γ射线暴的logN(>P)～logP分布

本文用简单的宇宙学模型 ,在标准烛光和均匀分布的假设下计算了γ射线暴的logN(>P)～logP分布 (大小谱 ) .在考虑了探测效率修正和死时间修正后 ,由宇宙学模型计算的理论结果和BATSE实测的大小谱没有显著的偏离     

Marine Ingressive Events Recorded in Epicontinental Sequences:Example from the Cretaceous Songliao Basin of NE China in Comparison with the Triassic Central Europe Basin of SW Germany

Songliao Basin is filled predominantly with continental facies sediments including alluvial fan, fluvial plain, fan delta , lacustrine delta, shore ?shallow lacustrine, beach salty flat, semi - deep to deep lacustrine, subaqueous gravity flow, lacustrine swamp and pyroclastic sediments. However, some event units were formed during lake - marine linking periods of the Mid - Cretaceous in the basin, which include black shales with high values for salinity ( Sr/Ba) , alkalinity (Ca Mg)/ (Si Al) , reducibility ( Ni Zn)/Ga and sulfide sulfur as well as heavy isotopes. The Breitenholz ?section to be represen-ted for facies comparison with the Cretaceous evaporitic series in Northeast China is localized in Southwest Germany. Stratig-raphically it belongs to the Crabfeld Formation of Keuper of the Germanic Triassic corresponding to Ladinian - Camian of the international reference scale, and is generally called Lower Gipskeuper. The Germanic Triassic was deposited in the epiconti-nental(cratonic) central Euro     

吸积双星脉冲星EXO2030+375中回旋吸收线的迹象

本文作者首次发现了EXO 2030+375的回旋吸收线迹象.这是迄今唯一一个同时有用回旋吸收线直接测量的磁场数据和用吸积演化方法间接测量的中子星磁矩数据的X射线脉冲星.两种测量方法的结果有很大差别,本文提出了可能导致这种差别的物理机制.     

High-pressure eclogites in northern Jiangsu – southern Shandong province, eastern China

Abstract Eclogites are distributed for more than 500 km along a major tectonic boundary between the Sino-Korean and Yangtze cratons in central and eastern China. These eclogites usually have high-P assemblages including omphacite + kyanite and/or coesite (or its pseudomorph), and form a high-P eclogite terrane. They occur as isolated lenses or blocks 10 cm to 300 m long in gneisses (Type I), serpentinized garnet peridotites (Type II) and marbles (Type III). Type I eclogites were formed by prograde metamorphism, and their primary metamorphic mineral assemblage consists mainly of garnet [pyrope (Prp) = 15–40 mol%], omphacite [jadeite (Jd) = 34–64 mol%], pargasitic amphibole, kyanite, phengitic muscovite, zoisite, an SiO₂ phase, apatite, rutile and zircon. Type II eclogites characteristically contain no SiO₂ phase, and are divided into prograde eclogites and mantle-derived eclogites. The prograde eclogites of Type II are petrographically similar to Type I eclogites. The mantle-derived eclogites have high MgO/(FeO + Fe₂O₃) and Cr₂O₃ compositions in bulk rock and minerals, and consist mainly of pyrope-rich garnet (Prp = 48–60 mol%), sodic augite (Jd = 10–27 mol%) and rutile. Type III eclogites have an unusual mineral assemblage of grossular-rich (Grs = 57 mol%) garnet + omphacite (Jd = 30–34 mol%) + pargasite + rutile. Pargasitic and taramitic amphiboles, calcic plagioclase (An₆₈), epidote, zoisite, K-feldspar and paragonite occur as inclusions in garnet and omphacite in the prograde eclogites. This suggests that the prograde eclogites were formed by recrystallization of epidote amphibolite and/or amphibolite facies rocks with near-isothermal compression reflecting crustal thickening during continent–continent collision of late Proterozoic age. Equilibrium conditions of the prograde eclogites range from P > 26 kbar and T= 500–750°C in the western part to P > 28 kbar and T= 810–880°C in the eastern part of the high-P eclogite terrane. The prograde eclogites in the eastern part are considered to have been derived from a deeper position than those in the western part. Subsequent reactions, manifested by (1) narrow rims of sodic plagioclase or paragonite on kyanite and (2) symplectites between omphacite and quartz are interpreted as an effect of near-isothermal decompression during the retrograde stage. The conditions at which symplectites re-equilibrated tend to increase from west (P < 10 kbar and T < 580°C) to east (P > 9 kbar and T > 680°C). Equilibrium temperatures of Type II mantle-derived eclogites and Type III eclogite are 730–750°C and 680°C, respectively.     

