三维城市地表反射率计算模式   总被引：1，自引：1，他引：0  

王建凯  王开存  王普才 《大气科学》2008,32(5):1119-1127

地表反射率是控制地表能量平衡的一个重要参数。城市建筑物的分布具有较大的不均一性,这不仅给地基观测城市地表反射率带来了很大困难,数值模拟城市地表反射率也是非常困难的。作者开发了一个三维城市地表反射率模式city_photo,该方法结合了蒙特卡洛方法和几何光学方法的优点,具有较高的精度和较快的计算速度。通过引入城市地图的概念,该模式能够计算具有不同结构的城市的地表反射率。2002至2004年晴空MODIS（MODerate Resolution Imaging Spectroradiometer,中分辨率成像光谱辐射计）1~7通道可见光和近红外通道地表反射率资料被用来检验模式的有效性,位于北京朝阳区的中国科学院大气物理研究所的AERONET站点观测得到气溶胶光学特性和水汽资料,6S（Second Simulation of Satellite Signal in the Solar Spectrum）大气辐射传输模式被用来对其进行大气订正。模式计算的北京城市地表反射率个例与MODIS 7个通道地表反射率观测结果具有很高的相关性,相关系数在0.80~0.93之间,说明模式能够较好地模拟城市地表反射率随太阳和观测角度的变化情况。最后讨论了城市结构对城市地表反射率的影响。  相似文献   

基于机载多光谱遥感数据的溢油信息提取方法     

刘丙新  李颖  高超 《国土资源遥感》2014,(1)

为研究应用紫外-可见光-近红外-热红外遥感数据识别海上溢油的方法,利用机载多光谱溢油监测设备获取了舟山海域多光谱遥感数据,并利用野外地物光谱仪获取了水体和油膜的反射光谱。通过提取并分析机载多光谱遥感图像上多目标的影像特征和光谱响应特征,利用决策树分类法对海上油膜相对厚度的分布进行分类和制图。研究表明,基于机载多光谱遥感数据的溢油信息提取方法总体分类精度达93.7%,能够准确区分薄油膜和厚油膜,可有效提取海洋溢油污染信息,完全能够满足海洋溢油污染遥感监测需求。  相似文献   

Old stellar population synthesis： new age and mass estimates for Mayall Ⅱ = G1     

Jun Ma  ;Richard de Grijs  ;Zhou Fan  ;Soo-Chang Rey  ;Zhen-Yu Wu  ;Xu Zhou  ;Jiang-Hua Wu  ;Zhao-Ji Jiang  ;Jian-Sheng Chen  ;Kyungsook Lee  ;Sangmo Tony Sohn 《天体物理学报》2009,(6):641-652

Mayall Ⅱ = G1 is one of the most luminous globular clusters （GCs） in M31. Here, we determine its age and mass by comparing multicolor photometry with theoretical stellar population synthesis models. Based on far- and near-ultraviolet GALEX photometry, broad-band UBVRI, and infrared JHKs 2MASS data, we construct the most extensive spectral energy distribution of G 1 to date, spanning the wavelength range from 1538 to 20 000A. A quantitative comparison with a variety of simple stellar population （SSP） models yields a mean age which is consistent with G1 being among the oldest building blocks of M31 and having formed within ～1.7 Gyr after the Big Bang. Irrespective of the SSP model or stellar initial mass function adopted, the resulting mass estimates （of order 10^7M⊙） indicate that GI is one of the most massive GCs in the Local Group. However, we speculate that the cluster＇s exceptionally high mass suggests that it may not be a genuine GC. Our results also suggest that G1 may contain, on average, （1.65±0.63） × 10^2L⊙ far-ultraviolet-bright, hot, extreme horizontal-branch stars, depending on the adopted SSP model. In addition, we demonstrate that extensive multi-passband photometry coupled with SSP analysis enables one to obtain age estimates for old SSPs that have similar accuracies as those from integrated spectroscopy or resolved stellar photometry, provided that some of the free parameters can be constrained independently.  相似文献   

An infrared study of Be stars based on ISO SWS01 spectra     

Pin Zhang Zai-Qi Fu 《天体物理学报》2009,(7):770-776

The Infrared Space Observatory （ISO） Short-Wavelength Spectrometer （SWS） spectra of 10 Be stars are presented. It can be seen that the Be stars show a diversity in their ISO SWS01 spectral classifications by Kraemer et al., from naked stars, stars associated with dust, stars with warm dust shells, stars with cool dust shells to very red sources. In addition, the Brα/HI（14-6） line flux ratio derived for the sample stars is compared with that of P Cyg, and it is found that the line ratio of Be stars which were investigated show not only lower values as suggested by Waters et al., but also larger values. Therefore, the line ratio cannot be used to judge whether a star is a Be star or not.  相似文献   

一次朝圣的旅途——参观LAMOST望远镜     

邹季强 《天文爱好者》2009,(1):89-89

首次获悉我国正在筹建全球最大的大视场光纤光谱望远镜（LAMOST）已是几年前的事情了,这一在世界上领先的项目立即引起了我的关注。随后,通过网络、《天文爱好者》杂志等渠道,逐步加深了对它的了解。这一次,我非常荣幸地参加了由“北京市青少年科技俱乐部”组织的参观LAMOST望远镜的活动,得以第一时间目睹它的风采。  相似文献   

