吉黑东部斑岩型－浅成热液型铜金矿床多重成矿模型   总被引：9，自引：2，他引：9  

芮宗瑶  张洪涛  王龙生  陈仁义 《矿床地质》1995,(2)

通过四个典型矿床（小西南岔、闹枝、五凤和刺猬沟）的对比，发现它们在形成时间－空间－成因上既相互联系，又相互区别。小西南岔和闹枝矿床存在三个成矿流体系统：加热天水系统（Ａ）、排放流体系统（Ｂ）、蒸气缕（ｓｔｅａｍｐｌｕｍｅ）反应系统（Ｃ）；五凤和刺猬沟矿床只有一个成矿流体系统，即排放流体系统（Ｂ）。前者的成矿流体由浅成岩浆房的补给；后者的成矿流体主要为循环天水，浅成岩浆房的补给不明显。小西南岔金铜矿床产于中生代火山岩盆地边缘的隆起带，属于斑岩型矿床；闹枝金（铜）矿床产于中生代火山岩盆地内的断隆块，属于斑岩－浅成热液过渡型矿床；五凤和刺猬沟金（银）矿床产于中生代火山岩盆地内断裂带，属于浅成熟液型矿床。在区域成矿上，由浅入深，浅成热液型斑岩－浅成热液过渡型和斑岩型构成多重成矿模型。  相似文献   

线性矩法估计参数的保证修正值系数B的推求   总被引：3，自引：0，他引：3  

刘攀  郭生练  胡安焱 《水文》2006,26(6):27-29

在设计洪水的抽样误差估计中,采用保证修正值系数B方法估计均方差简单易用。应用线性矩法估计频率分布曲线的参数,有较好的无偏性和有效性,具有一定的应用前景。目前线性矩法的B值诺模图尚未确定,给用线性矩法确定参数时估计抽样误差带来了难度与不便。采用统计试验,分析了离差系数、偏态系数和样本长度对B值的影响,结果表明线性矩法估计参数时仍可采用保证修正值系数B值诺模图方法来估计抽样误差,并推求了不同偏态系数、设计频率情形下的B值,制成了线性矩法的B值诺模图备用。  相似文献   

用模糊ARTMAP算法对CBERS-2数据进行分类   总被引：3，自引：0，他引：3  

骆成凤  王长耀  牛铮 《武汉大学学报(信息科学版)》2006,31(4):325-328

用模糊ARTMAP（fuzzy adaptive resonance theorymap）神经网络算法对CBERS-2数据进行了分类实践。首先介绍了模糊ARTMAP神经网络的算法原理和具体训练分类过程；然后用2004年9月新疆石河子地区的影像数据进行土地利用分类试验，并将分类结果与基于统计的最大似然法（MLC）、反向传播神经网络（BP）的分类结果作比较，总分类精度比MLC和BP算法分别提高9．9％和4．6％。结果表明，模糊ARTMAP对试验区CBERS-2影像上的裸地识别能力很强，对高分辨率的CBERS-2影像可获得很好的分类结果。  相似文献   

基于B/S结构的网上考试系统     

吕静  陈春晓 《浙江气象》2006,27(4):37-42

介绍了基于B／S结构的网上考试系统应用于气象部门的理论研究，并分析了系统总体结构，提供了一种应用SQL数据库以及ASP编程实现的网络考试系统，详细阐述了科目管理、随机生成试卷等模块的设计与实现，以及相关数据库表的结构。  相似文献   

The complex gravitational lens system B1933+503     

C. M. Sykes  I. W. A. Browne  N. J. Jackson  D. R. Marlow  S. Nair  P. N. Wilkinson  R. D. Blandford  J. Cohen  C. D. Fassnacht  D. Hogg  T. J. Pearson  A. C. S. Readhead  D. S. Womble  S. T. Myers  A. G. de Bruyn  M. Bremer  G. K. Miley  & R. T. Schilizzi 《Monthly notices of the Royal Astronomical Society》1998,301(2):310-314

We report the discovery of the most complex arcsec-scale radio gravitational lens system yet known. B1933+503 was found during the course of the CLASS survey and MERLIN and VLA radio maps reveal up to 10 components. Four of these are compact and have flat spectra; the rest are more extended and have steep spectra. The background lensed object appears to consist of a flat-spectrum core (quadruply imaged) and two compact 'lobes' symmetrically disposed relative to the core. One of the lobes is quadruply imaged while the other is doubly imaged. An HST observation of the system with the WFPC2 shows a galaxy with an axial ratio of 0.5, but none of the images of the background object is detected. A redshift of 0.755 has been measured for the lens galaxy.  相似文献   

