Ecological Distribution and Significance of Metadiaptomus asiaticus Uljanirs,a Copepod Recently Found on the Qinghai-Tibetan Plateau

正1 Introduction In 2006,plankton investigation was carried out in the lakes in Ali district,Tibet.7 planktonic crustaceans were identified and reported.Metadiaptomus asiaticus Uljanirs was reported for the first time on the QTP(Yuan et al.,2007).However,detailed data on this species,especially its ecological significance,were not mentioned.In this     

沁水煤田赵庄矿区地质构造分析与研究

在野外踏勘和室内资料整理分析的基础上,对赵庄矿区物探工作所查明的断层、井下揭露的断层以及野外观测到的断层进行了断层倾角统计和分断距统计对比分析。对矿区范围内井上下的断层和野外实测节理滑动面的发育规律进行了总结。在此基础上,分析了赵庄矿区地质构造体系及其演化规律。     

Equilibrium Structures of Rotationally and Tidally Distorted Polytropic Models of Stars

We propose suitable modifications in the concept of Roche equipotentials to account for the effect of mass distribution inside a star. The Kippenhahn and Thomas (1970) approach is used to incorporate the effects of rotational and tidal forces in the equations of stellar structure. The proposed method is applied to compute structures of certain rotationally and tidally distorted polytropic models.     

湘中古台山金锑矿床变形序列、成矿事件及控矿构造

湘中古台山金锑矿位于雪峰构造带西南段东北部,发育SN向金矿脉和NW向金锑矿脉2类矿脉。前人提出SN向和NW向断裂为容矿构造,并获得了印支期成矿的⁴⁰Ar-³⁹Ar同位素年龄,但对容矿断裂的性质、形成时代以及2类矿脉的时代关系缺乏研究和认识。鉴于此,文章通过地表和井下露头构造以及矿化蚀变的观测、解析,结合区域构造特征、区域构造演化和测年资料等,厘定了古台山金锑矿区构造变形序列及其时代、不同类型矿脉的成矿时代和构造背景,探讨了构造控矿规律及动力机制。主要认识如下：(1)研究区自早至晚经历了5期主要变形事件：志留纪晚期受到NWW向挤压,形成NNE向板劈理、NNE向褶皱(水车背斜)、SN向顺层断裂、逆冲剪切破裂和断裂;中三叠世晚期受到NNW向挤压,局部形成NEE向轴面劈理;晚三叠世受到SN向挤压,形成EW向褶皱、NW向—NNW向右行走滑断裂和剪切破裂、NNE向左行走滑断裂和剪切破裂、EW向逆冲剪切破裂等;中侏罗世晚期受到NWW向挤压,形成EW向右行剪切破裂和断裂;古近纪中晚期受到NE向—NNE向挤压,形成SN向—NNE向右行剪切破裂和断裂、EW向—N...     

青藏高原错那—沃卡裂谷中部电性结构及其动力学意义

藏南裂谷作为青藏高原最显著的伸展构造样式之一,是研究高原生长过程的重要窗口,但目前其深部成因机制仍存在较大争议。本文利用沿错那—沃卡裂谷中部的大地电磁数据,分析裂谷区域的大地电磁测深曲线特征和相位张量,并通过三维大地电磁反演获得邛多江地堑和沃卡地堑深部电性结构。三维大地电磁反演结果显示,沃卡地堑和邛多江地堑深部存在一条连续的显著高导异常,并呈现“俯冲”形态,且上覆高阻结构体,而在邛多江地堑两侧浅部则分布低阻异常。结合早期的研究结果,本文支持错那—沃卡裂谷深部的高导异常为地壳部分熔融,可能与南向地壳流相关,并研究认为在南北向持续挤压作用下,裂谷下方的弱地壳层,通过解耦上地壳和下部地壳,促进了藏南裂谷系的发育。     

江西武功山花岗岩地貌特征与成因

江西武功山花岗岩穹窿构造地貌景观类型具有多样性、典型性,具有极高的美学价值、科学价值和旅游开发价值。武功山花岗岩地貌类型可划分为花岗岩风化壳高山草甸、花岗岩侵蚀构造地貌、花岗岩流水侵蚀地貌和花岗岩崩塌堆积地貌等,而且每一类型又有多种微地貌景观,具有显著的集聚性特征,主要集中在金顶、明月山和羊狮幕地区,空间上可分为4个梯度,分别为中心高山草甸带、中心边缘构造侵蚀地貌区、外围峡谷、孤峰、瀑布、温泉区、武功山主山体前缘区。花岗岩穹窿构造核部及外缘区域的花岗岩地貌发育模式和发育阶段具有明显差异,反映了武功山不同山体单元多期差异性隆升后,在亚热带气候环境下,流水溯源侵蚀、构造、岩体性质等内外营力对原始地貌面的差异性作用过程。本研究不仅可为花岗岩穹窿构造地貌景观空间展布规律和地貌特征的研究提供有效借鉴,而且可为武功山地区地学科普、地质遗迹保护等提供支撑。     

