秦岭勉略缝合带组成与古洋盆演化

秦岭勉略构造带是典型的蛇绿构造混杂岩带,带内组成复杂、变形强烈,其主导构造样式表现为以系列北倾逆冲断层为格架,不同岩片推覆叠置的叠瓦状构造。详细的组成及构造研究表明,缝合带由洋盆形成演化不同阶段、不同性质的陆缘沉积岩系、不同类型蛇绿岩以及洋盆俯冲－碰撞造山过程中以不同方式出露的构造岩块组成,同时区域地层对比表明勉略古洋盆形成过程具有自西而东“剪刀式”打开扩展的性质与特点。     

Slope stability analysis using evolutionary optimization techniques

Slope stability optimization, in the presence of a band of a weak layer between two strong layers, is accounted for in complicated geotechnical problems. Classical optimization algorithms are not suitable for solving such problems as they need a proper preliminary solution to converge to a valid result. Therefore, it is necessary to find a proper algorithm which is capable of finding the best global solution. Recently a lot of metaheuristic algorithms have been proposed which are able to evade local minima effectively. In this study four evolutionary algorithms, including well‐known and recent ones, such as genetic algorithm, differential evolution, evolutionary strategy and biogeography‐based optimization (BBO), are applied in slope stability analysis and their efficiencies are explored by three benchmark case studies. Result show BBO is the most efficient among these evolutionary algorithms and other proposed algorithms applied to this problem. Copyright © 2016 John Wiley & Sons, Ltd.     

非单一电离层扰动场的台阵探测分析

真实的ＴＩＤ一类大尺度电离层扰动是非平稳和色散的，而且是统计非单一的．本文首先给出了描述这种真实扰动场的数学模型，进而导出了联系台阵探测可测量与扰动场传播参量的观测方程，在此基础上提出了求解观测方程的时频分析方法．这一台阵探测数据分析的新方法，既能分离出非单一电离层扰动场中各种准单一扰动成分，又能获得准单一扰动成分传播参量随时间的演变和随频率的色散．分析实例表明，本文方法分辨率好，精度高，结果可靠，是适用于ＴＩＤ一类大尺度电离层扰动台阵探测数据分析的有效方法．     

变质作用P—T—t轨迹若干问题评述

着重介绍了目前变质作用P－T─t轨迹研究在变质作用温压确定、变质作用不同阶段时间标定、变质作用动态演化过程的组构标志、变质作用演化热模拟以及变质作用P─T─t轨迹与大地构造环境之间关系等方面所存在的若干问题。     

北黄海盆地东部M隆起构造特征及演化

北黄海盆地是中国东部近海中生代断陷型盆地,详细记载着中国东部复杂的构造活动信息,期间经历了多期岩浆活动和构造反转。M隆起位于北黄海盆地东部,其构造活动记录比周边的坳陷更为详细。为充分认识M隆起的地质结构及沉积响应关系,在充分利用地震、钻测井等资料的基础上,结合区域构造背景,从构造运动学和动力学等方面探讨分析其构造演化历程,进而为北黄海盆地乃至中国东部地区的构造演化提供新的依据。高精度三维地震资料及地质分析揭示,该隆起区发育有5个典型的不整合面,纵向上可划分为5个构造层。结合北黄海盆地所处构造位置、构造变形和沉积充填特征,及板块运动和区域构造演化史,将北黄海盆地东部M隆起自中侏罗世至今的构造演化划分为5个阶段(共9期):裂陷阶段(稳定沉积期、掀斜形成期、早白垩世凹陷沉积期)、构造反转阶段(晚白垩世抬升剥蚀期)、再次裂陷阶段(早渐新世初沉积期、早渐新世末剥蚀期、F2断层活跃期)、再次构造反转阶段(整体抬升期)、区域沉降阶段(区域沉降期)。     

鄱阳湖湿地地理信息系统建设及其关键技术研究

以鄱阳湖湿地为研究对象,建立了集知识、模型和决策为一体的鄱阳湖湿地基础地理信息系统,在一定程度上解决了湿地生态经济建设中环境污染及水文监测、洪涝灾害预测、湿地土地规划时空演变模拟以及水利枢纽建设等不同行业相关业务之间既紧密联系又相互隔离的矛盾。     

中国铝物质流历史变化分析和再生铝资源利用研究

本文采用物质流分析(Material Flow Analysis, MFA)的方法, 构建了铝全生命周期动态物质流分析框架, 自上而下的追踪了1949—2021年中国铝的流量、存量和供需情况。结果表明: 1)1949—2021年中国铝土矿铝物质累计流入量5.86亿t, 国内开采与进口各占一半左右。实际铝物质累计消费量3.74亿t。生命周期内铝损失严重, 铝物质损失量2.39亿t。2)2021年人均铝物质社会存量208.9 kg/人, 与同经济发展时期的北美、日本基本一致。3)1990年以来中国再生铝产量快速增长, 累计0.77亿t, 以国内生产为主, 占比76.7%。随着含铝产品到达寿命及未来铝需求量的持续走高, 将迎来含铝产品的报废时代。建议从全生命周期的角度出发, 减少铝在各个环节的损失量; 合理布局再生铝产业, 提高再生铝的利用, 优化铝供应结构, 促进铝工业低碳转型, 支撑“双碳”目标的实现。     

The most metal-poor galaxies

Summary. Metallicity is a key parameter that controls many aspects in the formation and evolution of stars and galaxies. In this review we focus on the metal deficient galaxies, in particular the most metal-poor ones, because they play a crucial r?le in the cosmic scenery. We first set the stage by discussing the difficult problem of defining a global metallicity and how this quantity can be measured for a given galaxy. The mechanisms that control the metallicity in a galaxy are reviewed in detail and involve many aspects of modern astrophysics: galaxy formation and evolution, massive star formation, stellar winds, chemical yields, outflows and inflows etc. Because metallicity roughly scales as the galactic mass, it is among the dwarfs that the most metal-poor galaxies are found. The core of our paper reviews the considerable progress made in our understanding of the properties and the physical processes that are at work in these objects. The question on how they are related and may evolve from one class of objects to another is discussed. While discussing metal-poor galaxies in general, we present a more detailed discussion of a few very metal-poor blue compact dwarf galaxies like IZw18. Although most of what is known relates to our local universe, we show that it pertains to our quest for primeval galaxies and is connected to the question of the origin of structure in the universe. We discuss what do QSO absorption lines and known distant galaxies tell us already? We illustrate the importance of star-forming metal-poor galaxies for the determination of the primordial helium abundance, their use as distance indicator and discuss the possibility to detect nearly metal-free galaxies at high redshift from Ly emission. Received 19 August 1999 / Published online: 15 February 2000     

The effect of the neutron-star crust on the evolution of a core magnetic field

We consider the expulsion of the magnetic field from the super-conducting core of a neutron star and its subsequent decay in the crust. Particular attention is paid to a strong feedback of the distortion of magnetic field lines in the crust on the expulsion of the flux from the core. This causes a considerable delay in the core flux expulsion if the initial field strength is larger than 10¹¹ G. It is shown that the hypothesis on the magnetic field expulsion induced by the neutron-star spin-down is adequate only for a relatively weak initial magnetic field B ≈10¹¹ G. The expulsion time-scale depends not only on the conductivity of the crust, but also on the initial magnetic field strength itself. Our model of the field evolution naturally explains the existence of the residual magnetic field of neutron stars. Its strength is correlated with the impurity concentration in neutron-star crusts and anticorrelated with the initial field strengths.