Modelling the 10-image lensed system B1933+503     

S. Nair 《Monthly notices of the Royal Astronomical Society》1998,301(2):315-322

A gravitational lens model is presented for the newly discovered 10-image system B1933+503. The underlying object, revealed by modelling, is a triple radio source on the scale of a couple of hundred mas that is well-aligned along the line of sight with a foreground and somewhat flattened lensing galaxy, the orientation and location of which match those of an observed galaxy, known to be at a redshift of 0.755. Uncertainties in the modelling are obtained by a Monte Carlo exercise. Observational tests of the lens model are proposed, and the time delays between various pairs of images are determined, as the core of the source is known to be significantly variable. Future observations of the lens hold the key to using B1933+503 to constrain Hubble's constant. Despite the absence of a source redshift, the utility of the system as a probe of the structure of the lens galaxy is unparalleled as it provides a surfeit of easily identifiable constraints for modelling the system.  相似文献   

A timing formula for main-sequence star binary pulsars     

Norbert Wex 《Monthly notices of the Royal Astronomical Society》1998,298(1):67-77

In binary radio pulsars with a main-sequence star companion, the spin-induced quadrupole moment of the companion gives rise to a precession of the binary orbit. As a first approximation one can model the secular evolution caused by this classical spin-orbit coupling by linear-in-time changes of the longitude of periastron and the projected semi-major axis of the pulsar orbit. This simple representation of the precession of the orbit neglects two important aspects of the orbital dynamics of a binary pulsar with an oblate companion. First, the quasiperiodic effects along the orbit, owing to the anisotropic 1/ r ³ nature of the quadrupole potential. Secondly, the long-term secular evolution of the binary orbit, which leads to an evolution of the longitude of periastron and the projected semi-major axis, which is non-linear in time.   In this paper a simple timing formula for binary radio pulsars with a main-sequence star companion is presented which models the short-term secular and most of the short-term periodic effects caused by the classical spin-orbit coupling. I also give extensions of the timing formula that account for long-term secular changes in the binary pulsar motion. It is shown that the short-term periodic effects are important for the timing observations of the binary pulsar PSR B1259–63. The long-term secular effects are likely to become important in the next few years of timing observations of the binary pulsar PSR J0045–7319. They could help to restrict or even determine the moments of inertia of the companion star and thus probe its internal structure.   Finally, I reinvestigate the spin-orbit precession of the binary pulsar PSR J0045–7319 since the analysis given in the literature is based on an incorrect expression for the precession of the longitude of periastron. A lower limit of 20° for the inclination of the B star with respect to the orbital plane is derived.  相似文献   

参数调整对气象预测的B-P网络模型性能的影响     

邓新民  顾永刚 《成都信息工程学院学报》1998,(1)

为了探索ＢＰ网络的参数调整特性,进行了参数α、β的选取对ＢＰ算法的收敛速度和模型的稳定性的影响研究。通过ＢＰ网络用于气象预测建模的参数调整个例分析表明：参数α、β的取值对ＢＰ模型的稳定性无显著影响,但参数值的调整尤其是β值的调整对建模的收敛速度有明显的影响。  相似文献   

Mathematical Modelling and Accuracy Testing of Spot Level 1B Stereopairs     

M. J. Valadan Zoej  & G. Petrie 《The Photogrammetric Record》1998,16(91):67-82

During a project concerned with DEM generation using SPOT stereoscopic imagery, difficulties were experienced when using Level 1B stereopairs for the task. This paper presents a mathematical solution to overcome this problem which has been implemented at the University of Glasgow. Results are included from experimental tests which were carried out over a test field in Jordan using this solution. These tests used five SPOT Level 1B stereopairs together with a single SPOT Level 1A stereopair for comparative purposes. The residual errors at the ground control points and independent check points are given and show that a satisfactory solution was achieved.  相似文献   

陕西段家坡黄土剖面中布容／松山古地磁界线附近铱异常的发现及其启示   总被引：3，自引：0，他引：3  

马配学  侯泉林 《地质学报》1998,72(2):173-177

利用高灵敏度放射化学中子活化分析方法,对我国陕西段家坡黄土剖面早－中更新统（约０．７３Ｍａ）沉积界线附近铱和其它元素的丰度进行了测定。结果表明,在布容／松山（Ｂ／Ｍ）古地磁界线附近铱的含量明显增大,最大值为４６．３ｐｇ／ｇ。相对于整个剖面的平均背景值（约１５ｐｇ／ｇ）大约富集了３倍。用地壳元素钪进行标准化之后,铱异常十分明显,而其它元素在界线附近则没有变化。黄土剖面上铱异常的赋存层位与西南太平洋钻  相似文献