关于地理信息产业的发展及几点建议

进入信息时代 ,地理信息产业迅速发展 ,取得巨大的成果 ,现代化的地理信息产品和技术服务在经济与社会可持续发展中的重要作用越来越明显 ,因此发展地理信息产业自然成为更为重要的任务     

基于单齿侵入理论的牙轮钻头钻速方程

考虑井底水平地应力、钻井流体压力及地层孔隙压力,基于单齿侵入理论推导单齿侵入井底岩石的侵深公式,建立纯滚动锥形齿、楔形齿和滚动、剪切复合运动锥形齿等牙轮钻头的钻速方程.通过实验分析刃尖角、井底液柱压力对单齿侵入深度的影响,以及转速、轴向载荷对微钻头、牙轮钻头机械钻速的影响.结果表明:随着牙齿刃尖角的增大,锥形齿和楔形齿的侵深呈指数递减趋势;随着井底液柱压力的增大,牙齿侵入深度呈指数递减趋势,其中锥形齿降低速率大.在软到中硬地层中,牙齿侵入深度大,冲击侵入、回转剪切复合破岩方式的破岩效率高;在硬度地层中,牙齿侵入深度小,纯滚动冲击侵入破岩效率高.为分析实钻时牙轮钻头的机械钻速提供计算方法.     

基于语义规则和词向量的台风灾害网络情感分析方法

灾害期间的舆情引导有助于维护社会稳定。社交媒体是舆论传播的重要渠道,通过微博评论了解用户的网络情感及关注的话题,可以帮助相关舆情监测部门掌握公众的关注热点,从而选择适当的干预节点来应对网络舆情,并对公众情绪进行疏导,这对于应急管理具有现实意义。现有的研究大多是利用有监督的机器学习方法进行情感分类,这需要人工进行语料的标注,工作量大。本文根据微博评论文本的特点,综合考虑情感词以及表情符号等多重情感源,构建了台风灾害领域情感词典。在此基础上,提出了一种基于情感词语义规则的情感倾向计算方法,以及基于词向量的话题聚类方法。首先,采集了近年5次台风灾害期间共计40多万条微博评论文本,基于大连理工情感词汇本体库进行扩展构建了台风灾害领域情感词典,结合PMI法构建表情符号词典,根据语义规则确定情感倾向,并使用3500条评论文本验证了该方法的有效性。然后,本文基于词向量、TF-IDF与K-means的聚类方法探索灾害期间热点话题。最后,以2020年4号台风“黑格比”为例,基于台风期间的5万余条微博评论文本进行了舆情情感分析,并识别出6类与台风相关的话题。通过时空分析发现,随着时间的推移,微博评论文本的数量发生一定变化,评论数量多的地区大都集中在沿海地区和经济水平高的地区,台风登陆当天浙江省的恐惧情感达到最高。结果表明,基于语义规则和词向量的台风灾害网络情感分析方法,能在类似灾害事件发生时为政府部门掌握和引导网络舆情提供辅助。     

Wavelength calibration by combining arc and night sky lines for LAMOST

A novel method is presented for the wavelength calibration of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST). The proposed method combines the arc lines and night sky lines, and can achieve high performance. Firstly, the initial wavelength calibration is performed by employing arc lines. Afterwards, the centroids of sky lines are calculated by the initial calibration results and adjusted by the gravity method iteratively. Finally, the ultimate wavelength calibration is obtained by fitting the centroids of arc lines and sky lines with their corresponding wavelengths. Experiments are performed on the data observed by LAMOST, and the results of the proposed method are more accurate than that of the calibration only by arc lines or sky lines. The calibration sky lines are dense in the red channel (5,700–9,000 Å) of LAMOST, but only a few ones are in the blue channel (3,700–5,900 Å). The new method achieves excellent results in the red channel as the substantial sky lines are employed, and the calibration accuracy of the blue channel is also enhanced in some degree by the scare sky lines.     

油藏地质建模及实时跟踪研究

为了提高采收率,降低开发风险,以滩海地区某油田为研究对象,结合地质、测井、地震等资料,对该油藏进行实时跟踪地质特征综合研究。应用地质建模、随钻测井、地质导向等技术,建立了精细的三维地质导向模型,并根据随钻测井数据和综合地质信息,实时验证构造和储集层信息,对导向模型不断校正,使模型与实钻结果一致,还以该模型为基础,优化水平井钻井的前进轨迹。结果表明,此种方法的应用降低了海上油田开发风险,能取得良好的开发效果。     

