两种四维奇异值分解同化方法的比较及误差分析   总被引：1，自引：1，他引：0  

王金成  李建平  丑纪范 《大气科学》2008,32(2)

4DSVD是最近提出的一种新的资料同化方法。目前还存在一些需要解决的问题,比如如何选取样本,如何得到支撑大气吸引子的基向量以及选取基向量的个数问题等等。作者利用奇异值分解(SVD)与经验正交函数分解(EOF)两种方法来获得支撑大气吸引子的基向量,推导了基于这两种方法的4DSVD分析场的理论公式,并用简单的数值试验比较了基于这两种方法的4DSVD分析场的空间相关系数和误差,初步分析了分析场与基向量个数的关系以及与样本选取的关系和分析误差的来源及各种误差对分析误差影响的相对大小。结果表明,用SVD方法作为获得支撑大气吸引子基向量的方法得到的分析场较EOF方法稳定,分析场与基向量个数有密切关系,观测误差、模式误差和观测代表性误差是分析误差的主要来源,且其引起的分析误差随着基向量个数增多而增大。  相似文献   

三种气象绘图软件及自动化制图比较分析     

马占良 《青海气象》2008,(Z1)

1引言在气象数据处理和应用分析中,经常需要绘制大量气象要素图形。由于计算机性能的日益提高,目前已有多种计算机绘图软件系统成为科研人员工作中不可缺少的工具,并且广泛用于各类气象业务科研及分析处理领域。面对大量的数据,如果每  相似文献   

甘肃金川矿区地表三维形变InSAR监测     

杨旺  何毅  张立峰  王文辉  陈有东  陈毅 《国土资源遥感》2022,(1):177-188

金川矿区是我国最大的镍矿生产基地,2018年提出复采计划以来,对该矿区地表形变的监测还是空白.该文基于3个轨道(升轨128、降轨33和135)的Sentinel-1A数据,利用小基线集雷达干涉(small baseline subset In-SAR,SBAS-InSAR)和结合先验条件的最小二乘迭代法获得金川矿区20...  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   

河北冬奥赛区一次夜间增温过程的数值模拟及诊断     

章鸣  连志鸾  平凡  祝善友 《大气科学》2022,46(1):168-180

夜间增温是河北冬奥赛区冬季频发的天气现象,对其进行准确的模拟与预报对赛区建设及比赛保障至关重要.本文针对河北冬奥赛区2020年2月8日夜间至9日凌晨发生的一次夜间增温过程,通过引入高分辨率地形数据,利用中尺度区域数值模式WRF4.1.5精细化再现了此次夜间增温过程,并探究了此次过程的气象特征及成因.研究结果表明:此次夜...  相似文献