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991.
992.
风暴的自动识别,跟踪与预报 总被引:17,自引:2,他引:15
利用多普勒雷达体扫描资料对风暴进行实时地自动识别、跟踪、结构分析和临近预报,风暴的识别基于其个连续区域的体积和雷达反射率大于给定的体积阈值和反射率阈值;用矩心跟踪法匹配相邻两时刻的风暴,对风暴的合并与分裂进行了处理;根据风暴在过去各个时刻的中心位置和体积,利用最小二乘法进行线性外推来预报其在下一时刻的位置和面积。结果表明本方法能较好地识别、跟踪和警戒强对流性天气。 相似文献
993.
Estimation of Cloud Motion Using Cross-Correlation 总被引:6,自引:0,他引:6
Li Zhenjun 《大气科学进展》1998,15(2):277-282
EstimationofCloudMotionUsingCros-CorelationLiZhenjun(李振军)AirForceCenterofMeteorology,Beijing100843ReceivedAugust25,1997;revis... 相似文献
994.
A probabilistic approach to structural model updating 总被引:3,自引:0,他引:3
Lambros S. Katafygiotis Costas Papadimitriou Heung-Fai Lam 《Soil Dynamics and Earthquake Engineering》1998,17(7-8):495-507
The problem of updating a structural model and its associated uncertainties by utilizing measured dynamic response data is addressed. A Bayesian probabilistic formulation is followed to obtain the posterior probability density function (PDF) of the uncertain model parameters for given measured data. The present paper discusses the issue of identifiability of the model parameters and reviews existing asymptotic approximations for identifiable cases. The focus of the paper is on the treatment of the general unidentifiable case where the earlier approximations are not applicable. In this case the posterior PDF of the parameters is found to be concentrated in the neighborhood of an extended and extremely complex manifold in the parameter space. The computational difficulties associated with calculating the posterior PDF in such cases are discussed and an algorithm for an efficient approximate representation of the above manifold and the posterior PDF is presented. Numerical examples involving noisy data are presented to demonstrate the concepts and the proposed method. 相似文献
995.
996.
应用模糊评判法预测新疆东准噶尔地区金成矿有利区 总被引:1,自引:0,他引:1
应用模糊综合评判原理,在对新疆东准噶尔地区金成矿地质基本特征分析基础上,选取地质、地球化学参数,利用各参数的权重分配进行调整,确定最佳权重分配方案,对新疆东准噶尔地区金的含矿性进行综合评判,其结果预测了该地区金矿成矿有利区。 相似文献
997.
998.
We present an investigation of rotation–activity correlations using International Ultraviolet Explorer ( IUE ) SWP measurements of the C iv emission line at 1550Å for 72 active binary systems. We use a standard stellar evolution code to derive non-empirical Rossby numbers, R 0 , for each star in our sample and compare the resulting C iv rotation–activity correlation to that found for empirically derived values of the Rossby number and that based on rotation alone. For dwarf stars our values of R 0 do not differ greatly from empirical ones and we find a corresponding lack of improvement in correlation. Only a marginal improvement in correlation is found for evolved components in our sample. We discuss possible additional factors, other than rotation or convection, that may influence the activity levels in active binaries. Our observational data imply, in contrast to the theoretical predictions of convective motions, that activity is only weakly related to mass in evolved stars. We conclude that current dynamo theory is limited in its application to the study of active stars because of the uncertainty in the angular velocity-depth profile in stellar interiors and the unknown effects of binarity and surface gravity. 相似文献
999.
Randomly amplified polymorphic DNA (RAPD) technique was applied to assess the genetic variations and phylogenetic relationships
in 4 species ofPorphyra. The samples were collected from the coast of Canada, Vietnam, Zhoushan, Fujian and Qingdao in China. Amplifications with
20 primers were carried out under predetermined optimal reaction conditions (samples were first heated at 94°C for 5 min.
and followed by 45 cycles of 1 min at 94°C, 1 min at 36°C, and 2 min at 72°C, then held at 72°C for 10 min). The amplified
products were scored as present (1) or absent (0) for each DNA sample and an index of genetic similarity (F) was calculated
by using Nei & Li’s matching coefficient method (1979). The value of (1−F) was used to quantify the genetic distances between
species and construct a phylogenetic tree. The relationship indicated by the UPGMA and NJ cluster analysis on the values of
the genetic distance is in good overall agreement with classical taxonomy. The obvious differences between natural and cultivated
population ofP. haitanensi suggest that variation or hybridization with other species occurred during the culture.
Contribution No. 100 from the Experimental Marine Biology Laboratory, IOCAS.
Contribution No. 3289 from the Institute of Oceanology, Chinese Academy of Sciences.
The research supported by the Foundation of the Chinese Academy of Sciences. 相似文献
1000.