Stellar Population Analysis of Galaxies based on Genetic Algorithms     

Abdel-Fattah Attia  H. A. Ismail  I. M. Selim  A. M. Osman  I. A. Isaa  M. A. Marie  A. A. Shaker 《中国天文和天体物理学报》2005,5(4):347-355

We present a new method for determining the age and relative contribution of different stellar populations in galaxies based on the genetic algorithm. We apply this method to the barred spiral galaxy NGC 3384, using CCD images in U, B, V, R and I bands. This analysis indicates that the galaxy NGC 3384 is mainly inhabited by old stellar population (age >109yr). Some problems were encountered when numerical simulations are used for determining the contribution of different stellar populations in the integrated color of a galaxy. The results show that the proposed genetic algorithm can search efficiently through the very large space of the possible ages.  相似文献   

星系NGC5018的星族合成研究     

孔旭  张文浩  李成  程福臻  A.Weiss 《天文学报》2002,43(3):264-271

利用星团谱样本的星族合成方法,研究了邻近巨椭圆星系NGC5018中的星族成分和其内部的恒星形成历史,给出了星系中不同年龄和金属丰度星族的成分占有比.星族合成结果表明,NGC5018中不仅存在大量金属丰度低的年老恒星成分,而且较年轻的星族成分(T=5×108yr)对星系光度贡献也很重要.星系吞并和相互作用过程可能是触发这些较年轻星族形成的物理原因,椭圆星系内部的恒星形成历史可能是2次爆发或者多次爆发过程.这些结果可以很好地解释NGC5018颜色偏蓝、Mg2谱指数强度偏弱等观测特征.  相似文献   

Propagation in 3D spiral-arm cosmic-ray source distribution models and secondary particle production using Picard     

《Astroparticle Physics》2015

We study the impact of possible spiral-arm distributions of Galactic cosmic-ray sources on the flux of various cosmic-ray nuclei throughout our Galaxy. We investigate model cosmic-ray spectra at the nominal position of the sun and at different positions within the Galaxy. The modelling is performed using the recently introduced numerical cosmic ray propagation code Picard. Assuming non-axisymmetric cosmic-ray source distributions yields new insights on the behaviour of primary versus secondary nuclei.We find that primary cosmic rays are more strongly confined to the vicinity of the sources, while the distribution of secondary cosmic rays is much more homogeneous compared to the primaries. This leads to stronger spatial variation in secondary to primary ratios when compared to axisymmetric source distribution models. A good fit to the cosmic-ray data at Earth can be accomplished in different spiral-arm models, although leading to decisively different spatial distributions of the cosmic-ray flux. These lead to different cosmic ray anisotropies, where even reproducing the data becomes possible. Consequently, we advocate directions to seek best fit propagation parameters that take into account the higher complexity introduced by the spiral-arm structure on the cosmic-ray distribution. We specifically investigate whether the flux at Earth is representative for a large fraction of the Galaxy. The variance among possible spiral-arm models allows us to quantify the spatial variation of the cosmic-ray flux within the Galaxy in presence of non-axisymmetric source distributions.  相似文献   

用传输矩阵方法研究多层介质增透膜的透射特性     

黎开洪  杨进 《成都信息工程学院学报》2006,21(Z1):104-110

利用麦克斯韦方程组和边界条件,推导出由高低折射率介质组成周期性的多层增透膜系的传输矩阵,用传输性矩阵求出增透膜系的反射率和透射率表示式,采用Maple语言和数值计算方法得到4层和8层高反射膜系的反射率随入射光波长变化曲线,分析和讨论入射光的入射角对反射率和透射率的影响.得到的结果有利于对多层介质增透膜系结构的理解,为光学仪器镀膜的设计提供了理论依据.  相似文献   

常顶瓦斯油吸附法脱除微量氯的实验研究     

李玉明  伦会荣 《山东国土资源》2006,(Z1)

炼油厂将常压塔顶油和减一线油作为重整原料,但由于氯含量过高(30×10-6)无法利用,传统方法是将其中的有机氯转化为无机氯化氢后脱除,但其对加氢催化剂有毒害,采用常顶瓦斯油吸附法可直接脱除微量氯。  相似文献   

