An excursion set model for the distribution of dark matter and dark matter haloes

A model of the gravitationally evolved dark matter distribution, in the Eulerian space, is developed. It is a simple extension of the excursion set model that is commonly used to estimate the mass function of collapsed dark matter haloes. In addition to describing the evolution of the Eulerian space distribution of the haloes, the model allows one to describe the evolution of the dark matter itself. It can also be used to describe density profiles, on scales larger than the virial radius of these haloes, and to quantify the way in which matter flows in and out of Eulerian cells. When the initial Lagrangian space distribution is white noise Gaussian, the model suggests that the Inverse Gaussian distribution should provide a reasonably good approximation to the evolved Eulerian density field, in agreement with numerical simulations. Application of this model to clustering from more general Gaussian initial conditions is discussed at the end.     

Damped Lyα absorbers from dwarf galaxy ejecta

It is argued that the formation of a dwarf galaxy causes a massive burst of star formation, resulting in the ejection of most of the available gas from the galaxy as a weakly collimated wind. The ejected gas can give rise to a damped Lyα absorber (DLA). Weakly collimated outflows naturally explain the asymmetric profiles seen in low-ionization absorption lines caused by heavy elements associated with DLAs, where absorption is strongest at one edge of the absorption feature. The shape of the distribution of column densities in the model agrees reasonably well with observations. In particular, the break in slope is caused by external photoionization of the wind. A semi-analytical model for galaxy formation is used to show that, for currently acceptable cosmological parameters, dwarf galaxy outflows can account for the majority of DLA systems and their distribution with redshift. This model also predicts a correlation between velocity structure and metallicity of DLA systems, in qualitative agreement with observations. DLAs do not require many large, rapidly rotating disc galaxies to have formed early on, as in other models for their origin.     

Mass segregation in young stellar clusters

We investigate the evolutionary effect of dynamical mass segregation in young stellar clusters. Dynamical mass segregation acts on a time-scale of order the relaxation time of a cluster. Although some degree of mass segregation occurs earlier, the position of massive stars in rich young clusters generally reflects the cluster's initial conditions. In particular, the positions of the massive stars in the Trapezium cluster in Orion cannot be due to dynamical mass segregation, but indicate that they formed in, or near, the centre of the cluster. Implications of this for cluster formation and for the formation of high-mass stars are discussed.     

辽宁省金矿成矿作用研究

辽宁省是我国重要的金矿产地之一。省内金矿可划分为岩浆热液型、陆相火山岩型、同韧性剪切变质热液型、变质—岩浆热液叠生型、砂砾岩型及河相冲积型（砂金矿）六种类型。金矿的形成与特定的地层、构造、岩浆岩密切相关。稳定同位素资料表明，金矿的成矿物质主要来源于古老的结晶基底——太古宙变质杂岩（第一矿源层）及早元古宙中浅变质岩（衍生矿源层）；含矿热液主要为岩浆水，变质水和大气水，且多为两种水的混合物；大气水在成矿作用中占有重要地位。金矿的成矿演化经历了太古代－早元古代矿源层及同韧性剪切变质热液金矿床、晚三叠纪－燕山早期岩浆热液及叠生型矿床及燕山晚期陆相火山岩型矿床三个形成阶段。     

准噶尔盆地中部1区块侏罗系三工河组油气输导特征分析

分析准噶尔盆地中部1区块侏罗系三工河组油藏输导格架构成及输导特征对油气分布的控制机制.研究区内砂岩输导层包括J1s12输导层及J1b1输导层,对2套输导层的分布及成因类型进行综合评价,认为J1s12砂体为区内主要输导层;将区内断裂体系划分为深层油源断裂与浅层层间断裂,前者是油气垂向输导的最主要通道,后者是油气向圈闭聚集的重要通道.结果表明:现今构造格局不是准中1区块岩性油气藏成藏控制因素,成藏期主要输导层J1s12古构造脊控制油气运移方向,油源断裂沟通的圈闭及输导层古构造脊上与层间断层沟通的圈闭是油气聚集的主要场所.     

Morphological observation of Epithemia ocellata (Ehr.) Kütz. (Bacillariophyceae) from China

The species of Epithemia ocellata (Ehr.) Kütz. from Northeastern China were observed by scanning electron microscopy (SEM). The studies on silica valve formation in different stages were made. At the early stage, a Y-shaped raphe sternum was found. Areolae were made from virgae and vimines. In immature valves, the canal formation before the raphe fissure is visible. The raphe system, virgae and vimines (areolae) might be the early siliceous elements of the valve during morphogenesis. The formations of virgae and vimines are similar to that of Gephyria media W. Arnott. Rows of silica papillae formed gradually on the face of the valve. After the areolae were covered with silica and form rows of papillae, the outer valve surface could become mature. Details of the internal costae were observed in mature valves.     

山东莱芜九龙山寒武纪张夏组核形石灰岩分类及沉积环境探讨

核形石灰岩作为微生物岩的一种重要类型,长期受到地质学家的广泛关注;近年来,随着研究的不断深入,有关核形石灰岩分类、沉积环境等的探讨再次成为沉积学研究的热点。通过野外观察描述与室内镜下分析相结合,对山东莱芜九龙山寒武纪张夏组产出的核形石灰岩进行系统研究。根据核形石灰岩的宏观特征、共生组分及其含量等特征,将该地区产出的含核形石的灰岩分为:生屑质核形石灰岩、含生屑核形石灰岩、含核形石生屑灰岩与含核形石鲕粒灰岩4类,同时对4种含核形石灰岩的沉积环境进行系统分析,主要为潮下低能带与潮下高能带,并简要分析了该地区核形石灰岩的形成过程。     

潍北凹陷孔店组二段页岩气资源潜力分析

潍北凹陷是昌潍坳陷的次一级凹陷盆地,也是胜利油田外围常规油气开采区。潍北凹陷孔店组二段发育了较厚的暗色泥页岩,是页岩气形成最有利层段,也是常规油气的生烃母岩。利用昌页参1井数据,结合以往资料,对潍北凹陷孔店组二段岩性特征,有机地球化学特征、矿物组成、泥页岩含气性特征等进行分析研究,认为孔店组二段上亚段下部和中亚段下部具备页岩气资源勘查开发潜力。     

Research on formation density MWD instrument in engineering geological exploration

A high efficiency method is very important in geological survey for a new city in China. Geophysical parameters are Measured While Drilling(MWD), and these parameters are processed and explained on the ground, so the method can replace conventional engineering geological exploration for drilling rock sample. According petroleum engineering MWD, using the different characters of different rock absorbs γ radial, with the method of storing data in hole and explaining data on the ground, engineering geological exploration formation density MWD is researched. The MWD works stabilized, and the performance is good with precise data.