长江口南支沉积物元素地球化学分区与环境指示意义

对采自长江口南支的130个表层底质沉积物样品采用X射线荧光光谱法进行了20种常、微量元素的地球化学分析。在此基础上,应用系统聚类法对该区域进行了元素地球化学分区。研究结果表明,研究区主要可以分为两大地球化学分区:Ⅰ区以相对富集SiO2,Sr,Zr元素为典型特征,主要涵盖5 m等深线以浅的长江三角洲前缘区;Ⅱ区以相对富集Al2O3,TFe2O3(全铁),MgO,Pb元素为典型特征,涵盖了前三角洲的广大区域。从地球化学分区的空间分布来分析,这两个分区元素之间的差异反映的是沉积水动力条件与沉积介质物化性质这两个环境要素空间分布的差异性,即在研究区内,表层沉积物元素地球化学空间分布的差异性实质上反映了沉积环境空间分布的差异性。     

基于路网数据和复杂图论的中国城市交通布局评价

城市化的快速发展推动了我国城市道路网的不断扩张和发展.城市道路网是一个动态、开放、自组织的空间复杂网络,构成了城市的结构框架,研究城市道路网的结构特征对路网规划和城市建设有着重要的应用价值.在国内城市道路网络结构特征的相关研究中,很少有学者基于道路走向的视角对整个城市路网结构进行研究,也缺少对全国主要城市路网的整体性评...     

CA FCM方案与其它几种人工增雨评估方案的比较

对河南省12次飞机增雨作业,分别采用作业区域趋势对比双比分析评估方案、区域趋势相关回归分析方案、区域趋势协变量多元回归分析方案、浮动对比区历史回归分析方案（FCM）、以降水量为协变量的CAFCM（ClusterAnalysis〖CD*2〗based Floating Control historical regression Method）方案和以降水量和整层大气可降水量为协变量的CAFCM方案进行效果评估,均得到大于15％的相对增雨量。对结果比较分析表明：协变量由降水量和整层大气降水量两个组成的C     

Essential properties of the cD galaxy in Abell 1795 — II. Radio structure

We consider current problems connected with the evolution of central dominant (cD) galaxies in clusters. In the second part of this series, internal properties of the cD galaxy — in particular its radio structure — are related to the appropriate ones of the cluster. The observations point to an earlier jet ejection along the major axis of the galaxy and a following change of the jet axis. From the existence of “hot-spot” like regions in different directions it is suggested that the radio engine would have to be intermittent with a relatively short period. Alternatively to the intermittent ejection scenario, the radio morphology of 4C 26.42 can be explained in the frame of the “standard” beam or jet model. The radio structure of 4C 26.42 being an inversion-symmetric configuration, which is probably due to galactic cannibalism, could be interpreted as a transition at the inner hot spots (at about 1 kpc) from supersonic, stable Fanaroff-Riley type II jets to subsonic, unstable FR I type structures (“plumes”). A quantitative investigation of the two scenarios for jet interaction with the surroudning interstellar/intercluster medium in 4C 26.42 gives parameter values in reasonable agreement with the ones discussed in the literature for related objects.     

On the total kinetic energy of our galaxy

The total kinetic energy of the Galaxy is estimated from the potential energy by applying the virial theorem. The limits of the potential energy depend strongly on the value of the local escape velocity. They are estimated to be between −7. 10¹⁶ M_Ȯ km²s⁻² and −1. 10¹⁶ M_Ȯ km²s⁻² (escape velocity approximately between 450 km s⁻¹ and 600 km s⁻¹). The specific kinetic energy of the Galaxy as a whole is most likely about 21 000 km²s⁻², being equally distributed among the subsystems if the local escape velocity is near its lower limit; the higher the local escape velocity is, the higher is the specific kinetic energy of the Galaxy due to the influence of the dark corona. The specific kinetic energy of the dark corona tends to become equal to that of the Galaxy as a whole for very high values of the local escape velocity. For the purpose of estimating the totl potential energy of the Galaxy, inter alia, a new model of the Milky Way is developed, which yields both the potential and the density analytically so that it is suitale for calculating the galactocentric orbits.     

Essential properties of the cD galaxy in Abell 1795 — I. General optical and X-ray structure,dynamics and formation

We investigate current problems connected with the formation of cD galaxies. The subject of the present paper is to compare internal properties of the cD galaxy Zw162010 with cluster properties of Abell 1795. This consideration is a first attempt to find commonly valid essential correlations between peculiarities of brightest cluster members as structures and active phenomena and global cluster properties as for instance galaxy populations and concentration degrees. The colours, the X-ray emission, and the velocity of the cD galaxy are used to discuss the obvious influence of the environment on the evolution of the active nucleus. In a second paper (Kirchner et al. 1992) the radio structure is used to investigate the influence of the surrounding cluster medium onto the development of the active nucleus. Furtheron, various jet ejection scenarios will be quantitatively examined.     

基于Mycat的分布式技术在收集与分发系统中的应用

基于Mycat的分布式数据库集群,采用了 Mycat+Mysql+Haproxy+Keepalived的技术架构,实现了一个高可用、高性能和高扩展的分布式数据库集群系统,并对单机版Mysql数据库和基于Mycat分布式数据库集群进行性能比较.结果表明,基于Mycat的分布式技术研发数据库集群系统具有高效性和可行性,可以...     

The irregular galaxy Cassiopeia 1 – a new member of the Local group

A photometry in the V, R, I (Cousins) system has been performed for stars in the galaxy Cassiopeia 1. The resulting colour-agnitude (CM) diagram of Cas 1 reveals the existence of blue stars and the absence of red ones. From an analysis of the CM diagram of the galaxy it is concluded that A_v = 4.0 mag, and the distance modulus (m – M)_o = 24.5 mag, corresponding to a distance of 790 kpc. The visual magnitude of the galaxy is V = 14^m.62 (M_v = −13^m.8) and the colour index (V – R) = 0.89 mag. From the distance determination the galaxy Cassiopeia 1 is a member of the Local group.     

全球-地方联结与产业集群的技术学习--以河南许昌发制品产业为例

以产业区理论、管制理论和全球生产网络理论为基础,以学习创新为核心,构建了一个融生产体系与社会生产体制、制度与协调机制、地方生产网络、全球生产网络“四位一体”的学习型产业区分析框架;运用该框架,以河南许昌发制品产业集群为案例,研究了全球-地方网络联结的方式、动态及其对技术学习的影响。研究发现,通过全球与地方生产网络的建构和有机联结,传统产业集群的技术学习是可以从“低端道路”迈向“高端道路”的,发展学习型产业区应作为我国经济发展与技术创新的一项重大战略和政策。     

A new load balancing scheme on heterogeneous database cluster

IntroductionAlthoughthe development of cluster has gainedmore and more advantages of low-cost ,high-per-formance and high-availability computing, effi-cient resource usage such as CPU, memory andI/Ois still a keyto achieve better performanceincluster syst…