解析法测定天文方位角计算软件     

程朋根  李金平 《测绘工程》1996,5(4):44-50

介绍北极星时角法测定天文方位角的基本方法，进而说明解析法测定天文方位角的基本原理，阐述计算软件的功能、菜单设计特点和操作方法，以实例说明软件的实用性。  相似文献   

ERROR COMPARISON OF WIND FIELD RETRIEVAL FROM SINGLE AND DUAL-DOPPLER RADAR OBSERVATIONS          下载免费PDF全文

Tao Zuyu 《Acta Meteorologica Sinica》1994,8(3):337-345

The error distributions of the wind fields retrieved from single and dual-Doppler radar observations are given inthis paper.The results indicate that the error of dual-Doppler retrieval depends on the position in the scan region of thedual-Doppler radar.The error of single-Doppler retrieval by using velocity azimuth processing(VAP)technique de-pends on the angle between the directions of wind and the radar beam.Generally,the winds retrieved from single Doppl-er radar are close to those retrieved from dual-Doppler radar.But,the error distribution of the single-Doppler retrievalis different from the dual-Doppler retrieval.We simulate the retrievals of single Doppler observation by the use of theoutput wind data from a 3-D numerical model of severe convection.The comparison of the simulated single-anddual-Doppler retrievals shows that the VAP may be a suitable technique for the operational analysis of mesoscale windfields.It can also be used as a supplement to wind field retrieval in the field experiment.  相似文献   

Estimation of azimuth and slowness of tele-seismic signals recorded by a local seismic network     

靳平  潘常周 《地震学报(英文版)》2002,15(6):646-655

Introduction The azimuth and slowness are two major features of seismic signals. The accurate estimation of them is quite important for both phase identification and event location. Generally, there are two types of seismic stations, i.e. 3-component stations (3C) and arrays. To estimate the two direc-tional parameters, the polarization analysis (Jurkevics, 1988) is commonly used for 3C stations and the frequency-wavenumber spectrum analysis ( f-k) (Capon, 1969; Kvaerna, Doornbos, 1986) is …  相似文献   

由地方台网记录确定远震信号的方位角和慢度          下载免费PDF全文

靳平  潘常洲 《地震学报》2002,24(6):617-626

介绍一种新的适合于地方遥测台网数据处理的方法，估算远震信号到达台站的方位角和慢度．该方法是根据信号在各台站上的到时与台站位置矢量在信号传播方向上的投影之间的相关性的原理．实际分析结果表明，应用该方法对地方台网的记录进行处理时可以准确地计算出信号的方位角和慢度，并能准确快捷地对地方台网记录的远震信号进行解释．   相似文献   

GPS短边方位测量若干问题的探讨     

熊建明  王宇飞 《四川测绘》2002,25(3):115-118

本文对GPS短边方位测量中遇到的问题进行了探讨，如仪器的检验，数据剔除率，检核测量误差的方法和方位平差及精度估计等。通过分析推导得出GPS方位边的平差公式和精度估计公式。  相似文献   

区域航空γ能谱场地球化学解释及预测方法的探讨     

孙念义 《铀矿地质》1987,(5)

本文以“铀矿区域评价准则”为依据,试用因子分析主成分比值法,铀对钍(钾)的区域相对场法和铀成矿有利指数法,对我国YW-10和YW-10B两个测区的区域航空γ能谱场进行了地球化学解释及预测方法的研究,与已知矿区660测区从宏观上做了对比分析,并研究了γ能谱参数在走向长270km,宽50—70km空间上的分布变化规律。研究结果表明,这些方法对了解成岩时原始铀的分布及后期铀的地球化学活动规律,估计成岩、成矿阶段铀源岩可能提供的生铀量,识别铀成矿有利地区是有用的。  相似文献   

云南漾濞县6.4级地震前地电场异常回溯性分析          下载免费PDF全文

侯泽宇  安张辉  范莹莹  付阿龙  谭大诚  卫雷 《地震工程学报》2021,43(4):807-817

针对2021年5月21日云南漾濞M_S6.4地震,采用滑动相关性方法和地电场优势方位角方法,开展震中周围200 km范围内地电场台站地震异常的统计特征分析和优势方位角的回溯性研究,发现:(1)通过对漾濞M_S6.4震中周围历史地震事件的统计分析,认为该区域地电场地震异常现象通常在震前约20(±5)天开始出现,如弥渡、祥云和洱源台;(2)漾濞M_S6.4地震前,洱源和祥云台地电场优势方位角在震前约15天或更早时间开始出现异常变化现象;(3)当地电场台站与地震事件处于同一发震断层(或断裂带)时,其观测到地震异常的可能性更大。此外,结合研究区域已有大地电磁测深结果,对地震反映敏感的地电场台站测区下方电性结构特征进行了初步探索,认为当测区位于电阻率边界上时,更易观测到地震地电场异常变化现象,相关研究结论将有望为地电场台站的选址建设、地震异常分析等工作提供技术支撑。  相似文献   