High resolution spectroscopy of two young active late type stars within 20 parsecs of the Sun     

Hui-Juan Wang Jian-Yan Wei 《中国天文和天体物理学报》2009,9(3)

We present high-resolution optical echell spectroscopy of HIP 544 and HIP 46843, two nearby solar like stars. The discovery of these young stars at such a close distance to the Sun is really a surprising phenomenon. It will help us to have a better understanding of the structure and evolutionary history of the Milky Way. The radial ve-locities (RV) of HIP 544 and HIP 46843 are measured to be -6.88±0.13km s-1 and 8.30±0.16km s-1, respectively, which are more accurate than before. The equivalent widths (EW) of the Li I 6707.8 A absorption line of HIP 544 and HIP 46843 are mea-sured to be 110±5mA and 195±5mA respectively. Based on these properties, HIP 544 is estimated to be 100-800Myr old and HIP 46843 30-100Myr old using three relatively creditable methods.  相似文献   

An unusual timing and spectral state of a black hole microquasar XTE J1550-564     

Ying-Kang Jin Shuang-Nan Zhang Ti-Pei Li 《中国天文和天体物理学报》2009,9(2)

An unusual timing and spectral state of a black hole microquasar XTE J1550-564 observed with RXTE is analyzed. Millisecond variabilities are found, which are significantly shorter than the minimum possible time scale in the light curves of black hole binaries, as suggested by Sunyaev & Revnivtsev (2000). The X-ray spectral fitting result indicates that there is an unusual soft component in the spectrum, which may be responsible for the millisecond variabilities. The millisecond variabilities as well as the unusual soft spectral component should be produced from some small, but independent active regions in the accretion disk.  相似文献   

浙东南石平川花岗岩体LA ICP MS锆石U Pb年代学及构造意义   总被引：8，自引：0，他引：8  

李艳军  魏俊浩  姚春亮  鄢云飞  谭俊  付乐兵  潘锦勃  李伟 《地质论评》2009,55(5):673-684

石平川钾长花岗岩体位于浙江沿海火山岩带的中南部,LA-ICPMS锆石UPb定年结果为102.5±1.2 Ma（MSDW=2.1）,形成于早白垩世末期。岩相学及化学成分显示其属高钾钙碱性岩系,具有高硅富钾和铝低铁、镁、磷和钛特征,SiO2含量为74.79%～77.79%,K2O为4.26%～7.97%,铝指数A/CNK=0.98～1.10,属准铝质—弱过铝质岩石。富集Rb、Th、U和K,亏损Sr、Ba、Nb、P和Ti,REE具有中等负Eu异常（Eu/Eu*=0.33～0.50）,总体呈现LREE富集的右倾“V”型配分模式。岩石\[n（87Sr）/n（86Sr）\]i值为0.70801～0.71012（t=102.5Ma）,εNd（t）值为-8.63～-8.76,显示壳—幔混合成因特征。矿物组成及地球化学特征显示石平川岩体为高演化I型花岗岩。微量元素显示石平川岩体具有后碰撞花岗岩的特征,侵位于早白垩世末期的张性构造环境,其形成可能与印度板块北向漂移所导致的古太平洋板块碰撞弧后引张构造有关。  相似文献   

作物病虫害高光谱遥感进展与展望   总被引：2，自引：0，他引：2  

张凝  杨贵军  赵春江  张竞成  杨小冬  潘瑜春  黄文江  徐波  李明  朱西存  李振海 《遥感学报》2021,25(1):403-422

作物病虫害作为影响农作物品质、产量及威胁粮食安全的主要因素,仅依靠人工田间调查对其进行监测已不能满足当下农业生产精准高效的需求。高光谱遥感作为能够获取地表物体连续波谱信息的遥感技术,已经成为当下作物病虫害监测识别的重要手段。本文对作物病虫害高光谱遥感监测识别的研究进展进行综述,通过对该领域发表文献的统计以及对主要机构、团队、数据源的分析,明确了病虫害高光谱遥感监测的研究热点和趋势;在此基础上,分析高光谱技术及其作物病虫害的监测识别机理,从病虫害胁迫探测、分类识别、危害严重度定量分析及早期检测四个方面综述相关技术及研究现状;通过探讨当下高光谱遥感病虫害监测识别面临的挑战,提出作物病虫害标准图谱库的建立、星载高光谱传感器的完善以及星空地一体化监测平台的搭建是当前作物病虫害高光谱遥感监测识别技 术落到实处的关键,也是未来发展的重点方向。  相似文献   

基于多源测高卫星的日本海域平均海面高模型建立     

刘杨  宋丽洁  王新建 《北京测绘》2021,35(4):534-538

平均海面模型是研究海图基准及海平面化的重要参考.经过数据预处理、重复周期观测数据共线平差、非重复周期观测数据海面时变校正、多种卫星测高数据联合交叉点平差、海面高格网化等几个环节,利用1993—2012年近20年的测高数据,建立日本海域(30° ～45°N、130° ～145°E)2′ ×2′网格分辨率的平均海平面模型(Japan Mean Sea Surface,JPMSS),与WHU2013、CLS15、DTU18三种全球平均海面高模型以及TP(Topex/Poseidon)/J1(Jason-1)/J2(Jason-2)平均参考框架,进行比较分析,结果显示,在研究区域内,JPMSS相比于其他模型误差最小,精度较为可靠.  相似文献