基于VBA的断面图绘制程序的实现     

范亚男  周宇 《测绘信息与工程》2014,(3):68-70

断面测量作为城市测量工作中的重要组成部分,其在市政设计及施工中起着重要作用。断面图作为断面测量工作提交给客户的重要成果资料,占有较大比重。断面图的绘制一般都有业主单位的特殊要求,绘制过程较为复杂,工作量较大。本文从实际工作出发,分析断面图绘制中可以提高效率的部分工作,并设计和编写程序以提高工作效率。  相似文献   

高速铁路沉降数据处理与评估系统设计与实现     

许双安  任晓春  袁永信 《测绘信息与工程》2014,(4):54-57

详述了高速铁路沉降观测数据处理与评估系统的设计与实现,重点对系统的设计思想、总体结构、基本功能和主要特点进行了详细叙述。  相似文献   

对我国政府在全球采掘业透明倡议中应持立场的思考和建议     

陈丽萍  孙春强  马永正  姜雅 《国土资源情报》2014,(3):24-32

历经10余年的发展,采掘业透明倡议已经发生了巨大变化,西方发达国家开始积极介入,主动宣布试点或计划实施。形势的变化要求我国及时调整以往所持立场。本文简要介绍了全球采掘业透明倡议的组织架构及运作、实施现状,深入分析了各利益相关方的动机,对其未来发展加以研判,并结合我国涉及采掘业透明倡议的情况,提出了新形势下我国短期内不宜实施,但须及时调整立场;鼓励金融机构和企业介入EITI和其他反腐败倡议;政府应考虑成为EITI的正式支持国。  相似文献   

客运专线轨检小车测量控制系统研究与开发     

王涛  谢忠俍  张亚 《测绘与空间地理信息》2014,(3):16-18

针对国内某轨检小车研发项目,采用模块化的程序设计集成开发环境Microsoft Visual Studio.NET,开发出了一套功能完善的高速铁路轨道检测控制系统。该系统以高速铁路精密定轨测量原理方法为基础,采用模块化的程序设计思路,实现了轨道检测数据的自动采集、自动记录、自动数据分析和平差处理、成果显示和自动检核等功能。工程应用实践表明,该检测系统运行稳定可靠,检测精度高,具有一定的实用性和推广价值。  相似文献   

Catalog of cosmic gamma-ray bursts from the KONUS experiment data     

E. P. Mazets  S. V. Golenetskii  V. N. Ilyinskii  V. N. Panov  R. L. Aptekar  Yu. A. Guryan  M. P. Proskura  I. A. Sokolov  Z. Ya. Sokolova  T. V. Kharitonova  A. V. Dyatchkov  N. G. Khavenson 《Astrophysics and Space Science》1981,80(1):3-83

Data are presented on the temporal structure, fluxes, energy spectra and coordinates of the sources of gamma-ray bursts detected in the KONUS experiment on Venera 11 and Venera 12 space probes in the period September 1978 to May 1979. The statistical distributions of gamma bursts in duration, intensity, and peak power, as well as the distribution of the burst sources over the celestial sphere presented are based on the updated KONUS information obtained until February 1980.  相似文献   

3种贝类糖胺聚糖的粗提及含量比较     

刘亚  吴晓萍  章超桦  付武君  温尔佳 《广东海洋大学学报》2006,26(3):61-63

以企鹅珍珠贝、菲律宾蛤仔和锯齿巴非蛤全脏器为原料,经酶解、离心去蛋白、醇沉、分离、洗涤、干燥,得糖胺聚糖(GAG)粗制品,分别测定并比较3种贝类的GAG的含量和得率。结果表明,企鹅珍珠贝的GAG质量分数为22.35%,菲律宾蛤仔为18.69%,锯齿巴非蛤为20.36%,由此得出企鹅珍珠贝的GAG的含量比其他两种贝类高,是较好的GAG来源。  相似文献   

Effects of land use and cultivation time on soil organic and inorganic carbon storage in deep soils     

Yu  Xia  Zhou  Weijian  Wang  Yunqiang  Cheng  Peng  Hou  Yaoyao  Xiong  Xiaohu  Du  Hua  Yang  Ling  Wang  Ya 《地理学报(英文版)》2020,30(6):921-934

