一种遥感影像同名点密集匹配方法

针对在遥感相机检校、三维重建、信息提取、变化监测等应用中,都需要在影像中每隔若干个点、甚至是逐点寻找密集同名点的情况,该文将基于特征的方法和基于模板的方法相结合,提出一种新的高精度的密集同名点提取方法。将参考影像降采样为与遥感影像同一分辨率,然后使用SIFT算法提取粗精度同名点,建立全局几何模型,使用其将遥感影像每个像元及其邻域投影到参考影像,并以其为模板,应用优化相位匹配法获取高精度同名点。经实验验证,只要遥感影像和参考影像中相应区域的景物变化不大,该文方法可以有效地确定密集的高精度同名点对。     

地浸砂岩型铀矿致密泥岩齿形复合片钻头的研究与应用

针对地浸砂岩型铀矿钻探中致密泥岩钻进效率低的问题,在内蒙古巴音戈壁盆地研究试验了齿形复合片钻头与圆片状复合片钻头,提高了钻进效率.对研磨性较弱,中等硬度致密泥岩,采用Φ104 mm双环式齿形复合片钻头(六组)的钻进效率达到2.60 m/h,比普通复合片钻头提高73%;采用Φ110 mm双环式平底齿形复合片钻头(四组)的...     

密集颗粒流中的速度波动及自扩散特征

 密集颗粒流是颗粒介质中非常重要的一种运动状态,其内部单个粒子的速度波动通常是导致系统出现输运、混合、分离等宏观过程的微观基础,因此,如何对其进行定量描述是颗粒介质研究中一个非常关键的问题。基于所建立的环形剪切颗粒流的离散元模型,首先分析了系统达到剪切稳定状态时不同局部区域内微观粒子速度波动的宏观统计特征;通过引入自扩散系数定量研究了剪切颗粒流内粒子扩散运动过程中的局部化和各向异性特征;最后讨论了局部剪切率、初始体积分数以及粒子间的摩擦系数对系统自扩散系数的影响规律。     

融合SIFT与SGM的倾斜航空影像密集匹配

针对倾斜航空摄影特点与匹配处理要求,提出了融合尺度不变特征转换SIFT与半全局匹配SGM的倾斜影像密集匹配方法,包括两个阶段:(1)引入局部二阶矩变换的SIFT倾斜影像稀疏匹配。利用与二阶矩特征值有关的Hessian-Gabor算子提取影像初始特征,通过窗口二阶矩变换及椭圆归一化处理去除特征邻域的仿射变化,使得改进SIFT的特征描述符仿射不变性大大增强,满足宽基线倾斜像对稳健匹配要求的同时并能获得较多的匹配特征作为后续SGM优化计算的路径约束条件;(2)路径受限优化下的SGM倾斜影像密集匹配。以倾斜影像SIFT成功匹配像素的互信息为约束,对SGM的动态规划路径进行分段纠正,减小错误匹配代价的传播并加速最优路径搜索过程;以匹配像素的离散视差信息为基础,基于TPS变换生成良好初始视差图,以提高SGM互信息计算的可靠性并提高计算效率;对理想水平像对下的摄影测量水平核线重排过程进行扩展,整体旋转摄影基线以消除分量BX,BY的影响并建立虚拟"水平"像空间辅助坐标系,从而利用相对定向参数生成沿扫描线方向的"水平"核线影像以满足SGM应用要求。倾斜影像密集匹配试验结果证明了算法的有效性,可为后续摄影测量DSM自动生成或3维快速重建工作提供可靠、逐像素的密集匹配点。     

内蒙古中东部草原景观区多金属矿地球化学勘查方法对比研究

内蒙古中东部草原景观区成矿地质条件有利,但由于风成砂等的覆盖,导致常规地球化学勘查在该地区找矿中受到限制。在内蒙古东乌旗1017高地进行了土壤热磁组分测量、土壤细粒级组分测量和铁锰氧化物态测量方法的对比试验,结果表明,3种方法均能有效地圈出地球化学异常,而且3种方法圈定的异常吻合程度很好。相比较而言,土壤热磁组分测量能够显著提高异常强度,有利于发现微弱的地球化学异常信息,显示出该方法在草原景观区良好的应用前景。     

Efficiency Analysis of Focal Plane Arrays in Deep Dishes

In this paper we demonstrate the practical analysis of a dense Focal Plane Array (FPA) for a deep dish radio telescope. The analytical model is used to optimize efficiency and bandwidth of deep dish system by varying design parameters such as feed size and FPA aperture field. A prototype FPA was evaluated on the Westerbork Synthesis Radio Telescope (WSRT) and the resulting efficiency is discussed.     

What Can the Redshift Observed in EXO 0748-676 Tell Us？

The mass-radius relations for bare and crusted strange stars are calculated with the bag model. Comparing these relations with the observed one derived from the redshift of EXO 0748-676, we come to the conclusion that it is incorrect to say that EXO 0748 676 cannot be a strange star. Various strange star models can show that EXO 0748-676 could have a mass of (1.3 - 1.7)M⊙ and a radius of(8.4 - 11.4) km. It is proposed that a proportion of nascent strange stars could be bare and have masses - 0.1 M⊙, and their masses increased over a long period of accretion.     

Kelvin–Helmholtz instability and circulation transfer at an isotropic–anisotropic superfluid interface in a neutron star

A recent laboratory experiment suggests that a Kelvin–Helmholtz (KH) instability at the interface between two superfluids – one rotating and anisotropic, the other stationary and isotropic – may trigger sudden spin-up of the stationary superfluid. This result suggests that a KH instability at the crust–core (  ¹ S₀–³ P₂  –superfluid) boundary of a neutron star may provide a trigger mechanism for pulsar glitches. We calculate the dispersion relation of the KH instability involving two different superfluids including the normal fluid components and their effects on stability, particularly entropy transport. We show that an entropy difference between the core and crust superfluids reduces the threshold differential shear velocity and threshold crust–core density ratio. We evaluate the wavelength of maximum growth of the instability for neutron star parameters and find the resultant circulation transfer to be within the range observed in pulsar glitches.     

Strange Stars： Can Their Crust Reach the Neutron Drip Density？

The electrostatic potential of electrons near the surface of static strange stars at zero temperature is studied within the frame of the MIT bag model. We find that for QCD parameters within rather wide ranges, if the nuclear crust on the strange star is at a density leading to neutron drip, then the electrostatic potential will be insufficient to establish an outwardly directed electric field, which is crucial for the survival of such a crust. If a minimum gap width of 200 fm is brought in as a more stringent constraint, then our calculations will completely rule out the possibility of such crusts. Therefore, our results argue against the existence of neutron-drip crusts in nature.