基于GIS与三维激光扫描的古建筑保护研究

以三维激光扫描点云数据作为基础数据，以河南大学明伦校区近代建筑群为研究对象，结合地理数据库和三维建模技术，建立了古建筑数据库利用ArcGIS Engine二次开发平台，设计了基于GIS的古建筑数字化保护系统，并同时探讨了系统建立过程中的若干技术问题：研究结果说明，基于三维激光扫描和GIS的新技术手段，为古建筑的数字化保护带来了新的契机。     

Documentation of Istanbul Historic Peninsula by Kinematic Terrestrial Laser Scanning

Although the Historic Peninsula of old Istanbul was added to the UNESCO World Heritage List in 1985, complete documentation of this important area has not yet been carried out. In 2006 the Istanbul Metropolitan Municipality's Historical Environment Protection Directorate initiated the "Historic Peninsula Project", which covers an area of 1500 ha and includes approximately 48 000 buildings in crowded and frequently narrow streets. BİMTAŞ, a company owned by the Municipality, immediately started the documentation of all buildings in the project area using terrestrial laser scanning. This created the challenge of building up an efficient production environment with new high-end technology to fulfil the requirements of this project in a very short timeframe of 2 years. This paper describes the entire production environment for documentation of all buildings, detailing the frequent adaptations of the process resulting from learning on the job. Although the data acquisition and mapping environment was established in the course of production, it was always essential to optimise the technical solutions in order to meet the requirements for data quality and delivery deadlines. Only 80 ha of the required 1500 ha was completed using static scanning during the first 6 months, thus requiring a change from static to mobile terrestrial laser scanning in order to accelerate the work and to conclude the scanning phase for the remaining major area within 3 months.     

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Hydroxyl in mantle olivine xenocrysts from the Udachnaya kimberlite pipe

The incorporation of hydrogen in mantle olivine xenocrysts from the Udachnaya kimberlite pipe was investigated by Fourier-transform infrared spectroscopy and secondary ion mass spectrometry (SIMS). IR spectra were collected in the OH stretching region on oriented single crystals using a conventional IR source at ambient conditions and in situ at temperatures down to −180°C as well as with IR synchrotron radiation. The IR spectra of the samples are complex containing more than 20 strongly polarized OH bands in the range 3,730–3,330 cm⁻¹. Bands at high energies (3,730–3,670 cm⁻¹) were assigned to inclusions of serpentine, talc and the 10 Å phase. All other bands are believed to be intrinsic to olivine. The corresponding point defects are (a) associated with vacant Si sites (3,607 cm⁻¹ E || a, 3,597 E || a, 3,571 cm⁻¹ E || c, 3,567 E || c, and 3,556 E || b), and (b) with vacant M1 sites (most of the bands polarized parallel to a). From the pleochroic behavior and position of the OH bands associated with the vacant M1 sites, we propose two types of hydrogen—one bonded to O1 and another to O2, so that both OH vectors are strongly aligned parallel to a. The O2–H groups may be responsible for the OH bands at higher wavenumbers than those for the O1–H groups. The multiplicity of the corresponding OH bands in the spectra can be explained by different chemical environments and by slightly different distortions of the M1 sites in these high-pressure olivines. Four samples were investigated by SIMS. The calculated integral molar absorption coefficient using the IR and SIMS results of 37,500±5,000 L mol H₂O cm⁻² is within the uncertainties slightly higher than the value determined by Bell et al. (J Geophys Res 108(B2):2105–2113, 2003) (28,450±1,830 L mol H₂O cm⁻²). The reason for the difference is the different distributions of the absorption intensity of the spectra of both studies (mean wavenumber 3,548 vs. 3,570 cm⁻¹). Olivine samples with a mean wavenumber of about 3,548 cm⁻¹ should be quantified with the absorption coefficient as determined in this study; those containing more bands at higher wavenumber (mean wavenumber 3,570 cm⁻¹) should be quantified using the value determined by Bell et al. (J Geophys Res 108(B2):2105–2113, 2003).

