祁连山及邻区第四纪地层区划与沉积序列

在前人资料和野外勘查的基础上对祁连山及邻区贵德盆地、循化—化隆盆地、同仁盆地、西宁盆地、门源盆地、临夏盆地、兰州盆地、定西盆地、天水盆地、肃北盆地、酒泉盆地、玉门盆地、张掖盆地、武威盆地、哈拉湖盆地、苏里盆地、木里盆地、民和盆地、共和盆地、青海湖盆地及柴达木等20余个盆地的第四纪地层进行了研究。以祁连山第四纪构造地貌演化、盆地沉积序列、古生物及古气候特征为地层分区依据,对祁连山及邻区第四纪地层进行了地层分区,并对部分地层名称做了厘定或统一。祁连山及邻区第四纪沉积特征总体为东部(主要为陇中地区)黄土分布广泛,堆积了世界上最厚的黄土地层;北部(河西走廊地区)冲洪积扇堆积及风沙发育;南部(柴北盆地)以冲洪积-湖积为主,晚更新世以来发育风成沙及黄土;共和盆地由湖泊转向冲积扇和风沙沉积;青海湖盆延续至今;中西部高山及山间盆地冰碛、冰水堆积以及河流阶地堆积发育。根据上述特征及划分原则,将祁连山及邻区第四纪地层区划分为:兰州—西宁地层区,贵德地层区,酒泉—张掖地层区,柴北地层区,共和地层区,青海湖地层区及肃北—门源地层区。     

Filament activation and magnetic reconnection

Solar Physics - A curved filament in a decaying active region (AR&;nbsp;8329) was observed on 9 September 1998 with a combination of several instruments. The main data base is a 4-hour long time...     

Relation of Velocity Distribution and Mass for DA White Dwarfstwo

White dwarfs are the evolutionary endpoint of the low-and-medium mass stars. In the studies of white dwarfs, the mass of white dwarf is an important physical parameter. In this paper, we give an analysis about the velocity distribution of DA white dwarfs in the Sloan Digital Sky Survey (SDSS), and hope to find the relation between mass and velocity distribution of white dwarfs. We get the radial velocity and tangential velocity of every DA white dwarf according to their proper motion and spectral shift. Through analyzing the velocity distribution of DA white dwarfs, we find that the small-mass white dwarfs, which are produced from the single-star evolution channel, have a relatively large velocity dispersion.     

Searching for Variable Stars in and around Open Clusters

We present a snapshot of our recent results of a variable star survey in 1 degree fields around three open clusters: NGC 188, NGC 7789 and M67. A total number of 39 variable stars are newly discovered, including 22 W UMa stars, 10 EA (Algol) type binaries, one RR-lyr and one RRd pulsator, and five unclassified variables.     

Correlations among color,morphology, and luminosity for the luminous red galaxy (LRG) sample of the SDSS data release 5

We have investigated the correlations among color, morphology and luminosity for all LRGs, cut I LRGs, cut II LRGs, and Main galaxies that are also classified as LRGs. It is found that the morphology of LRGs is tightly correlated with luminosity. The rest-frame u-g color of cut I LRGs and cut II LRGs is nearly independent of luminosity, but the color of Main galaxies is correlated with luminosity. For cut I LRGs and Main galaxies, the early type proportion apparently changes with color: at the rest-frame u-g < 1.3 it increases strongly with increasing color, while at the rest-frame u-g > 1.3 it decreases with increasing color. We also notice that the morphology of cut II LRGs is only a weak function of color. Published in Astrofizika, Vol. 50, No. 3, pp. 335–345 (August 2007).     

Inferring the emission regions for different kinds of gamma‐ray bursts

Using a theoretical model describing pulse shapes, we have clarified the relations between the observed pulses and their corresponding timescales, such as the angular spreading time, the dynamic time as well as the cooling time. We find that the angular spreading timescale caused by curvature effect of fireball surface only contributes to the falling part of the observed pulses, while the dynamic one in the co‐moving frame of the shell merely contributes to the rising portion of pulses provided the radiative time is negligible. In addition, the pulses resulted from the pure radiative cooling time of relativistic electrons exhibit properties of fast rise and slow decay (a quasi‐FRED) profile together with smooth peaks. Besides, we interpret the phenomena of wider pulses tending to be more asymmetric to be a consequence of the difference in emission regions. Meanwhile, we find the intrinsic emission time is decided by the ratios of lorentz factors and radii of the shells between short and long bursts. Based on the analysis of asymmetry, our results suggest that the long GRB pulses may occur in the regions with larger radius, while the short bursts could locate at the smaller distance from central engine. (© 2007 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

抚州市近50年暴雨气候特征

利用逐日降水资料,分析了抚州市1961—2010年暴雨分布规律和气候特点。结果表明,其年代际变化均呈波浪型,20世纪90年代暴雨最多,70年代最少;暴雨具有明显的季节特征,夏季暴雨最多,尤其是6月中下旬最为集中;多区域性暴雨,占暴雨总日数的37.3%,连续暴雨也较多,以连续2 d区域性暴雨为主;暴雨东部多于西部,北部多于南部;年暴雨站次数与年降水量呈很好的正相关;夜暴雨多于昼暴雨。最后,分析了暴雨、大暴雨的主要影响系统和典型天气形势。     

扬子地块新元古代裂谷盆地莲沱组沉积分异及其物源分析

扬子地块莲沱组及相当地层单元的划分和对比,一直是我国南华系(即Cryogenian)研究关键难题之一.新元古代裂谷盆地开启早期,构造-沉积分异作用,同裂谷相变很大,使得盆地边缘区地层序列不完整.过分依赖岩石地层单元对比,历存分歧,典型的就是关于莲沱组与板溪群地层对比、时代归属以及莲沱组的沉积环境问题.本文通过对扬子地块...     

西太平洋地球动力学问题与未来大洋钻探目标

西太平洋区域是全球地质构造和海陆相互作用最活动的区域,经过50多年的大洋钻探研究,人们对西太平洋弧后海底扩张成因、俯冲工厂的动力学机制、地幔演化过程、发震带、热点岩浆活动、沉积古环境等都有了深入研究和分析,但是西太平洋边缘海盆具有很大的构造多样性和复杂性,仍然有很多的科学目标和科学问题有待进一步开展研究.本文详细分析了...     

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…