长白山望天鹅火山双峰式火山岩的成因演化

望天鹅火山活动从早到晚分为三期：①长白期以粗面玄武岩为主,少量碱性玄武岩和玄武质粗安岩;②望天鹅期又分早晚两个亚期,早期玄武质粗安岩和粗面岩,晚期碱性流纹岩;③红头山期碱性流纹岩。望天鹅火山岩的岩石学、ＲＥＥ、不相容元素和Ｎｄ、Ｓｒ、Ｐｂ同位素（１４３Ｎｄ／１４４Ｎｄ、８７Ｓｒ／８６Ｓｒ、２０６Ｐｂ／２０４Ｐｂ分别变化于０．５１２５６７～０．５１２６４２、０．７０５１９８～０．７１６７４２和１７．４３４～１７．９３４）,揭示了岩浆源区明显受洋壳的俯冲和壳幔混合混染,三期火山岩具有共同的岩浆源区和紧密的成因演化关系,分离结晶作用控制了岩浆的演化过程。原始碱性系列玄武质岩浆经橄榄石、辉石的结晶分异,向粗面玄武岩演化;粗面玄武岩经斜长石强烈的结晶分离作用,还有辉石、钛铁氧化物和磷灰石的分离结晶作用形成具显著Ｅｕ、Ｓｒ、Ｂａ、Ｔｉ、Ｐ负异常的碱性流纹岩,导致本区火山岩缺失中性（ＳｉＯ２＝５７％～６３％）的安山岩和粗安岩,呈现双峰式火山岩组合的特点。     

铀矿地质样品中有机碳的测定

用盐酸预处理岩矿样品以驱除样品中的碳酸盐碳;滤出酸不溶物并洗净,待干燥后置入900-1000℃的管式炉中,在富氧气流中灼烧,有机碳被氧化成CO2由烧碱石棉吸收后称重,根据烧碱石棉管的增重计算有机碳的含量。对含有机碳为0．23％的样品进行10次测定,标准偏差为0．0116％,变异系数为5．04％。     

香港地区活动断裂的初步探讨

香港地区的断裂构造颇为发育,主要有北东、北东东和北西向三组断裂。在现今构造应力场作用之下,北东东和北西向断裂组成共轭断裂系统。由于本地区地震活动水平不高,尚难确定哪组断裂与地震活动密切相关。断层泥的热释光资料表明,断裂的最新活动应在晚更新世,断裂的复发周期应在１０万年左右。目前尚不能肯定哪条断裂为活动断裂。     

大陆下地壳的研究进展综述

大陆下地壳对认识整个地壳的组成演化具有重要意义,对大陆下地壳的研究正在世界范围蓬勃开展,大陆下地壳的研究基于两个方面：一是太古代地壳剖面的研究,二是麻粒岩包体的研究,相比较而言后者的研究程度要难得多,下地壳包体出露少,成分多为麻粒岩,且无一例外地都含有基性麻粒岩,对其成因现基本趋于一致认识,即由幔源岩浆底侵至地壳再受变质而成,然后被火山作用带至地表,因此,基性麻粒岩包体更可能反映了现今大陆下地壳的     

Inflation in Bianchi type-IX Einstein-Cartan Cosmological Model

Within the framework of Einstein-Cartan theory with Weyssenhoff fluid, we investigate an inflation model for an anisotropic Bianchi type-IX cosmological model. The system of field equations is solved numerically and an inflation epoch is achieved. The general condition for the inflation to occur is also discussed. This anisotropic model evolves quickly towards to an isotropic one.     

塔里木盆地塔中地区奥陶系碳酸盐岩储层空隙研究

空隙是构成碳酸盐岩储层的基本单元,空隙发育史对应了成岩演化史,且不同类型空隙的储层具有不同的分布规律。塔里木盆地塔中地区奥陶系碳酸盐岩储层的空隙可以分为６类２１种,以裂缝—孔洞型为主,礁、丘、滩相碳酸盐岩、中—细晶白云岩与古岩溶和构造岩溶的复合区为有利空隙发育带,也是风化壳型油气藏和内幕型油气藏的有利储集相带。     

The Complete Sequence of Mitochondrial COⅡ Gene of Fenneropenaeus chinensis and Its Applicability as a Marker for Phylogenetic Analysis