Structural style of the Chos Malal fold and thrust belt,Neuquén basin,Argentina: Relationship between thick- and thin-skinned tectonics

The Chos Malal fold and thrust belt (FTB) is a thick-skinned mountain belt formed by Mesozoic deposits of the Neuquén Basin during the Andean orogeny. Four structural cross-sections in the entire deformed area, supported by field and subsurface data, suggest a strong link between thick and thin-skinned structures. Major Andean thrusts branching from a detachment placed 12 km into the crust created large basement wedges, which were inserted in the cover producing minor order structures. The westernmost of these wedges is exposed forming the Cordillera del Viento, while others basement slices at depth were interpreted from seismic lines. These thick-skinned structures transferred deformation to the cover along the Auquilco Formation and contributed to create all thin-skinned structures surveyed in the Chos Malal FTB. We recognized half-graben geometries in the seismic lines, preserving their extensional configuration, which suggests that the main normal faults were not inverted. Shortenings calculated from the restoration of the four cross-sections are 16.9 km (29.7%), 16.9 km (29.7%), 14.7 km (26.9%) and 14.15 km (26.3%), which evidence a slight diminution of the contraction toward the south probably associated with the plunge of the Cordillera del Viento structure in this segment of the Chos Malal FTB.     

Rajkanella hottingerinaformis n. gen., n. sp., a new larger benthic foraminifer from the middle-upper Cenomanian of Kosovo

A new larger benthic porcelaneous foraminifer of soritid affinity is described as Rajkanella hottingerinaformis n. gen., n. sp. from the middle-upper Cenomanian of Kosovo. It occurs in foraminiferal packstones and grainstones, in association with cuneolinids, rhapidionids, chrysalidinids, and other benthic foraminifers. Due to its general morphology and superficial chamber subdivision by exoskeletal elements, Rajkanella n. gen. can be compared with the early Paleogene genus Hottingerina Drobne, 1975, from which it mainly differs in its apertural features, ornamented test, and coiled adult stage. Further differences to coeval Pseudorhapydionina De Castro, 1971, Pseudorhipidionina De Castro, 1971, and to other comparable genera, are discussed. The discovery of Rajkanella hottingerinaformis in the middle-upper Cenomanian is a further witness of the significant radiation and blooming of increasingly complex porcelaneous foraminifers in inner platform, shallow-water depositional settings during that period.     

Comparative Analysis of Seismic Response Characteristics of Pile-Soil-Stnicture Interaction System

The study on the earthquake-resistant performance of a pile-soil-structure interaction system is a relatively complicated and primarily important issue in civil engineering practice. In this paper, a computational model and computation procedures for pile-supported structures, which can duly consider the pile-soil interaction effect, are established by the finite element method. Numerical implementation is made in the time domain. A simplified approximation for the seismic response analysis of pile-soil-structure systems is briefly presented. Then a comparative study is performed for an engineering example with numerical results computed respectively by the finite element method and the simplified method. Through comparative analysis, it is shown that the results obtained by the simplified method well agree with those achieved by the finite element method. The numerical results and findings will offer instructive guidelines for earthquake-resistant analysis and design of pile-supported structures.     

日冕磁场和重联的射电信号

总结了近期用射电频谱仪（高时间和高频谱分辨）和野边山射电日像仪（高空间分辨）以及国内外其它空间和地面设备分析日冕磁场和重联的系列工作。主要结论可归纳为：1）在Dulk等人（1982）的近似下自恰计算射电爆发源区磁场的平行和垂直分量，并首次得到该磁场在日面的两雏分布。2）为了考虑非热电子低能截止的影响，必须采用更严格的回旋同步辐射理论来计算。结果表明：低能截止和日冕磁场对计算有明显的影响，而其它参数（包括背景温度、密度、高能截止和辐射方向）的影响均可忽略。因此，对低能截止和日冕磁场必须联立求解。3）射电爆发中的精细结构可能反映了射电爆发源比较靠近粒子加速（磁场重联）的区域，利用高时间和高频率分辨的频谱仪和高空间分辨的日像仪联合分析，可以确定精细结构的源区位置，从而确定粒子加速（磁场重联）的准确时间和地点。