全站仪测程检验的一种新方法

测程是全站仪重要技术指标之一,本文从相位式测距仪的测程公式出发,探讨了在短基线或短距离上进行测程检测的原理和方法,为中、长程全站仪的测程检验提供了可能性。这种检验方法是在短基线或短距离上用改变反射镜有效面积进行测程实验,操作简单方便,结果可靠。利用本文研究成果可以算出任意棱镜组合所对应的测程,这样可更合理地使用棱镜,以便减少仪器幅相误差的影响,提高测程精度。     

一种适用任意距离的大地主题解算方法的研究和试验

介绍了嵌套系数法解算大地主题问题的原理和公式;并以详尽的算例对该方法进行了实验和分析,与贝塞尔方法以及高斯平均约数算法相比较,指出该算法是一种适用于任意大地距离的高精度算法,并且不存在奇异问题。     

层状极化介质激发极化效应特征研究

这里研究层状极化介质激发极化效应特征。首先,在忽略电磁效应的情况下,用柯尔～柯尔模型表征极化介质复电阻率,计算三层不同地电断面复电阻率的振幅和相位随极距变化的曲线;然后,分析极化层不同充电率和不同时间常数、不同激发频率和极化层不同埋深,对测深曲线的影响规律,并提出了具有实际指导意义的极化层埋深与极距的对应关系。这些工作都能够为野外开展复电阻率测量和资料解释起到参考作用。     

鹤岗地震台面波震级偏差分析

在地震震级国家标准《地震震级的规定》(GB17740—2017)发布以后,收集整理鹤岗地震台2018年1月—2020年3月测定的远震面波震级M_(S(HEG)),与中国地震台网中心地震目录中给定的面波震级M_(S(CENC))进行比较,统计二者偏差值。利用统计学方法,分析震级偏差与震级、震中距和反方位角的关系。结果表明:与中国地震台网中心地震目录发布震级相比,鹤岗地震台测定的面波震级偏高,且震级偏差与震中距表现为正相关性;震中位于鹤岗地震台站西北方位,震级偏差较小,而在其他方位,震级偏差则较大。     

Lateral and longitudinal flight dispersals of a stonefly,Alloperla ishikariana (Plecoptera,Chloroperlidae), from the hyporheic zone in a gravel-bed river in Japan

The life-history traits of amphibitic insects are not well understood. These insects inhabit saturated interstitial areas below the riverbed (hyporheic zone) at the larval stage, mate in terrestrial habitats, and return to rivers for oviposition, but there is no knowledge concerning their dispersal characteristics. We sought to address this by examining how far amphibitic insects disperse away from the channel (laterally) and along upstream or downstream (longitudinally) in a gravel-bed river. Alloperla ishikariana was selected as the focal species because it numerically dominates other amphibites in an 18-km study segment of a 4th-order gravel-bed river in Hokkaido, Northern Japan. Malaise traps were set at various distances from the channel towards the riparian forest to estimate lateral dispersal distances. An elevated stable nitrogen isotope ratio in downstream larvae, caused by the influence of effluent from a wastewater treatment plant, was used to assess longitudinal dispersal by identifying and tracking adult movements. Laterally, 50th and 90th percentile dispersal distances were 11.66 and 35.09 m for female A. ishikariana and 20.59 and 59.20 m for male, respectively; this overlapped with distances previously estimated for other aquatic benthic taxa. Longitudinally, 50th and 90th percentile dispersal distances were 0.74 and 1.43 km for female and 3.11 and 7.87 km for male, respectively. Alloperla ishikariana had one of the longest upstream traveling distances compared with other aquatic insects, and the longest among Plecoptera taxa known thus far where male exhibited a greater dispersal distance. A higher number of adults demonstrated upstream movement, suggesting an upstream bias in the longitudinal dispersal of A. ishikariana. Overall, amphibitic stoneflies did not exhibit distinct dispersal characteristics compared with the results of previous reports on presumably benthic taxa. Our findings support an improved visualization of a multi-dimensionally connected river ecosystem in terms of material flow, including vertical connectivity.     

