知识图谱发展与构建的研究进展

近年来知识图谱技术引起了广泛的关注和研究,本文介绍了近期知识图谱的发展、构建方法、详细的构建过程,并对知识图谱在交叉学科领域的应用和未来的研究方向做了总结.本文详细介绍了构建文本知识图谱、视觉知识图谱、多模态知识图谱的关键技术,比如信息提取、知识融合、知识表示等.作为知识工程的重要组成部分,知识图谱,尤其是多模态知识图谱的发展对大数据时代的高效知识管理、知识获取、知识共享有着重要的意义.     

Casio fx-9860G SD编制导线测量电子手簿

本文根据导线测量手簿的要求,运用casio计算器及其编程语言,编制导线测量的电子手簿。将检核条件加入该程序,进行外业导线测量记录,在计算机中导入数据,结合VB语言编程,在excel中生成完整手簿,以及南方平差文件。     

高分辨率SAR图像中建筑物特征融合检测算法

针对高分辨率SAR图像中的建筑物检测问题,提出了一种基于视觉注意和特征融合的检测算法。首先,根据SAR图像中建筑物目标与背景存在较大差异的特点,采用视觉注意机制进行建筑物的感兴趣区分割;然后,提取位于感兴趣区域内的高亮线条和阴影区域;最后,采用D-S证据理论对注意焦点、高亮线条和阴影区域进行特征融合,实现建筑物目标的检测。实验结果表明,本文算法对矩形建筑物具有较高的检测精度。     

计算机自动识别分类技术在森林遥感中的应用

本文叙述应用计算机自动识别分类技术在航天遥感图像中对森林资源进行分类的一些探索研究。本文介绍了采用自编程序“地理坐标系和图像坐标系的精密仿射变换”、“识别型增强技术”、“多光谱信息的特征提取”、“多光谱模糊算法聚类分析”等一系列算法后所取得的分类图像结果,与实地及目视解译相比较,森林分类相对精度达90％。     

Speckle observations with PISCO in Merate: XIII. Astrometric measurements of visual binaries in 2012, and new orbits for ADS 10786 BC, 12144, 12515, 16314 and 16539

We present relative astrometric measurements of visual binaries, made in 2012 with the speckle camera PISCO at the 102‐cm Zeiss telescope of Brera Astronomical Observatory, in Merate. Our observing list contains orbital couples as well as binaries whose motion is still uncertain. We obtained 355 new measurements of 344 visual binary stars, with angular separations in the range 0′.14–6′.9, and an average accuracy of 0.′02. The mean error on the position angles is 0°.5. Most of the position angles were determined without the usual 180° ambiguity with the application of triple‐correlation techniques and/or by inspection of the long integration files. We also present new revised orbits for ADS 10786 BC, 12144, 12515, 16314, and 16539, partly derived from PISCO observations. The corresponding estimated values for the masses of those systems are compatible with the spectral types. (© 2014 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

Measurements of visual double stars with PISCO2 at the Nice 76-cm refractor in 2013–2014 (new data) and in 2015

We present relative astrometric and photometric measurements of visual double stars made in 2013–2015, with PISCO2 installed at the 76-cm refractor of Côte d'Azur Observatory in Nice (France). Our observing list contains orbital couples as well as double stars whose motion is still uncertain. Most of the observations were done in 2015, but some other observations of wide couples were done in 2013–2014 (0.3% of the total of the observations). Three different techniques were used for obtaining measurements: lucky imaging, speckle interferometry and the direct vector autocorrelation method. From our observations of 2837 multiple stars, we obtained 5182 new measurements with angular separations in the range of 0 ${}^{″}$.1–32 ${}^{″}$ and an average accuracy of $0^{″}.018$. The mean error on the position angles is 0°.8. Most of the position angles were determined without the usual 180° ambiguity with the application of the direct vector autocorrelation technique and/or by inspection of the Lucky images or the long integration files. We managed to routinely monitor faint systems ( $m_V\approx 9-11$) with large magnitude difference (up to $\mathrm{\Delta }{m}_V\approx 4.5$). We have thus been able to measure 21 systems containing red dwarf stars that had been poorly monitored since their discovery, from which we estimated the stellar masses thanks to Gaia measurements. We also measured the magnitude difference of the two components of 1079 double stars with an estimated error of 0.2 mag. Except for a few objects that are discussed, our measurements are in good agreement with the ephemerides computed with published orbital elements, even for the double stars whose separation is smaller than the diffraction limit. Thanks to good seeing images and with the use of high-contrast numerical filters, we have also been able to obtain 196 measurements with an angular separation smaller than the diffraction limit of our instrumentation, and consistent with those obtained with larger telescopes. We also report measurements of the 164 new double stars that we found in the files obtained during the observations. Finally, from a study of the DR3 Gaia release, it is shown that all the objects of the Tycho Double Star Catalog that we did not resolve in 2015 are probably false detections by Tycho.     

新时代《地图学》的教学思考

随着时代发展和技术演进,地图学的内容不断丰富和演化。《地图学》是很多地学相关专业的专业基础课,但在教学过程中仍存在一些问题,结合多年教学经验,从教学内容、教学方法、实践应用等方面进行了一些思索与探讨。