2019年广西北流—广东化州MS 5.2地震前活动性参数异常分析

2019年10月12日,广西北流—广东化州交界发生M_S 5.2地震,选取广西北流—广东化州区域2010年1月1日—2019年12月31日M_L≥2.0地震目录,对震前地震活动性参数进行时空扫描,并进行地震空区分析,发现部分地震活动性参数异常,且震前存在孕震空区。分析结果如下：震前b值时间扫描曲线长期位于均值线之上,持续时间一年以上;b、C、D值空间扫描均存在异常,其中震前b值异常范围为1.0—2.0,C值异常范围为0.04—0.32,D值异常范围为0.01—0.09;2016年4月至2019年9月,震中附近出现孕震空区,后在空区边缘发生此次M_S 5.2地震。     

Polarization in IR bands and the structure of cosmic dust grains

The water ice and silicate dust bands centered at about 3 and 10 μm, respectively, are simultaneously observed in the spectra of several objects. So far the wavelength dependence of the polarization in both bands has been modeled using two-layer spheroids, with the shape of the silicate core being confocal to that of the ice mantle. We show that nonconfocality of the spheroidal core and mantle boundaries changes fundamentally the wavelength dependence of the polarization within the 10-μm silicate band and affects significantly the polarization within the 3-μm water ice band, while the extinction profiles of these bands remain essentially unchanged. Since the results have been obtained for a theoretical model, we discuss their applicability and significance for cosmic dust grains. Original Russian Text ? M.S. Prokopjeva, V.B. Il’in, 2007, published in Pis’ma v Astronomicheskiĭ Zhurnal, 2007, Vol. 33, No. 10, pp. 784–791.     

三维激光扫描技术在双龙洞测量中的应用

介绍了三维激光扫描技术在金华双龙洞测量中的应用情况。这一研究不仅提高了洞穴测量的工作精度和工作效率,还为洞穴内部地貌与地质体形态三维可视化构建、虚拟洞穴内部地理场景构建、洞穴地理信息系统建设提供数据源,为洞穴数据库建设、洞穴景观旅游开发、洞穴环境与景观保护、洞穴考古等提供直观精密的基础数据。     

基于投影点密度的车载激光扫描距离图像分割方法

对车载激光扫描系统获取的距离图像的分割进行研究,提出利用投影点密度进行距离图像分割的方法.该方法不需要其他辅助数据就可以进行距离图像的分割,给出应用实例.图像的分割是目标识别、定位、特征提取与建模的基础和关键.距离图像是离散坐标点阵列,不表达目标边界特征和拓扑关系,到目前为止还没有距离图像分割的成熟、可行方法.本文研究成果,展现了激光扫描技术在数据获取、处理研究上的新方向.     

基于多尺度、多图幅地理空间基础的输电信息系统的研究与实践

正确、及时、全面地获取输电网络的各种资源信息,并加以提炼、分析,实现输电管理部门间的协同工作和信息共享,为管理者和决策者提供辅助决策依据,从而保障输电网络安全、高效地运行,提高企业的综合经济效益,降低电网运行维护中的损耗[1]。本文提出了采用C/S+B/S两种开发模式相结合的混合体系结构作为系统的总体解决方案。以ESR I公司的ArcG IS系列产品作为基础的GIS开发系统,以.NET的核心语言C#作为系统的最终开发语言。同时,功能强大的数据库软件Oracle和空间数据库引擎ArcSDE为系统统一协调、并发处理以及共享分布各种信息提供了可靠的保障。该系统具有界面友好、方便实用、安全稳定、兼容性强、伸缩性强和可扩展性强等优点。该系统已推广和应用到部分地市,具有极其广阔的推广应用前景。     

三维辐射传输模式分析非均匀云对天空辐射场影响

为了解非均匀分立云体分布状况下的天空辐射场与无云晴空辐射场的差异, 本文借助一个三维辐射传输数值模式SHDOM模拟了离散云块分布条件下的天空辐射场分布, 重点分析不同云况分布情况下“非云”大气的辐射分布特征, 并将该区域与无云晴空大气辐射场的相同区域进行了比对。工作主要从辐亮度以及450 nm/650 nm的辐射比两参数入手进行讨论。研究发现, 相对无云晴空大气, 云的存在会对周围“非云”大气散射辐射产生影响, 影响程度与云量、云及气溶胶光学厚度等参数相关。数值模拟结果表明, 在云量不太大的条件下, 无云视场空间的大部分辐射值与无云晴空相比变化很小, 集中在±2％之间。这一结果表明, 已有的一维均匀大气辐射传输模式运算结果所得云与非云相元的判据基本适用于非均匀分布的有云大气。另一方面, 模拟结果表明我们也完全可以利用非均匀有云大气中的无云视场观测结果进行大气气溶胶等晴空大气光学特征的探测研究。