中国科学院资源环境科学研究工作的创新与发展

１１９９８年工作回顾１９９８年在以江泽民同志为核心的党中央领导下,在实施科教兴国战略和“迎接知识经济时代,建设国家创新体系”的试点工作中,我们全院从事资源环境科学技术研究的同志,从２１世纪中国发展的战略需要和世界科学前沿的前景出发,重新确定科技发展目...     

黄山第四纪泥砾沉积物分形结构特征与成因机制分析

黄山第四纪泥砾沉积物粒度组成的分维值介于２７０８～２７３５之间,非常接近古泥石流堆积物粒度组成的典型分维值２７５．结合沉积特征,表明该沉积物属第四纪间冰缘环境下的稀性泥石流沉积,其形成过程与季风型冰缘环境有关     

中国南水北调工程进展综述

论述南水北调工程的调水背景、工程规划、工程特征、环境影响与生态环境保护及其工程综合效益。     

西昆仑造山带中带提热艾力组沉积环境及物源区构造背景

西昆仑造山带中带上石炭统提热艾力组为一套浅变质碎屑岩沉积,四周被三叠纪岩浆岩所包围,研究其沉积环境及物源特征对揭示该区构造背景具有重要的意义。通过野外详细的剖面测制、沉积相标志的观察,结合室内岩矿鉴定和地球化学等综合分析,揭示该套碎屑岩具典型的鲍马序列结构特征,岩性成分成熟度低,主要为一套近物源的斜坡重力流沉积,其物源区较为复杂,主要为切割岩浆弧、过渡岩浆弧和再旋回造山带,源区构造环境为大陆岛弧及活动大陆边缘,表现出活动大陆边缘弧后盆地的沉积特点。     

下扬子区二叠系烃源岩评价与生源环境

基于下扬子区海域-陆域钻井岩心和露头岩样, 通过有机岩石学和有机地球化学方法, 应用有效指标参数, 从不同维度综合分析下扬子区上二叠统大隆组、龙潭组和下二叠统孤峰组、栖霞组4套烃源岩在纵向及平面上的有机地球化学特征、生烃潜力和生源环境。根据测试数据及前人研究资料, 栖霞组和大隆组烃源岩的有机质丰度为中等-好级别, 龙潭组烃源岩的有机质丰度为一般-中等级别, 孤峰组烃源岩有机质丰度达到很好级别。下二叠统烃源岩有机质丰度在平面展布上表现出海域优于陆域的特点, 上二叠统则反之。根据干酪根碳同位素特征, 栖霞组烃源岩有机质类型最好, 为Ⅰ~Ⅱ型; 其他3套烃源岩均为Ⅱ~Ⅲ型母质类型。4套烃源岩成熟度参数镜质体反射率主频分布范围为1.3%~2.0%, 均达到高热演化阶段, 在平面展布上表现出明显的非均一性。二叠系4套烃源岩生物来源以低等水生生物为主, 有机质均在贫氧的弱还原-弱氧化条件下保存, 其中大隆组沉积的水体动荡频繁和生物变化较明显。综合认为, 下扬子区二叠系烃源岩有机质丰度高, 类型较好, 具有形成大型油气田的良好物质基础, 尤其是以往被忽略的孤峰组烃源岩评价等级被提高, 是一套潜在的优质烃源岩, 其对该区进一步的油气勘探具有重要的指导意义。     

Microbial signatures in sabkha evaporite deposits of Chott el Gharsa (Tunisia) and their astrobiological implications

This study investigates the geomicrobiological potential of Upper Pleistocene evaporite deposits of the Chott el Gharsa, a wide continental sabkha in southern Tunisia. Organic and inorganic-derived biosignatures are mostly contained in microcrystalline, laminated gypsum lithofacies consisting of light/dark alternations of concordant laminae, which have precipitated from high salt concentrated waters. These biosignatures include mineralized microbial-interpreted morphologies, such as mucilage, rods, and microfibers, and dumbbell morphologies in the hollow cores of dolomite crystals that are associated with sulfates. Mineral products that are induced by microbial activity and their organic compounds lead to the formation of lenticular-shaped gypsum crystals, with a high length/width ratio, dolomite precipitation and formation of pyrite framboids. Morphological and structural aspects of these biosignatures, and their composition, in laminated, dolomite-rich sulfate deposits could be detected through microscopic investigations and micro-analyses performed by the instrumentation that is planned for ongoing Mars sample return missions.     

ISO14000环境管理系列国际标准简介

本文概述ＩＳＯ１４０００环境管理系列国际标准的产生背景、国际环境管理标准化技术委员会、已发布的五项环境管理国际标准以及宣传贯彻该系列标准的建议。     

入海泥沙减少对黄河三角洲潮滩粒度特征的影响

为探究不同悬沙浓度下潮滩粒度特征的变化,对黄河三角洲潮滩进行了物理模拟实验。使用采自研究区的潮滩表层沉积物,设定与实际潮滩尺寸按比例缩小的室内水槽以及波浪潮汐动力模拟,对不同悬沙浓度条件（0～14.9 kg/m3）下的模拟“潮滩”进行粒度分析。结果表明,随着悬沙浓度的减少,潮滩粒度特征发生了明显变化。随着含沙量的减少,整个潮滩的细颗粒沉积物分布范围减小,总体上沉积物呈现粗化特征,但颗粒较大的极粗粉砂的分布同样减少;在不同含沙量条件下,分选系数、偏度和峰度均值总体呈现出潮下带上部高、潮间带和潮下带下部低的特征,反映了模拟的潮间带上部和潮下带前缘的分选较潮滩中部更好的特征。含沙量的变化同样影响了模拟潮滩的微地貌形态,随着含沙量的降低,潮滩微地貌逐渐侵蚀破碎。潮滩物理模型实验有助于快速再现潮滩冲淤形态和变化特征,使特定条件下潮滩的变化具备可预见性,从而为人类有针对性地进行生产活动提供参考。     

Lofted charged dust distribution above the Moon surface

We developed kinetic theory for the charging processes of small dust grains near the lunar surface due to interaction with the anisotropic solar wind plasma. Once charged, these dust grains, which are exposed to the electric field in the sheath region near the lunar surface, could loft and distribute around such heights off the surface where they reach equilibrium with the local gravitational force. Analytical solutions were derived for the charging time, grain floating potential, and grain charge, characterizing the charging processes of small dust grains in a two-component and in a multi-component solar wind plasma, and further highlighting the unique features presented by the high streaming plasma velocity. We have also formulated a novel kinetic theory of sheath formation around an absorbing planar surface immersed in the anisotropic solar wind plasma in the case of a negligible photoelectric effect and presented solutions for the sheath structure. In this study we combined the results from these analyses and provided estimates for the size distribution function of dust that is expected to be lofted in regions dominated by the solar wind plasma, such as near the terminator and in nearby shadowed craters. Corresponding to the two dominant streaming velocity peaks of 300 and 800 km/s, mean dust diameters of 500 and 350 nm, respectively, are expected to be found at equilibrium at heights of relevance to exploration operations, e.g., around 1.5 m height off the lunar surface. In shadowed craters near the terminator region, where isotropic plasma should be dominating, we estimate mean lofted dust diameter of 800 nm around the same 1.5 m height off the lunar surface. The generally applicable solutions could be used to readily calculate the expected lofted size distribution near the lunar surface as a function of plasma parameters, dust grain composition, and other parameters of interest.