基于小波变换的遥感纹理信息提取

遥感纹理信息是地物空间特征的综合反映,综合纹理信息是进行专题信息提取获取的重要依据.遥感数据具有复杂性、统计性和随机性,同时,遥感图像中地学信息,如地质构造、蚀变信息及岩性分界等高频信息具有一定的方向性;小波变换具有"变焦性"、对称性、正则性等特点,可以较为快速地检测到奇变信号.利用小波变换可以快速、有效地提取遥感纹理高频奇变信息.     

Sources of SEP Acceleration during a Flare – CME Event

A high-speed, halo-type coronal mass ejection (CME), associated with a GOES M4.6 soft X-ray flare in NOAA AR 0180 at S12W29 and an EIT wave and dimming, occurred on 9 November 2002. A complex radio event was observed during the same period. It included narrow-band fluctuations and frequency-drifting features in the metric wavelength range, type III burst groups at metric – hectometric wavelengths, and an interplanetary type II radio burst, which was visible in the dynamic radio spectrum below 14 MHz. To study the association of the recorded solar energetic particle (SEP) populations with the propagating CME and flaring, we perform a multi-wavelength analysis using radio spectral and imaging observations combined with white-light, EUV, hard X-ray, and magnetogram data. Velocity dispersion analysis of the particle distributions (SOHO and Wind in situ observations) provides estimates for the release times of electrons and protons. Our analysis indicates that proton acceleration was delayed compared to the electrons. The dynamics of the interplanetary type II burst identify the burst source as a bow shock created by the fast CME. The type III burst groups, with start times close to the estimated electron-release times, trace electron beams travelling along open field lines into the interplanetary space. The type III bursts seem to encounter a steep density gradient as they overtake the type II shock front, resulting in an abrupt change in the frequency drift rate of the type III burst emission. Our study presents evidence in support of a scenario in which electrons are accelerated low in the corona behind the CME shock front, while protons are accelerated later, possibly at the CME bow shock high in the corona.     

Acoustic-Gravity Waves from Bolide Sources

We have developed a new approach to modeling the acoustic-gravity wave (AGW) radiation from bolide sources. This first effort involves entry modeling of bolide sources that have available satellite data through procedures developed in ReVelle (Earth Moon Planets 95, 441–476, 2004a; in: A. Milani, G. Valsecchi, D. Vokrouhlicky (eds) NEO Fireball Diversity: Energetics-based Entry Modeling and Analysis Techniques, Near-earth Objects: Our Celestial Neighbors (IAU S236), 2007b). Results from the entry modeling are directly coupled to AGW production through line source blast wave theory for the initial wave amplitude and period at (at 10 blast wave radii and perpendicular to the trajectory). The second effort involves the prediction of the formation and or dominance of the propagation of the atmospheric Lamb, edge-wave composite mode in a viscous fluid (Pierce, J. Acoust. Soc. Amer. 35, 1798–1807, 1963) as a function of the source energy, horizontal range and source altitude using the Lamb wave frequency that was deduced directly during the entry modeling and that is used as a surrogate for the source energy. We have also determined that Lamb wave production by bolides at close range decreases dramatically as either the source energy decreases or the source altitude increases. Finally using procedures in Gill (Atmospheric-Ocean Dynamics, 1982) and in Tolstoy (Wave Propagation, 1973), we have analyzed two simple dispersion relationships and have calculated the expected dispersion for the Lamb edge-wave mode and for the excited, propagating internal acoustic waves. Finally, we have used the above formalism to fully evaluate these techniques for four large bolides, namely: the Tunguska bolide of June 30, 1908; the Revelstoke bolide of March 31, 1965; the Crete bolide of June 6, 2002 and the Antarctic bolide of September 3, 2004. Due to page limitations, we will only present results in detail for the Revelstoke bolide.     

FITS图像处理技术荟萃及在太阳观测中的应用

针对FITS图像文件的特点,结合其在天文学领域的广泛应用,对其各种处理技术进行了简明扼要的介绍.包括FITS文件完整性的检查、文件头和数据内容的查看、图像特性的伪彩编码、文件格式的转换、数据的压缩及相关太阳物理信息的提取等内容.     

