磁空间群PC 63/mmc的C-G系数计算

在晶体拉曼散射的张量计算中，晶体磁空间群的C-G系数具有重要的作用。利用本征函数法计算了Pc63／mmc磁空间群第一布里渊区中的对称点A之间的C-G系数。     

企业集团系统模式研究

采用系统理论和系统分析的方法,对企业集团系统的基本概念、基本特征和基本类型进行了系统综述与分析。     

Dark matter in very poor galaxy groups

We have analyzed a sample of 7000 galaxies in the Local Supercluster (LS) (V < 3100 km/s) selected from the LEDA database [Makarov, D.I., Karachentsev, I.D. A new catalogue of multiple galaxies in the local supercluster small galaxy groups. Small Galaxy Groups ASP Confer. Ser. 209, 40–46, 2000]. We have derived physical properties of poor LS groups selected by dynamical and 3D-Voronoi tessellation methods. Median values of mass-to-luminosity ratios for poor LS groups selected by these methods are 50 M_⊙/L_⊙ and 34 M_⊙/L_⊙, respectively. Physical parameters of LS galaxy triplets in comparison with other samples were evaluated. We suggest that the Dressler effect is present even in such poor groups as galaxy triplets. The data suggest that dark matter haloes are associated with the individual galaxies for LS triplets, which we find are dynamically younger systems. This contrasts with the properties of the Interacting and Northern & Southern triplet samples. For these two samples, the data suggest that the dark matter resides in a common halo. The median values of the mass-to-luminosity ratios for LS triplets, Northern & Southern triplets, and Interacting triplets are 35 M_⊙/L_⊙, 47 M_⊙/L_⊙, and 13 M_⊙/L_⊙, respectively.     

－类非线性微分方程解空间显易结构的唯一性

对所有形如的方程的集合Ｅ（Ｄ），引入线性变换群Ｇ（Ｄ），从而将Ｅ（Ｄ）进行等价分类，并由此提出解空间显易结构唯一性概念，指出Ｂｅｒｎｏｕｌｌｉ类方程具第一显易结构，但其显易结构不唯一，而任何非Ｂｅｒｎｏｕｌｌｉ类方程着具显易结构，则其显易结构必唯一．     

载人航天器显示仪表展望

根据９０年代的先进技术展望载人航天器显示仪表的未来发展。在简单回顾现有航天器仪表之后,介绍９０年代有代表性的先进的波音７７７飞机座舱仪表。接着讨论彩色液晶平板显示仪、大屏幕显示仪与玻璃座舱等９０年代的先进技术,并提出由计算机统一管理的带自然语言输出的仪表,以发挥航天员听觉的作用和减轻航天员的视觉负担。     

The entropy in groups – a clue to galaxy formation

The entropy in the hot X-ray gas in groups of galaxies is a fossil of the process of galaxy formation The amount of entropy in these low mass systems considerably exceeds that predicted from structure formation models. To explain these results requires “extra” energy which is a relic of the process of star formation and active galaxy heating. We present new XMM results on the entropy and entropy profiles. These results are inconsistent with pre-heating scenarios which have been developed to explain the entropy floor in groups but are broadly consistent with models of structure formation which include the effects of heating and/or the cooling of the gas. The total entropy in these systems provides a strong constraint on all models of galaxy and group formation, and on the poorly defined feedback process which controls the transformation of gas into stars and thus the formation of structure in the universe.     

光——一种特殊的建筑材料

本文主要根据光在当代建筑艺术的应用,探讨光这种特殊的材料的特点及其作用,以期唤起人们对光材料的重新认识和重视,并主动合理地把它运用到建筑设计中去.     

伸展垂直薄片非定常层流自然对流的群论分析

用Ｍｏｒｇａｎ的双参数变换群理论，对磁场作用下的伸展垂直薄片的不可压缩非定常层流自然对流边界层流动进行相似性分析，得到了三种情况下的相似性解方程组。并在不同的Ｐｒ，Ｎｍ，Ｆｃ和ｒ下，用四阶龙格－库塔法进行了数值求解，得到了速度和温度分布，并给出了一组相似性解的结果。     

中国企业集团发展研究

回顾了国际上企业集团的发展过程,总结了改革开放以来,我国企业集团从无到有、从低级到高级、从不完善到规范化的经验,指出了组建股份制企业集团的方向。     

Essential features of long-term changes of areas and diameters of sunspot groups in solar activity cycles 12–24

We analyze the Greenwich catalog data on areas of sunspot groups of last thirteen solar cycles. Various parameters of sunspots are considered, namely: average monthly smoothed areas, maximum area for each year and equivalent diameters of groups of sunspots. The first parameter shows an exceptional power of the 19th cycle of solar activity, which appears here more contrastively than in the numbers of spots (that is, in Wolf’s numbers). It was found that in the maximum areas of sunspot groups for a year there is a unique phenomenon: a short and high jump in the 18th cycle (in 1946–1947) that has no analogues in other cycles. We also studied the integral distributions for equivalent diameters and found the following: (a) the average value of the index of power-law approximation is 5.4 for the last 13 cycles and (b) there is reliable evidence of Hale's double cycle (about 44?years). Since this indicator reflects the dispersion of sunspot group diameters, the results obtained show that the convective zone of the Sun generates embryos of active regions in different statistical regimes which change with a cycle of about 44?years.