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91.
区域Gamma混合模型的SAR图像分割 总被引:1,自引:0,他引:1
针对传统Gamma混合模型用于SAR图像分割时忽略像素间空间相关性,导致分割结果不连续并产生大量误分割的现象,提出了区域Gamma混合模型的SAR图像分割算法。首先对图像进行分水岭分割,得到过分割区域块,然后将其作为输入样本进行基于Gamma混合模型的聚类,在模型的参数估计过程中进一步考虑区域间的空间相关性,设计邻域因子融入到迭代过程,得到邻域加权类分布概率。该算法充分利用像素间的空间相关性,能够降低噪声对分割结果的影响。通过合成图像和真实SAR图像的实验表明,本文算法能够实现SAR图像的准确分割。 相似文献
92.
在大型工程的变形监测中,传统方法是利用全站仪,按照等级测量规范进行方向法、全圆法观测,测站至少需要1个观测员、1个记录员,每个测回需要人工计算和比较,内业需要后处理,费工、费时、容易出错。结合测绘实践的现实需要,利用VB语言和TCA2003全站仪的内置程序功能,开发变形监测数据自动检查程序,为自动化测绘探索新的方法。 相似文献
93.
Further Information of the Associated Li Deposits in the No.6 Coal Seam at Jungar Coalfield,Inner Mongolia,Northern China 总被引:2,自引:0,他引:2
SUN Yuzhuang ZHAO Cunliang LI Yanheng WANG Jinxi ZHANG Jiany JIN Zhe LIN Mingyue Wolfgang KALKREUTH 《《地质学报》英文版》2013,87(4):1097-1108
Total 138 coal samples and 14 parting samples were taken from the No. 6 Seam of the Jungar Coalfield, Inner Mongolia. These samples were analysed by optical microscopy, sequential chemical extraction procedure (SCEP), inductively coupled plasma mass spectrometry (ICP-MS), X-ray powder diffraction (XRD), and scanning electron microscope in conjunction with an energy-dispersive X-ray spectrometer (SEM-EDX) analysis. The results indicate that the Li contents have reached the industrial grade of the coal associated Li deposit, and the total Li reserves have reached 2406600 tons, that is, 5157000 tons Li2O in the No. 6 seam in the Jungar Coalfield. The sequential chemical extraction procedure results suggest that the Li concentration is mainly related to inorganic matter. The minerals in the coals consist of kaolinite, boehmite, chlorite-group mineral, quartz, calcite, pyrite, siderite and amorphous clay material. Some Li could be absorbed by clay minerals in the Li-bearing coal seam. The chlorite phase?could be?most likely the host for a part of Li. The Yinshan Oldland should be the most possible source of Li of the coal. 相似文献
94.
黄龙玉矿床主要分布在云南省保山市龙陵县小黑山一带,矿体产于三叠系公养河群板岩与花岗岩接触带上。自古生代以来,除石炭纪、古近纪和新近纪外,其它地层均有出露。矿区岩浆活动频繁,具有多期次多阶段的岩浆侵入。黄龙玉的化学成分主要为SiO2,矿物成分为石英、玉髓和蛋白石,相对密度2.65~2.70,折射率1.54~1.56,Fe3+为致色离子,颜色成因以内源氧化转色为主,隐晶质—微粒结构,块状构造、条带状构造和角砾状构造。本文对黄龙玉产出的地质特征、宝石矿物学特征、品质特征以及与相似宝玉石—田黄和黄色翡翠对比等方面进行了深入阐述,为市场宝石的鉴别提供了一定的参考价值。 相似文献
95.
High‐resolution gamma ray spectrometry was exploited to locate the potential radioactive targets at Kab Amiri granite pluton, Central Eastern Desert, Egypt. The Kab Amiri pluton forms a concentric granitic body of monzogranite to syenogranite composition intruded into mafic‐ultramific rocks. To identify and detect anomalous concentrations of natural radioactive elements in the study area, contour maps of equivalent uranium (eU ppm), equivalent thorium (eTh ppm), potassium (K%) and their geochemical ratios (eU/Th, eTh/K and eU‐eTh/3.5) as well as standard deviation map of uranium were constructed and interpreted. Qualitative and quantitative interpretations of the spectrometric survey data revealed the presence of seven radioactive anomalies in the south of the studied area. These anomalies could be related to the prevailing faulting directions NE and ENE fault trends. The southernmost anomalous zone is related to high episyenitization and uranium concentrations. It exhibits a sharp increase in the eU concentrations reaching 370 ppm resulting in a high eU/eTh ratio reaching 4.5 and characterized by oval shape trending in the NE direction. Constructing the contour map of the (eU‐eTh/3.5) was helpful in defining the trends of uranium migration and enabling the delineation of the limit between the negative contours (leaching) and positive contours (deposition). 相似文献
96.
