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991.
利用2004—2008年5—9月大连新一代天气雷达和自动站资料,在进行回波分型、多次采用最优化Z I关系,结合系统误差消除的技术方法,得到适用于实际业务需要的整体本地化Z I关系。以大连地区2008年全部5次大暴雨过程为例,经RPG数据处理系统中的降水估计产品检验,较沿用 WSR 88D 默认值生成值准确率提高40%以上,经2009—2011年使用,估算准确率稳定在75%以上,提高了天气雷达数据处理的质量。  相似文献   
992.
Although Type Ia supernovae(SNe Ia) play an important role in the study of cosmology, their progenitors are still poorly understood. Thermonuclear explosions from the helium double-detonation sub-Chandrasekhar mass model have been considered as an alternative method for producing SNe Ia. By adopting the assumption that a double detonation occurs when a He layer with a critical ignition mass accumulates on the surface of a carbon–oxygen white dwarf(CO WD), we perform detailed binary evolution calculations for the He double-detonation model, in which a He layer from a He star accumulates on a CO WD. According to these calculations, we obtain the initial parameter spaces for SNe Ia in the orbital period and secondary mass plane for various initial WD masses. We implement these results into a detailed binary population synthesis approach to calculate SN Ia birthrates and delay times. From this model,the SN Ia birthrate in our Galaxy is ~0.4- 1.6 × 10-3yr-1. This indicates that the double-detonation model only produces part of the SNe Ia. The delay times from this model are ~ 70- 710 Myr, which contribute to the young population of SNe Ia in the observations. We found that the CO WD + sdB star system CD-30 11223 could produce an SN Ia via the double-detonation model in its future evolution.  相似文献   
993.
The Extreme Ultraviolet Camera(EUVC) onboard the Chang'e-3(CE-3)lander is used to observe the structure and dynamics of Earth's plasmasphere from the Moon. By detecting the resonance line emission of helium ions(He+) at 30.4 nm, the EUVC images the entire plasmasphere with a time resolution of 10 min and a spatial resolution of about 0.1 Earth radius(RE) in a single frame. We first present details about the data processing from EUVC and the data acquisition in the commissioning phase, and then report some initial results, which reflect the basic features of the plasmasphere well. The photon count and emission intensity of EUVC are consistent with previous observations and models, which indicate that the EUVC works normally and can provide high quality data for future studies.  相似文献   
994.
CIRCULAR-ECONOMY MODELS OF ANIMAL HUSBANDRY INDUSTRY IN JILIN PROVINCE   总被引:1,自引:1,他引:0  
1INTRODUCTION The circular-economyisan efficient resources metabolic process, based on principles of ecology and system engi- neering.Withcoupledstructure andthe complex ecolo- gical and economic evolution, it has the characteristics of overall integrity, coordination, and circulation (WANG, 2005). Compared with the traditionalecono- mic model, the circular-economy requires the technical model of production process to be changed from the opening flow pattern that is "resourcesconsumption…  相似文献   
995.
基于CC的防火墙安全功能分析   总被引:1,自引:0,他引:1  
防火墙是网络安全的核心手段。依据基于CC(Common Criteria)制订的国家标准——包过滤防火墙安全技术要求和应用级防火墙安全技术要求,提出每项安全功能要求对应的实际安全措施,并分析当前防火墙未实现的安全功能要求。  相似文献   
996.
We have collected nearly all the available observed data of the elements from Ba to Dy in halo and disk stars in the metallicity range -4.0 <[Fe/H]< 0.5. Based on the observed data of Ba and Eu, we evaluated the least-squares regressions of [Ba/Fe] on [Fe/H], and [Eu/H] on [Ba/H]. Assuming that the heavy elements (heavier than Ba) are produced by a combination of the main components of s- and r-processes in metal-poor stars, and choosing Ba and Eu as respective representative elements of the main s- and the main r-processes, a statistical model for predicting the Galactic chemical evolution of the heavy elements is presented. With this model, we calculate the mean abundance trends of the heavy elements La, Ce, Pr, Nd, Sm, and Dy with the metallicity. We compare our results with the observed data at various metallicities, showing that the predicted trends are in good agreement with the observed trends, at least for the metallicity range [Fe/H]> -2.5. Finally, we discuss our results and deduce some importa  相似文献   
997.
介绍了稀疏矩阵的四种常见形式以及稀疏矩阵技术在天测与测地VLBI数据处理中的应用。推演了天测与测地VLBI数据综合解算中所用稀疏矩阵形式下待估参数求解和协方差矩阵估算的算法。通过对是否采用稀疏矩阵技术时方程求解 (乘法和加法 )运算对数的估算和比较 ,表明普通最小二乘方法的运算对数约为参数总数的 3次方 ,而采用稀疏矩阵技术时的运算对数近似与参数总数成线性关系 ,从而能够在现代空间对地观测技术的大样本数据处理中显著缩短计算时间。  相似文献   
998.
999.
仲佳勇  张杰  赵刚  鲁欣 《天文学报》2004,45(1):16-24
利用原子数据模拟程序RCN/RCG、AUTOSTRUCTURE(AS)、GRASP分别对类氖铁的离子结构进行计算,计算过程包含了对波函数的相对论修正,计算结果包括电偶级光谱跃迁的能级间隔,谐振子强度,跃迁几率,并与实验值进行了比较,分析了3种原子数据模拟程序在计算原子结构上的精确度.  相似文献   
1000.
A 3-D coupled ice sheet model, GLIMMER model is introduced, and an idealized ice sheet experiment under the EISMINT-1 criterion of moving boundary condition is presented. The results of the experiment reveal that for a steady-state ice sheet profile the characteristic curves describe the process of evolution which are accordant with theoretical estimates. By solving the coupled thermodynamics equations of ice sheet, one may find the characteristic curves which derived from the conservation of the mass, energy and momentum to the ice flow profile. At the same time, an agreement, approximate to the GLIMMER case and the confirmed theoretical results, is found. Present study is explorihg work to introduce and discuss the handicaps of EISMINT criterion and GLIMMER, and prospect a few directions of the GLIMMER model.  相似文献   
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