三维完全欧氏距离变换的改进算法

三维欧氏距离变换是对由黑白像素构成的三维二值图像中所有像素找出其到最近黑色像素的欧氏距离。在对现有三维欧氏距离变换算法进行深入研究的基础上,充分利用二维欧氏距离变换的结果,进一步减少参与距离计算和比较的黑点个数,进而提出了三维完全欧氏距离变换的改进算法。整个算法的时间复杂度为O((n3log n)/φ(n))。并将该改进算法应用于海底污染源的扩散分析,取得了较好的效果。     

基于影像尺度空间表达与鲁棒Hausdorff距离的快速角点特征匹配方法

快速影像匹配是进行影像时间序列分析与飞行器导航的重要方法.本文对待匹配影像进行高斯低通滤波预处理时,运用影像的尺度空间表达思想对不同分辨率的基准影像和实时影像选择了相应的σ值进行卷积滤波处理,使基准影像和实时影像具有相近的分辨率,从而提高两影像所提取角点的重复率,使得影像的正确匹配概率得到提高.然后用基于影像几何结构分析的改进的快速角点探测算法进行了影像的角点提取;最后用本文提出的改进的鲁棒Hausdorff距离进行了基准影像和实时影像的匹配.实验证明,本文方法对影像噪声和灰度变化不敏感,具有抗影像尺度变化的能力.在基准影像和实时影像灰度差变化较大的情况下,依然能取得较高的正确匹配概率.由于采用基于影像信息量评价的搜索策略和快速角点提取算法,匹配速度也较快.     

A new method for spatial centrographic analysis of mineral deposit clusters

A centrographic method for analysing mineral deposit clusters is illustrated using the komatiite-hosted Kambalda nickel sulphide deposit cluster, Yilgarn craton, Western Australia. In this method, the standard distance circle divides the cluster into a more endowed inner part and a less endowed peripheral part. The standard deviational ellipse, another centrographic object, depicts the preferred northwest–southeast trend of nickel orebodies at Kambalda. Weighted centrography shows that nickel endowment is greater in the eastern than western part of the cluster. The spatio-geometric interaction of the circle and ellipse splits the cluster into several partitions. The relative concentration of nickel orebodies or endowment within a partition in relation to their concentration within the entire cluster is termed ‘capture efficiency’. Komatiite areal trace exhibits higher nickel orebody capture efficiency than spatio-geometric partitions; however, some spatio-geometric partitions exhibit nickel endowment capture efficiencies comparable to that of komatiite. Furthermore, nickel orebody and endowment capture efficiencies of komatiite are elevated only within the standard distance circle. These results suggest that at Kambalda, (i) the standard distance circle is a prime window for understanding the komatiite-hosted nickel system, and (ii) spatio-geometric partitions are plausible locales for spatial analysis of nickel orebodies and endowment. The proposed centrographic method is potentially useful in mineral resource estimations and mineral exploration targeting.     

Estimating the redshift distribution of photometric galaxy samples – II. Applications and tests of a new method

In Lima et al. we presented a new method for estimating the redshift distribution,   N ( z )  , of a photometric galaxy sample, using photometric observables and weighted sampling from a spectroscopic subsample of the data. In this paper, we extend this method and explore various applications of it, using both simulations and real data from the Sloan Digital Sky Survey (SDSS). In addition to estimating the redshift distribution for an entire sample, the weighting method enables accurate estimates of the redshift probability distribution,   p ( z )  , for each galaxy in a photometric sample. Use of   p ( z )  in cosmological analyses can substantially reduce biases associated with traditional photometric redshifts, in which a single redshift estimate is associated with each galaxy. The weighting procedure also naturally indicates which galaxies in the photometric sample are expected to have accurate redshift estimates, namely those that lie in regions of photometric-observable space that are well sampled by the spectroscopic subsample. In addition to providing a method that has some advantages over standard photo- z estimates, the weights method can also be used in conjunction with photo- z estimates e.g. by providing improved estimation of   N ( z )  via deconvolution of   N ( z _phot)  and improved estimates of photo- z scatter and bias. We present a publicly available   p ( z )  catalogue for ∼78 million SDSS DR7 galaxies.