SOHM-4与MHM-2010氢原子频标的特点比较

基于对已投入国家授时中心守时运转的SOHM-4型与MHM-2010型氢原子频标的长期关注,对这两种氢原子频标的性能作了较详细的比较和分析。讨论了它们共同的优点、各自的特长和不足之处,还给出了稳定度的测试结果。     

青海祁漫塔格地区斑岩铜矿的成矿条件和远景

文章对青海祁漫塔格地区斑岩铜矿成矿带的成矿地质条件进行了研究,其形成于造山带汇聚阶段中后期的活动陆缘环境,与驱龙斑岩铜矿对比具有相类似的成矿地质条件,找矿远景很大.特别是卡而却卡、乌兰乌珠尔、鸭子沟、尕怒大门等地区具有斑岩铜矿成矿的广阔前景,有希望找到新的大型超大型铜矿床.通过对乌兰乌珠尔矿床的解剖,该矿区构造裂隙发育,岩石蚀变强烈.具典型的"斑岩型"蚀变分带:由中心向外依次为强硅化带??硅化钾化带??绢英岩化带??青磐岩化带.成矿元素以铜为主,伴有铅、锌、锡等多种有用组分.岩浆岩、热液蚀变作用、热液运移和矿质沉淀的构造空间控制了矿床的产出.为进一步在该区找矿指明了方向.     

济南岩溶泉域地下水水质监测

基于GIS手段,利用欧洲方法编制的济南泉域岩溶含水层易污性评价图显示,济南泉域岩溶含水层总体易污性强,地下水容易受到污染。结合泉域污染源调查结果以及地下水补给、径流、排泄系统与水质监测网的现状,设计了51个监测点组成的地下水水质监测网,其中地表水监测点6个,第四系孔隙水监测点8个,变质岩裂隙水监测点1个,泉水监测点4个,岩溶水水源地监测点6个,岩溶地下水监测点26个,并对其监测频率及监测内容进行了分析。     

济南岩溶地下水化学成分的形成

本文研究济南岩溶排泄区地下水化学成分的形成。先用Cl-和NO3-浓度作为示踪剂分析补给区的大气降水输入,鉴别出西郊和平安店排泄区地下水没有被明显污染,市区和东郊排泄区地下水受到明显污染,污染主要来自当地浅层地下水或近地面土层。之后,利用西郊排泄区的测试数据进行了横向径流带的水-岩作用定量分析,与示踪剂研究结果一致,市区和东郊排泄区地下水被明显污染,同时提出地下水在径流过程中发生脱白云石化过程的趋势线。     

高速远程滑坡飞行数值分析

许多大型高速远程滑坡在近程活动阶段呈现凌空飞行运动,其飞行过程必须考虑空气动力学效应和地面效应,但是直接求解高速滑体凌空飞行运动的偏微分方程是困难的。因此,以往的研究只给出了定性分析或粗略的计算结果。本文将以头寨沟滑坡为例,使用数值模拟方法研究高速滑体凌空飞行的运动规律。结果表明,高速滑体凌空飞行时空气动力效应更多地表现为对滑体的抬升作用;高速滑体因空气动力效应的影响而产生不断增大的水平推力和竖向抬升力,使得水平加速度不断增大,竖向加速度不断减小,导致滑体的水平速度不断增大,而竖向速度则趋于稳定值,当水平速度远超过竖向速度时,滑体的飞行姿态将接近于平行于地面。因此,与不考虑空气动力学效应的情况相比,高速滑体凌空飞行时间更长,飞行距离更远,更加符合滑坡的实际情况。     

强降雨条件下土质边坡瞬态稳定性分析

基于实际降雨气象资料,设计了单峰降雨和8个不同时间间隔的双峰降雨计算方案,利用非饱和土力学理论,对边坡的瞬态稳定性进行了计算和分析,研究了水分在坡体内的运移对边坡稳定性的时间空间影响效应,同时考察了降雨入渗造成的土性渗透特性的改变。分析发现：一次降雨的影响历时约12 d,降雨后约0.5 d该类土质边坡最危险;不同时间间隔的两次降雨对边坡稳定的影响比单峰降雨的最小安全系数滞后约0.3 d～0.8 d,影响历时基本保持不变;土体物理力学性质、边坡最危险滑动面及其对应的安全系数随水分在坡体内渗透运移而变化。