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陈连旺  詹自敏 《大地测量与地球动力学》2011,31(6):1-5

?????????????????????????????????????ó???????????????????????仯??????1???????????仯????????????????NNW-SSE??????????3~9 kPa a^-1???????????仯???????????????NEE-SWW??????????1~6 kPa a^-1?????????????????????????????????????￡?2???????????仯????????????????NNW????????????????,??????????????????????????????????仯???????????????NEE????????λ?????????????????????仯????????????????????????????????????????????п????????Щ???????????????????3?????????????????????????????????з???????????-???ε???????????????????6 kPa a^-1?????-?????ε???????????????????5 kPa a^-1???????κ??????媲????ε????????????????????3~4 kPa a^-1??  相似文献   

水下溢油数值模拟研究   总被引：1，自引：0，他引：1  

陈海波  安伟  杨勇  尤云祥  雷方辉  赵宇鹏  李建伟 《海洋工程》2015,33(2):66-76

基于Lagrange积分法和Lagrange粒子追踪法建立了一个水下溢油数值模型。该溢油模型由两个子模型组成:羽流动力模型和对流扩散模型,其中羽流动力模型用以模拟溢油的喷发阶段和浮力羽流阶段;对流扩散模型用以模拟溢油的对流扩散阶段。通过数值实验,结合实验室水槽实验和水下溢油现场实验的观测资料进行模型验证。实验结果表明,模拟结果与观测资料一致性较好,从而验证了本文溢油模型的合理性和准确性;羽流动力模型为对流扩散模型提供源,海流、海水的垂向密度结构和油滴的直径分布是影响溢油在对流扩散阶段运动和分布的主要因素。  相似文献   

A LAYERED NUMERICAL MODEL FOR SIMULATING THE GENERATION AND PROPAGATION OF INTERNAL TIDES OVER CONTINENTAL SLOPE I. MODEL DESIGN     

中国海洋湖沼学报 《中国海洋湖沼学报》1999,17(2)

A layered three-dimensional nonlinear numerical model was constructed to simulate the generation and propagation of internal tides over the continental slope. The simulation was split into external mode computation (EMC) and internal mode computation (IMC) to minimize the computational load. IMC was carried out once after EMC was implemented N times. As to EMC, a semi-implicit numerical scheme was applied in such a way that the pressure gradient terms and the velocity divergence terms were discretized semi-implicitly, but the other terms were discretized explicitly. Eulerian-Lagrangian explicit discretization was applied to the convective terms simultaneously. As a result, the stability of EMC did not depend on the wave celerity and time step was not limited by the CFL condition. More than that, use of the conjugate gradient accelerated Jacobi method further improved the computational efficiency of the model.  相似文献   

非球形轴对称粒子光散射的散射矩阵元素展开系数的数值计算     

丁继烈  许丽生 《成都信息工程学院学报》1999,(3)

扼要地介绍了非球形粒子光散射的散射矩阵元素按广义球函数展开的基本理论，以及球形粒子散射矩阵元素间的关系。在此基础上较详细地阐述了计算展开系数的方法以及在程序研制中所遇到的一些问题。最后，对非球形的Ｃｈｅｂｙｓｈｅｖ粒子光散射的散射矩阵元素的展开系数进行了计算，结果表明数值技术和计算的正确性。  相似文献   

Reply to the discussion by Conti R., De Sanctis L. and Viggiani G.M.B. on ‘Influence of diaphragm wall installation on the numerical analysis of deep excavation’ by Burlon S., Mroueh H. & Shahrour I.     

S. Burlon  H. Mroueh  I. Shahrour 《国际地质力学数值与分析法杂志》2013,37(11):1688-1690

The authors thank the discussers R.Conti, L.De Sanctis and G.M.B.Viggiani for their interest to the paper entitled ‘Influence of diaphragm wall installation on the numerical analysis of deep excavation’ and for providing the opportunity to submit additional information to clarify some issues. The authors broadly agree with the comments which deal with three main aspects of the paper: presence of water and type of analysis, constitutive modelling and numerical strategies. The present reply addresses some additional issues that the discussers find not clear on the original paper submitted by the writers. Copyright © 2013 John Wiley & Sons, Ltd.  相似文献