风化壳离子吸附型稀土矿稀土浸出工业指标的意义 总被引:1,自引:0,他引:1
一直以来,风化壳型稀土矿床均以全相品位来圈定矿体,计算全相储量。而矿山实际生产长期以来是用浸出稀土品位及其总量为依据。在用浸出品位作为基本分析项目时,其分析成本仅有原全相分析的四分之一,且分析周期、普查周期亦大大缩短。同时选取合适的组合样求取浸出率可以求出全相储量,为国家提供稀土总量数据。总之,浸出工业指标比全相分析指标更能反映采选工艺的进步,保证充分利用资源,又能提供二种合理的储量。缩短资源评价周期。节约资源评价费用,是一种经济适用的工业指标,具有一定的参考价值。 相似文献
97.
以计算结果可靠的土层反应结果为基础数据,基于随机森林算法(Random Forest,简称“RF”),建立地震动、场地土层参数特征量与土层变形特征的关系,提出一种依据常规地震动和场地土层参数为特征量的地震荷载下土层变形等级预测新方法,给出了典型场地土体发生大应变的地震动阈值。结果表明:基于RF模型对土体的变形程度预测结果较为理想,各项评价指标始终保持一个较高水平;对于软土、中硬土及硬土场地,输入地震动分别大于0.05 g、0.15 g及0.19 g时,将产生大应变。同时,本文方法可在不进行土层地震反应数值模拟的情况下,得到场地各土层的剪应变等级,为强地震作用下土体实际力学状态的界定和认识提供新的分析手段,而且也可为地下结构抗震设计问题提供指导和参考。 相似文献
98.
Y. Mizumura J. Kushida K. Nishijima G.V. BicknellR.W. Clay P.G. EdwardsS. Gunji S. HaraS. Hayashi S. KabukiF. Kajino A. KawachiT. Kifune R. KiuchiK. Kodani Y. MatsubaraT. Mizukami Y. MizumotoM. Mori H. MuraishiT. Naito M. OhishiV. Stamatescu D.L. SwabyT. Tanimori G. ThorntonF. Tokanai T. ToyamaS. Yanagita T. YoshidaT. Yoshikoshi 《Astroparticle Physics》2012,35(9):563-572
We have searched for very high energy (VHE) gamma rays from four blazars using the CANGAROO-III imaging atmospheric Cherenkov telescope. We report the results of the observations of H 2356-309, PKS 2155-304, PKS 0537-441, and 3C 279, performed from 2005 to 2009, applying a new analysis to suppress the effects of the position dependence of Cherenkov images in the field of view. No significant VHE gamma ray emission was detected from any of the four blazars. The GeV gamma-ray spectra of these objects were obtained by analyzing Fermi/LAT archival data. Wide range (radio to VHE gamma-ray bands) spectral energy distributions (SEDs) including CANGAROO-III upper limits, GeV gamma-ray spectra, and archival data, even though they are non-simultaneous, are discussed using a one-zone synchrotron self-Compton (SSC) model in combination with a external Compton (EC) radiation. The HBLs (H 2356-309 and PKS 2155-304) can be explained by a simple SSC model, and PKS 0537-441 and 3C 279 are well modeled by a combination of SSC and EC model. We find a consistency with the blazar sequence in terms of strength of magnetic field and component size. 相似文献
99.
100.
Brian J. Morsony Jared C. Workman Davide Lazzati Mikhail V. Medvedev 《Monthly notices of the Royal Astronomical Society》2009,392(4):1397-1402
We consider radiation emitted by the jitter mechanism in a Blandford–McKee self-similar blastwave. We assume the magnetic field configuration throughout the whole blastwave meets the condition for the emission of jitter radiation and we compute the ensuing images, light curves and spectra. The calculations are performed for both a uniform and a wind environment. We compare our jitter results to synchrotron results. We show that jitter radiation produces slightly different spectra than synchrotron, in particular between the self-absorption and the peak frequency, where the jitter spectrum is flat, while the synchrotron spectrum grows as ν1/3 . The spectral difference is reflected in the early decay slope of the light curves. We conclude that jitter and synchrotron afterglows can be distinguished from each other with good quality observations. However, it is unlikely that the difference can explain the peculiar behaviour of several recent observations, such as flat X-ray slopes and uncorrelated optical and X-ray behaviour. 相似文献