基于IHS的多源遥感数据融合     

廖文峰 《地理空间信息》2012,(1):99-101,4

首先简要叙述了IHS法在遥感图像融合中的应用,然后对实验结果进行了分析,并用融合后的图像建立了土地利用类型的解译标志,以期为HIS法用于遥感图像融合提供参考。  相似文献   

现代遥感技术在土地执法监察工作中的应用     

孙洁芳  何芸  陈刚  孙伟 《地理空间信息》2012,10(4):100-101,104

描述了现代遥感技术在国土资源系统执法监察工作中的应用,对使用的工艺流程、技术路线进行了详细描述和分析。  相似文献   

遥感专业《数字图像处理》课程教学探讨   总被引：1，自引：1，他引：0  

刘春国  韩瑞梅  卢晓峰 《地理空间信息》2012,(3):180-182

《数字图像处理》是遥感科学与技术专业的一门专业必修课程。根据专业特性、课程体系和课程教学的要求,从课程教材和教学内容、方法和手段、实践教学等方面介绍了在遥感科学与技术专业开设《数字图像处理》课程的教学实践,并指出了进一步加强数字图像处理教学努力的方向。  相似文献   

汶川地震重灾区泥石流沟内崩滑物空间分布的RS-GIS定量方法   总被引：1，自引：0，他引：1  

张怀珍  范建容  胡凯衡  郭芬芬  刘飞  陈阳 《山地学报》2012,(1):78-86

汶川地震在山区引发大量崩塌、滑坡,形成大量的固体松散碎屑物质堆积在沟谷内(CLCAR,崩滑碎屑区),使得地震山区泥石流活动性增强。以岷江上游四川省汶川县银杏乡、映秀镇的15条泥石流沟的SPOT遥感影像为基础,利用GIS技术对CLCAR空间分布进行分析。建立CLCAR与流域高程、主沟侧距和沟口纵距的分布函数T(x)、M(x)和G(x),对CLCAR的空间分布特征进行描述;并计算其积分(DT、DM和DG)作为CLCAR空间分布特征的定量化参数。结果表明,函数T(x)、M(x)和G(x)能够较全面描述CLCAR的空间分布特征,DT、DM和DG能够作为CLCAR空间分布特征的定量化参数。泥石流沟谷内CLCAR的空间分布对泥石流的形成及规模具有一定的影响;在对灾区泥石流研究时有必要考虑泥石流沟内CLCAR空间分布特征。  相似文献   

胶州湾北部滨海湿地分布特征及质量评价     

王慧勇  史衍玺 《湿地科学与管理》2012,(4):40-42

以胶州湾北部滨海湿地为研究区域,运用RS和GIS技术提取湿地信息,研究时空变化特征,建立湿地定量评价系统,并对湿地质量进行分析。研究表明,自1997年到2007年,该地湿地类型变化较大,沿岸湿地退化现象严重,人为活动影响增大,非湿地面积大量增加,湿地质量不断下降。  相似文献   

Glaciofluvial erosional landforms in Åkvåg,Risør Municipality,Southern Norway     

《Norsk geografisk tidsskrift. Norwegian journal of geography》2012,66(2):117-122

  相似文献   

A synergic algorithm for retrieval of aerosol optical depth over land     

郭建平  薛勇  曹春香  张颢  光洁  张小曳  李小文 《大气科学进展》2009,26(5):973-983

In this paper, a novel algorithm for aerosol optical depth(AOD) retrieval with a 1 km spatial resolution over land is presented using the Advanced Along Track Scanning Radiometer (AATSR) dual-view capability at 0.55, 0.66 and 0.87 μm, in combination with the Bi-directional Reflectance Distribution Function (BRDF) model, a product of the Moderate Resolution Imaging Spectroradiometer (MODIS). The BRDF characteristics of the land surface, i.e. prior input parameters for this algorithm, are computed by extracti...  相似文献   

New magnetic field measurements of β Cephei stars and slowly pulsating B stars     

S. Hubrig  M. Briquet  P. De Cat  M. Schller  T. Morel  I. Ilyin 《Astronomische Nachrichten》2009,330(4):317-329

We present the results of the continuation of our magnetic survey with FORS 1 at the VLT of a sample of B‐type stars consisting of confirmed or candidate β Cephei stars and Slowly Pulsating B (hereafter SPB) stars, along with a small number of normal B‐type stars. A weak mean longitudinal magnetic field of the order of a few hundred Gauss was detected in three β Cephei stars and two stars suspected to be β Cephei stars, in five SPB stars and eight stars suspected to be SPB stars. Additionally, a longitudinal magnetic field at a level larger than 3σ has been diagnosed in two normal B‐type stars, the nitrogen‐rich early B‐type star HD 52089 and in the B5 IV star HD 153716. Roughly one third of β Cephei stars have detected magnetic fields: Out of 13 β Cephei stars studied to date with FORS 1, four stars possess weak magnetic fields, and out of the sample of six suspected β Cephei stars two show a weak magnetic field. The fraction of magnetic SPBs and candidate SPBs is found to be higher: Roughly half of the 34 SPB stars have been found to be magnetic and among the 16 candidate SPBs eight stars possess magnetic fields. In an attempt to understand why only a fraction of pulsating stars exhibit magnetic fields, we studied the position of magnetic and non‐magnetic pulsating stars in the H‐R diagram. We find that their domains in the H‐R diagram largely overlap, and no clear picture emerges as to the possible evolution of the magnetic field across the main sequence. It is possible that stronger fields tend to be found in stars with lower pulsating frequencies and smaller pulsating amplitudes. A somewhat similar trend is found if we consider a correlation between the field strength and the v sin i ‐values, i.e. stronger magnetic fields tend to be found in more slowly rotating stars (© 2009 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Saraswati Nadi in Haryana and its linkage with the Vedic Saraswati River — Integrated study based on satellite images and ground based information     

B. K. Bhadra  A. K. Gupta  J. R. Sharma 《Journal of the Geological Society of India》2009,73(2):273-288

Detailed studies on the status of Saraswati Nadi of northern Haryana have been carried out using multi date and multi resolution satellite images, GIS techniques and ground data. Palaeochannels have been delineated using remote sensing techniques and validated using discovered archaeological sites, sedimentological data from drilled wells and water quality data. Detailed analysis of hydrological data (rainfall and stream discharge), catchment area and petrographic analysis of rock samples have been done to decipher the dwindling state of Saraswati Nadi. Likelihood of Adi Badri as the place of origin of Saraswati Nadi and its possible linkage with the Vedic Saraswati River is discussed. Suggestions have been given for safeguarding and revival of Saraswati Nadi as a national heritage.  相似文献   

ASTER遥感数据解读与应用   总被引：19，自引：2，他引：19  

朱黎江  秦其明  陈思锦 《国土资源遥感》2003,14(2):59-63

ASTER遥感数据可以在地球表面自然过程与全球变化等多个研究领域得到广泛应用.本文首先对ASTER数据格式进行了分析,并对解读关键技术进行了研究,在此基础上,通过计算机编程实现了ASTER数据的读取;最后结合ASTER数据的特点给出了ASTER数据在几个主要研究领域的应用.  相似文献