The vertical distribution and exchange mechanisms of soil organic and inorganic carbon(SOC, SIC) play an important role in assessing carbon(C) cycling and budgets. However, the impact of land use through time for deep soil C(below 100 cm) is not well known. To investigate deep C storage under different land uses and evaluate how it changes with time, we collected soil samples to a depth of 500 cm in a soil profile in the Gutun watershed on the Chinese Loess Plateau(CLP); and determined SOC, SIC, and bulk density. The magnitude of SOC stocks in the 0–500 cm depth range fell into the following ranking: shrubland(17.2 kg m~(-2)) grassland(16.3 kg m~(-2)) forestland(15.2 kg m~(-2)) cropland(14.1 kg m~(-2)) gully land(6.4 kg m~(-2)). The ranking for SIC stocks were: grassland(104.1 kg m~(-2)) forestland(96.2 kg m~(-2)) shrubland(90.6 kg m~(-2)) cropland(82.4 kg m~(-2)) gully land(50.3 kg m~(-2)). Respective SOC and SIC stocks were at least 1.6-and 2.1-fold higher within the 100–500 cm depth range, as compared to the 0–100 cm depth range. Overall SOC and SIC stocks decreased significantly from the 5 th to the 15 th year of cultivation in croplands, and generally increased up to the 70 th year. Both SOC and SIC stocks showed a turning point at 15 years cultivation, which should be considered when evaluating soil C sequestration. Estimates of C stocks greatly depends on soil sampling depth, and understanding the influences of land use and time will improve soil productivity and conservation in regions with deep soils.  相似文献   

An efficient and adaptive approach for modeling gravity effects in spherical coordinates     

Zhiwei Li  Tianyao Hao  Ya Xu  Yi Xu 《Journal of Applied Geophysics》2011,73(3):221-231

The need to obtain more reliable Earth structures has been the impetus for conducting joint inversions of disparate geophysical datasets. For seismic arrival time tomography, joint inversion of arrival time and gravity data has become an important way to investigate velocity structure of the crust and upper mantle. However, the absence of an efficient approach for modeling gravity effects in spherical coordinates limits the joint tomographic analysis to only local scales. In order to extend the joint tomographic inversion into spherical coordinates, and enable it to be feasible for regional studies, we develop an efficient and adaptive approach for modeling gravity effects in spherical coordinates based on the longitudinal/latitudinal grid spacing. The complete gravity effects of spherical prisms, including gravitational potential, gravity vector and tensor gradients, are calculated by numerical integration of the Gauss–Legendre quadrature (GLQ). To ensure the efficiency of the gravity modeling, spherical prisms are recursively subdivided into smaller units according to their distances to the observation point. This approach is compatible with the parameterization of regional arrival time tomography for large areas, in which both the near- and far-field effects of the Earth's curvature cannot be ignored. Therefore, this approach can be implemented into the joint tomographic inversion of arrival time and gravity data conveniently. As practical applications, the complete gravity effects of a single anomalous density body have been calculated, and the gravity anomalies of two tomographic models in the Taiwan region have also been obtained using empirical relationships between P-wave velocity and density.  相似文献   

Estimating the dark halo mass from the relative thickness of stellar disks     

N. Ya. Sotnikova  S. A. Rodionov 《Astronomy Letters》2006,32(10):649-660

We analyze the relationship between the mass of a spherical component and the minimum possible thickness of stable stellar disks. This relationship for real galaxies allows the lower limit on the dark halo mass to be estimated (the thinner the stable stellar disk is, the more massive the dark halo must be). In our analysis, we use both theoretical relations and numerical N-body simulations of the dynamical evolution of thin disks in the presence of spherical components with different density profiles and different masses. We conclude that the theoretical relationship between the thickness of disk galaxies and the mass of their spherical components is a lower envelope for the model data points. We recommend using this theoretical relationship to estimate the lower limit for the dark halo mass in galaxies. The estimate obtained turns out to be weak. Even for the thinnest galaxies, the dark halo mass within four exponential disk scale lengths must be more than one stellar disk mass.  相似文献   

Interacting galaxies: Observational and theoretical aspects     

V. P. Reshetnikov  N. Ya. Sotnikova 《Astrophysics》1993,36(3):265-292

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