低应变动测桩及锚杆中波的传播规律差异研究

应力波法是检测桩基与锚杆质量的一种快速、有效的无损检测方法,运用该法对桩基与锚杆进行质量检测时均基于一维杆件的波动理论,波速是进行二者质量判断的最基本参数,部分研究和工程技术人员易将两种应力波速混淆,可能会造成实际检测中的误判。为此,以自由锚杆和不同龄期下标准混凝土试块中的应力波速为参考,采用低应变反射波法对桩基和锚杆中的应力波速进行了对比研究。研究表明,桩基中的应力波速与锚杆中的应力波速存在较大的差别,前者略大于标准规格混凝土试件中的波速,而后者小于自由锚杆中的应力波速大于桩基和标准混凝土试块中的波速;桩基和混凝土试块中的应力波速与龄期和强度近似服从上升指数关系,而锚杆中的应力波速与龄期和强度近似服从下降的指数关系。     

Spitzer IRAC infrared colours of submillimetre-bright galaxies

High-redshift submillimetre-bright galaxies identified by blank field surveys at millimetre and submillimetre wavelengths appear in the region of the Infra Red Array Camera (IRAC) colour–colour diagrams previously identified as the domain of luminous active galactic nuclei (AGNs). Our analysis using a set of empirical and theoretical dusty starburst spectral energy distribution (SED) models shows that power-law continuum sources associated with hot dust heated by young (≲100 Myr old), extreme starbursts at z > 2 also occupy the same general area as AGNs in the IRAC colour–colour plots. A detailed comparison of the IRAC colours and SEDs demonstrates that the two populations are distinct from each other, with submillimetre-bright galaxies having a systematically flatter IRAC spectrum (≳1 mag bluer in the observed [4.5]–[8.0] colour). Only about 20 per cent of the objects overlap in the colour–colour plots, and this low fraction suggests that submillimetre galaxies powered by a dust-obscured AGN are not common. The red infrared colours of the submillimetre galaxies are distinct from those of the ubiquitous foreground IRAC sources, and we propose a set of infrared colour selection criteria for identifying SMG counterparts that can be used even in the absence of radio or Multiband Imaging Photometer for Spitzer (MIPS) 24 μm data.     

Labile trace elements in basaltic achondrites: Can they distinguish between meteorites from the Moon,Mars, and V‐type asteroids?

Abstract— We report data for 14 mainly labile trace elements (Ag, Au, Bi, Cd, Cs, Ga, In, Rb, Sb, Se, Te, Tl, U, and Zn) in eight whole‐rock lunar meteorites (Asuka [A‐] 881757, Dar al Gani [DaG] 262, Elephant Moraine [EET] 87521, Queen Alexandra Range [QUE] 93069, QUE 94269, QUE 94281, Yamato [Y‐] 793169, and Y‐981031), and Martian meteorite (DaG 476) and incorporate these into a comparative study of basaltic meteorites from the Moon, Mars, and V‐type asteroids. Multivariate cluster analysis of data for these elements in 14 lunar, 13 Martian, and 34 howardite, eucrite, and diogenite (HED) meteorites demonstrate that materials from these three parents are distinguishable using these markers of late, low‐temperature episodes. This distinguishability is essentially as complete as that based on markers of high‐temperature igneous processes. Concentrations of these elements in 14 lunar meteorites are essentially lognormally distributed and generally more homogeneous than in Martian and HED meteorites. Mean siderophile and labile element concentrations in the 14 lunar meteorites indicate the presence of a CI‐equivalent micrometeorite admixture of 2.6% When only feldspathic samples are considered, our data show a slightly higher value of 3.4% consistent with an increasing micrometeorite content in regolith samples of higher maturity. Concentrations of labile elements in the 8 feldspathic samples hint at the presence of a fractionated highly labile element component, possibly volcanic in origin, at a level comparable to the micrometeorite component. Apparently, the process(es) that contributed to establishing lunar meteorite siderophile and labile trace element contents occurred in a system open to highly labile element transport.     

客观预报方程中因子的选取及应用效果分析

利用因子选取及方程建立人机交互平台,建立了云南省125个气象站的降水、温度客观要素预报方程.对比试验表明,绝大多数组合因子都优于单因子,组合因子预报方程的质量普遍比单因子预报方程好.预报检验结果显示,干季的降水预报尚未达到可用程度,雨季小雨及中雨、大雨的预报有一定业务指导意义,对于反映中小尺度系统的暴雨天气预报效果较差,在因子的选择上还需要做大量细致的工作.温度预报具有一定的参考价值,但还有待进一步改进.     

近距中等光度IRAS星系的射电观测

使用澳大利亚ＡＴ对６个近距中等红外光度的ＩＲＡＳ星系在双频上同时进行了观测．其中ＩＲＡＳ２０２７２－４７３８、ＩＲＡＳ２３１５６－４２３８探测到射电发射．获得了它们的射电流量、峰值位置、源的大小、频谱指数等射电参数,用红外、射电、光学资料对射电源进行了证认．并结合以前的观测资料讨论了这类星系射电发射的特点．