一种实用的地面数字化成图方法——简别码法

介绍一种由简别码(简码加判别码)代替编码法草图法地面数字成图的方法。与现行方法相比,该方法编码容易,操作简单方便,野外采集数据速度快,内业根据生成的简别码判读方便、编辑速度快,提高了整个成图工作的效率。     

云南永胜宝坪浅源热液改造型铜矿地质及成因

宝坪铜矿赋存于三叠系下统腊美组中。矿体呈似层状,少量脉状,严格受北北西-北西向构造控制。矿床成因类型属浅源热液改造型铜矿床。     

CDN技术在国土资源信息服务系统中的应用——以资源网为例

国土资源信息服务类网站信息服务覆盖广、浏览量大、易受到黑客和病毒的攻击。本文以资源网为例,主要介绍CDN技术在国土资源信息服务系统中的应用。CDN技术的引入,可以大规模多区域加速,保证用户的就近访问,隐藏源站服务器,对于提高国土资源信息服务类网站的响应速度,提高网站的安全性具有重大的现实意义。     

合肥市建设用地管理信息系统建设

本文在合肥市金土工程试点建设的背景下,通过对合肥市建设用地报批业务的分析和梳理,建立了建设用地报批管理业务模型和工作流程,完成了合肥市建设用地管理系统的设计与开发,并对系统的应用情况做了简要的介绍,对系统应用中存在的实际问题,提出了完善的建议措施。     

陕西宝鸡地区塌山黄土滑坡三维稳定性分析

在前人研究的基础上．以宝鸡市千阳县城关镇塌山黄土滑坡为例．运用有限元法探索黄土滑坡的三维稳定性评价分析方法。针对黄土滑坡体结构构造的复杂性和滑体、滑带、滑床的显著差异性．运用有限元三维稳定性分析方法分别计算了滑体与滑带不同部位的安全系数。计算结果表明：塌山黄土滑坡现今处于基本稳定状态,滑体不同部位的稳定性系数与野外调查滑体现今的变形迹象基本一致．表明该评价分析方法具有一定的可行性．基本适用于黄土地区滑坡的三维稳定性分析。     

测井仪器的故障分析与排除思路

TYSC-3Q与PSJ-2型数字测井仪是目前煤田测井中常用的二种测井仪器,在使用过程中难免发生诸如测井控制故障、声速探管故障、密度三侧向探管故障、井温、井液电阻率探管故障、电法面板故障、数字测井面板故障、电测井故障等常见故障类型。通过对各类故障因素进行剖析,指出了故障易发生的部位,并详细的介绍了检查的方法及故障的排除步骤。     

基于道路特征的海量GPS监控数据压缩方法

结合车辆的运动轨迹只能被限制于道路网络上的事实约束,提出了一种基于道路特征的车辆监控数据存储管理方法,存储车辆在道路网特征点处的信息,通过将原始数据中存储的二维地理坐标转换为存储一维的沿道路网的线性参照坐标实现了监控数据和道路网的结合,可极大地节省GPS车辆跟踪数据的存储空间,有利于对车辆数据的进一步分析利用和交通信息的提取.     

A solar flare in the Fe I 5324 line on 24 June, 1993

A solar flare with both H and Fe i 5324 emissions was observed in AR 7529 (S13, E65) on 24 June, 1993 at the Bejing Astronomical Observatory. Our calculations show that the Fe i 5324 emission region of the flare was located in the low photosphere at a height of about 180 km above ₅₀₀₀ = 1, which is lower than many previous studies of white-light flares. To study a Fe i 5324 flare, which represents a kind of extreme case in solar flares, would be useful for clarifying some arguments in the researches of white-light flares as well as for understanding the mechanism of solar flares.The synthetic analyses from vairous features of the flare lead to the following possible exciting mechanism of the Fe i 5324 flare: owing to the flow of energetic electrons from the corona and probably also the thermal conduction downward into the lower atmosphere, a condensation with a temperature higher than that below it was formed near the transition region. Then the low photosphere was heated through backwarming. The Fe i 5324 flare occurred as an indicator of the excitation in the low photosphere.     

Configuration of the chromospheric magnetic field in a unipolar sunspot region

A set of H chromospheric magnetograms at various wavelengths near the line center, chromospheric Dopplergrams, and photospheric vector magnetograms of a unipolar sunspot region near the solar limb were obtained with the vector video magnetograph at the Huairou Solar Observing Station. The superpenumbral chromospheric magnetic field is almost parallel to the surface at the outside of the sunspot penumbra, where the magnetic lines of force are mainly concentrated in the superpenumbral filaments. In the gaps between the filaments the chromospheric horizontal field is weak.