The complete mitochondrial cytochrome oxidase subunit Ⅱ （COⅡ） gene of Penaeinae shrimp Fenneropenaeus chinensis was cloned and sequenced. The gene is 688 bp in length and codes for 229 amino acids. It shows 83.2%, 87.0% and 83.8% sequence similarity to Marsupenaeus Japonicus, Penaeus monodon and Farfantepenaeus notialis, respectively. The A＋T content of the whole gene and that at the third position of codons are 64.7% and 78.2%, respectively. The phylogenetic relationship between F. chinensis and three other species representing genera Farfanatepenaeus, Marsupenaeus and Penaeus was analyzed. Results showed that the genetic distances among the four taxa ranged from 0.144 0 to 0.200 5, exceeding those estimated with COⅠ and partial 16S rRNA gene sequences among Marsupenaeus, Litopenaeus and Melicertus, and being therefore larger than the value among subgenera. It has been suggested that the COⅡ gene has a faster evolutionary rate than that of the COⅠ gene and partial 16S rRNA gene and could be used for phylogenetic analysis at genus or species level. The results of the present study indicated that Farfantepenaeus, Fenneropenaeus, Marsupenaeus and Penaeus are at a higher phylogenetic level than subgenus, which supports the opinion of the elevation of phylogenetic status of the four subgenera to genus level.     

黏粒和有机质对黄河口潮间带沉积物微团聚体的影响

微团聚体是形成沉积物结构的基本单元,沉积物的结构性影响了土体的稳定性、渗透性和强度等工程地质性质。对废弃黄河口刁口流路潮间带沉积物微团聚体受黏粒含量、有机质和生物黏液等胶结作用进行分析,结果表明,研究区沉积物多团聚成粉粒级微团聚体(0.05～0.01 mm),含量在85.3%～95.8%之间,与黄土高原土相比,0.05～0.01 mm微团聚体增加,而0.1～0.05 mm微团聚体减少,团聚性差,易于侵蚀;黏粒含量与团聚度表现出显著正相关性,说明黏粒含量增加了沉积物微团聚体的稳定性;沉积物中有机质含量在0.27%～0.61%之间,有机质含量较少,对沉积物微团聚体贡献少;生物扰动的螃蟹洞壁土、螃蟹掘出物的团聚度明显大于表层未受生物扰动土的团聚度,说明螃蟹分泌的黏液能加大微团聚体的稳定性。     

Analysis of types and changes of village-level economy in rural Gongyi city,Henan Province since 1990

Based on the research on the rural living standard in China in terms of annual net income per capita, we define six types of village-level economy, i.e. ＂to be extremely poor＂, ＂to make a basic living＂, ＂to dress warmly and eat one＇s fill＂, ＂to try to enrich （to disengage poverty）＂, ＂to be well-off＂ and ＂to be affluent＂. The data of average annual net income of all the 292 villages between 1990 and 2004 in rural Gongyi City, Henan Province were collected, verified and classified. By using standard deviation, coefficient of variation and regression analysis, it is found that the Gongyi＇s rural economy has boosted up remarkably from the relative-poverty and absolute-poverty stages in 1990 to the well-off in 2004. However, the absolute differences between villages present a trend of enlargement, while the relative differences fluctuating. On the other hand, spatial analysis of village-level economy shows that most villages with relatively high economic development level were located along national expressway and most villages with absolute-poverty lay in remote mountainous areas in 1990. Since the 1990s, the rapid urbanization and industrialization have had strongly positive effects on rural economic growth. Initial economic foundation, natural resources and traditional techniques also contribute to village economy. From the perspective of geography, villages with location advantages, such as near urban center or industrial parks, have more chances for their economic development and the ＂core-periphery＂ economic structure has been presented in the process of rural development.     

EUV and Magnetic Activities Associated with Type-I Solar Radio Bursts

Type-I bursts (i.e. noise storms) are the earliest-known type of solar radio emission at the meter wavelength. They are believed to be excited by non-thermal energetic electrons accelerated in the corona. The underlying dynamic process and exact emission mechanism still remain unresolved. Here, with a combined analysis of extreme ultraviolet (EUV), radio and photospheric magnetic field data of unprecedented quality recorded during a type-I storm on 30 July 2011, we identify a good correlation between the radio bursts and the co-spatial EUV and magnetic activities. The EUV activities manifest themselves as three major brightening stripes above a region adjacent to a compact sunspot, while the magnetic field there presents multiple moving magnetic features (MMFs) with persistent coalescence or cancelation and a morphologically similar three-part distribution. We find that the type-I intensities are correlated with those of the EUV emissions at various wavelengths with a correlation coefficient of 0.7?–?0.8. In addition, in the region between the brightening EUV stripes and the radio sources there appear consistent dynamic motions with a series of bi-directional flows, suggesting ongoing small-scale reconnection there. Mainly based on the induced connection between the magnetic motion at the photosphere and the EUV and radio activities in the corona, we suggest that the observed type-I noise storms and the EUV brightening activities are the consequence of small-scale magnetic reconnection driven by MMFs. This is in support of the original proposal made by Bentley et al. (Solar Phys. 193, 227, 2000).