GIS支持下地震与活动断裂关系研究--以上海及邻近海域为例

以MAPGIS软件为基础平台 ,利用GIS缓冲区分析和空间叠加分析技术 ,研究上海及邻近海域地震与活动断裂的关系。研究区地震活动断裂的发育程度以继承性NE -NNE向为主 ,但其活动强度不及NW -NNW向及近EW向断裂 ;沿NW -NNW向及近EW向断裂两侧 ,中强地震发生频率明显高于NE -NNE向断裂 ;不同时代活动断裂与中强地震之间存在一定的联系 ,表现为随着断裂活动时代变新 ,断裂周围中强地震发生的频率升高。     

重庆市自然灾害管理综合信息系统研究

从重庆市自然灾害情况和自然灾害信息管理现状分析入手,构建了该市自然灾害管理信息系统的系统目标、整体设计和界面的开发。该市自然灾害管理信息系统主要由4个模块组成:自然灾害数据库模块、远程通信管理模块、应用分析模型库和决策支持模块四大部分,四大模块通过一定的数据接口连结,成为一体化系统,对市自然灾害进行有效的管理和监测,从而减少自然灾害带来的经济损失。     

中国棉花种植空间变化及其原因分析

采用地理信息系统软件对1980、1990、2000年中国县域棉花生产数据进行处理,生成棉花种植空间分布差异地图并对之进行分析。分析结果表明,1980～1990年,中国棉花种植空间迅速缩减地区是鄂南、鄂中、湘北、陕西中部、晋西棉区、冀西南棉区以及江苏东部部分地区,种植空间迅速扩展的地区是鲁西北、鲁西南、冀东南和豫南等地区;同时,新疆棉区以巴楚县为核心的南疆等地区种植面积增长迅速;1990～2000年,变异的最大特点是新疆棉花生产的崛起和山东、河北棉花生产的萎缩。引起上述变化的原因是由于经济、政策、技术及自然以等因素发生变化的结果。     

云南弥渡县云景地区多元地学信息集成及找矿模型

云南弥渡县云景预查区位于巍山县扎村金矿东缘,属于西南三江成矿省昌都-普洱成矿带。本文结合前人地质资料以及野外地物化遥等多元勘查手段,对该预查区多元地学信息进行分析和集成。研究发现,该区成矿作用与区内浅层侵入岩关系密切,接触交代成矿作用明显,矿化受南北向构造控制,构造交汇部位矿化集中发育。斑岩体构成了区内主要的磁性源,含矿石英砂岩体具有接触过渡带高阻、高极化率的特征,中深部找矿潜力巨大;地球化学异常特征表现为热液叠加改造型金矿的元素组合特征,亲铜元素相对富集,成矿阶段呈多期次性,金成矿贯穿早期高温热液成矿阶段。通过多元地学信息集成提出了适合本区的热液叠加改造型金矿找矿模型。     

一种适用于高放废物地质处置数据管理的多源信息分类与编码体系

综合考虑高放废物地质处置多源信息的数据特点,按照学科专题领域划分原则,同时兼顾GIS等信息技术在新兴领域中的应用,形成了一套适用于高放废物地质处置数据管理的多源信息分类与编码体系。该体系遵循相关国际或国家基础信息标准及废物处置等行业标准,同时采用面向对象程序设计与兼顾GIS分析的思想,有利于更大程度地满足核技术领域信息共享需求。     

逆冲断层位移—长度关系解析 ——以杭锦旗断裂带为例

为了揭示鄂尔多斯盆地北部杭锦旗断裂带在晚石炭世—中三叠世逆冲断层生长的位移模式和位移—长度关系,本文通过地震剖面解释、地层回剥分析和断层古位移测算来厘定古断层的末端位置,明确断裂生长连接历史,并结合幂律关系,探究了断层生长模式以及断裂带岩性组合、运动学、反转和断层系统内在特征等方面的影响。研究表明,杭锦旗断裂带的构造演化受基底断裂的分段性制约。其北东走向的分段(泊尔江海子断裂东段)形成较早;在垂向上,断裂中部的位移大,向两端递减;在平面上,断裂末端与东西走向的分段(泊尔江海子断裂西段)叠覆,导致局部位移增大,最终发生硬连接。东西走向的三眼井断裂形成于晚石炭世,先后经历了断层分段、横向扩展和连接的演化阶段。乌兰吉林庙断裂作为调节带断裂,其活动相对较弱且局部发生反转。根据断层位移—长度剖面的几何形态和断层演化阶段分析,可将杭锦旗断裂带的逆冲阶段的位移模式分为4种类型:①近对称的三角状或椭圆状,代表独立断层;②左右极不对称的锯齿状或双峰状,代表断层之间发生软连接作用;③不规则波状,反映多条小型断层的连接作用;④异常尖峰状,代表大型断裂后期位移的调整。杭锦旗断裂带的D_(max)/L数据集与全球其他地区比较,要低一个数量级,可能与断裂带的后期反转有关。最后,针对杭锦旗断裂带在不同时期的构造演化和D_(max)/L变化特征,提出了断裂带逆冲阶段演化的路径模式。