement errors, sophisticated pre-processing steps have to be applied before further use of the satellite measurements. In the framework of the GOCE mission, this includes outlier detection, absolute calibration and validation of the SGG (satellite gravity gradiometry) measurements, and removal of temporal effects. In general, outliers are defined as observations that appear to be inconsistent with the remainder of the data set. One goal is to evaluate the effect of additive, innovative and bulk outliers on the estimates of the spherical harmonic coefficients. It can be shown that even a small number of undetected outliers (<0.2 of all data points) can have an adverse effect on the coefficient estimates. Consequently, concepts for the identification and removal of outliers have to be developed. Novel outlier detection algorithms are derived and statistical methods are presented that may be used for this purpose. The methods aim at high outlier identification rates as well as small failure rates. A combined algorithm, based on wavelets and a statistical method, shows best performance with an identification rate of about 99%. To further reduce the influence of undetected outliers, an outlier detection algorithm is implemented inside the gravity field solver (the Quick-Look Gravity Field Analysis tool was used). This results in spherical harmonic coefficient estimates that are of similar quality to those obtained without outliers in the input data. 相似文献
88.
R. Pail 《Journal of Geodesy》2005,79(4-5):231-241
In the recent design of the Gravity field and steady-state Ocean Circulation Explorer (GOCE) satellite mission, the gravity gradients are defined in the gradiometer reference frame (GRF), which deviates from the actual flight direction (local orbit reference frame, LORF) by up to 3–4°. The main objective of this paper is to investigate the effect of uncertainties in the knowledge of the gradiometer orientation due to attitude reconstitution errors on the gravity field solution. In the framework of several numerical simulations, which are based on a realistic mission configuration, different scenarios are investigated, to provide the accuracy requirements of the orientation information. It turns out that orientation errors have to be seriously considered, because they may represent a significant error component of the gravity field solution. While in a realistic mission scenario (colored gradiometer noise) the gravity field solutions are quite insensitive to small orientation biases, random noise applied to the attitude information can have a considerable impact on the accuracy of the resolved gravity field models. 相似文献
89.
B. Tapley J. Ries S. Bettadpur D. Chambers M. Cheng F. Condi B. Gunter Z. Kang P. Nagel R. Pastor T. Pekker S. Poole F. Wang 《Journal of Geodesy》2005,79(8):467-478
A new generation of Earth gravity field models called GGM02 are derived using approximately 14 months of data spanning from
April 2002 to December 2003 from the Gravity Recovery And Climate Experiment (GRACE). Relative to the preceding generation,
GGM01, there have been improvements to the data products, the gravity estimation methods and the background models. Based
on the calibrated covariances, GGM02 (both the GRACE-only model GGM02S and the combination model GGM02C) represents an improvement
greater than a factor of two over the previous GGM01 models. Error estimates indicate a cumulative error less than 1 cm geoid
height to spherical harmonic degree 70, which can be said to have met the GRACE minimum mission goals.
Electronic Supplementary Material Supplementary material is available in the online version of this article at 相似文献
90.
In space-borne gravitational field determination, two challenges are inherent. First, the continuation of the data down to
the surface of the Earth is an ill-posed problem, requiring therefore regularization techniques. Second huge data sets result
requiring efficient numerical methods. In this paper, we show how locally supported wavelets on the sphere can be developed
by means of a spherical version of the so-called up function. By construction, the corresponding scaling functions and wavelets
are infinitely smooth, so that they can be used for regularization purposes. In particular, we show how the ill-posed pseudo-differential
equations coming from satellite missions can be regularized by efficient numerical schemes using locally supported wavelets.
These methods seem in particular to be interesting for regional gravity field modelling. 相似文献