地形抹平与半经验模型的Landsat TM/ETM+地形校正方法     

姜亢  胡昌苗  于凯  赵永超 《遥感学报》2014,18(2):287-306

地形校正可以减小地形起伏对地物光谱的影响,提高计算机分类在山区的精度。设计了针对全球土地覆盖分类的Landsat TM/ETM+数据地形校正方法 SCOS(Smoothed COS余弦),首先对地形的坡度角进行抹平处理,很大程度上削弱了地表非朗伯性对地形校正的影响,然后利用简单有效的余弦校正去除地形效应。该方法与其他常用地形校正算法的对比分析是通过对全球不同区域、不同地表覆盖的有代表性的6景Landsat TM/ETM+数据的试验,采用统计分析与目视判读的方式,从过度校正和类内均一性两个方面进行的。结果表明,该方法在目视效果和统计结果上优于常规方法,并且更加简单有效,无需复杂的大气参数及传感器参数,满足全球地表覆盖分类对地形校正的需求。  相似文献   

Searches for very high energy gamma rays from blazars with CANGAROO-III telescope in 2005-2009     

Y. Mizumura  J. Kushida  K. Nishijima  G.V. BicknellR.W. Clay  P.G. EdwardsS. Gunji  S. HaraS. Hayashi  S. KabukiF. Kajino  A. KawachiT. Kifune  R. KiuchiK. Kodani  Y. MatsubaraT. Mizukami  Y. MizumotoM. Mori  H. MuraishiT. Naito  M. OhishiV. Stamatescu  D.L. SwabyT. Tanimori  G. ThorntonF. Tokanai  T. ToyamaS. Yanagita  T. YoshidaT. Yoshikoshi 《Astroparticle Physics》2012,35(9):563-572

We have searched for very high energy (VHE) gamma rays from four blazars using the CANGAROO-III imaging atmospheric Cherenkov telescope. We report the results of the observations of H 2356-309, PKS 2155-304, PKS 0537-441, and 3C 279, performed from 2005 to 2009, applying a new analysis to suppress the effects of the position dependence of Cherenkov images in the field of view. No significant VHE gamma ray emission was detected from any of the four blazars. The GeV gamma-ray spectra of these objects were obtained by analyzing Fermi/LAT archival data. Wide range (radio to VHE gamma-ray bands) spectral energy distributions (SEDs) including CANGAROO-III upper limits, GeV gamma-ray spectra, and archival data, even though they are non-simultaneous, are discussed using a one-zone synchrotron self-Compton (SSC) model in combination with a external Compton (EC) radiation. The HBLs (H 2356-309 and PKS 2155-304) can be explained by a simple SSC model, and PKS 0537-441 and 3C 279 are well modeled by a combination of SSC and EC model. We find a consistency with the blazar sequence in terms of strength of magnetic field and component size.  相似文献   

Jitter radiation images, spectra and light curves from a relativistic spherical blastwave     

Brian J. Morsony  Jared C. Workman  Davide Lazzati  Mikhail V. Medvedev 《Monthly notices of the Royal Astronomical Society》2009,392(4):1397-1402

We consider radiation emitted by the jitter mechanism in a Blandford–McKee self-similar blastwave. We assume the magnetic field configuration throughout the whole blastwave meets the condition for the emission of jitter radiation and we compute the ensuing images, light curves and spectra. The calculations are performed for both a uniform and a wind environment. We compare our jitter results to synchrotron results. We show that jitter radiation produces slightly different spectra than synchrotron, in particular between the self-absorption and the peak frequency, where the jitter spectrum is flat, while the synchrotron spectrum grows as  ν^1/3  . The spectral difference is reflected in the early decay slope of the light curves. We conclude that jitter and synchrotron afterglows can be distinguished from each other with good quality observations. However, it is unlikely that the difference can explain the peculiar behaviour of several recent observations, such as flat X-ray slopes and uncorrelated optical and X-ray behaviour.  相似文献