西秦岭寨上金矿综合地球物理研究

寨上金矿是中国西秦岭构造带内一个重要的超大规模卡林—类卡林型金矿床.以往对该金矿床的研究主要集中在矿床学、年代学和成矿特征等方面,缺乏地球物理工作的系统梳理.本文以贯穿研究区的可控源音频大地电磁测深及激电工作为主体研究寨上金矿的深部结构,结合地质资料建立了矿区典型地质—地球物理解释模型,探讨成矿机制,总结寨上金矿赋矿标...     

中国最老岩石和锆石

在中国大陆的许多地区都已发现大于3.4Ga的锆石和岩石.鞍山是全球仅有几个存在≥3.8Ga岩石的地区之一.它们以不大的规模存在于白家坟、东山、深沟寺杂岩中,由糜棱岩化奥长花岗岩、条带状奥长花岗岩和变质石英闪长岩组成.近年来,在鞍山地区还发现了许多3.7～3.6Ga岩石和锆石.锆石Hf同位素组成表明鞍山地区在3.8～3.6Ga期间存在周期性的地幔添加和陆壳形成.除鞍山外,在中国许多地区的不同类型岩石中也获得了≥3.4Ga锆石,虽然它们大多数都是碎屑和残余成因.(1)华北克拉通冀东铬云母石英岩中3.85～3.55Ga碎屑锆石:(2)华北克拉通信阳中生代火山岩长英质麻粒岩中3.66Ga岩浆锆石;(3)华南克拉通宜昌地区杨子地块新元古代砂岩中3.80Ga碎屑锆石(一颗);(4)华南克拉通华夏地块新元古代一古生代变质沉积岩中3.76～3.6Ga碎屑锆石;(5)西北地区塔里木地块阿克塔什塔格地区古元古代片麻状花岗岩中3.6Ga残余锆石;(6)西秦岭奥陶纪变质火山岩中4.08Ga捕掳锆石(一颗);(7)西藏普兰地区奥陶纪石英岩中4.1Ga碎屑锆石(一颗,有3.61Ga增生边).一些古老锆石有高达4.1～4.0Ga的Hf同位素模式年龄.在中国,>3.4Ga地壳物质的比例以往被低估了,发现冥古宙和始太古代物质的可能性仍然存在,它们将对中国早期陆壳演化提供新的制约.     

磨刀门河口枯季波生流场数值模拟研究

本文建立曲线坐标系下的双曲型缓坡方程波浪模型和考虑波浪辐射应力影响的深度平均2D潮流数学模型,首次研究了磨刀门河口2011年地形条件下的枯季波生流场。受波浪作用影响,落潮阶段,波浪作用方向与流向相反,在波浪顶托效应下拦门沙沙脊及外坡处流速普遍减小,形成两个主要回流区,口门外东西两侧浅滩处流速也减小,东西两汊及横洲深槽流速增大;涨潮阶段,波浪作用方向与流向相同,拦门沙沙脊及外坡处流速增大,沙脊处出现冲越流,口门两侧浅滩处流速增大,横洲深槽流速减小。     

1997年2月27日巴基斯坦地震（Ms=7.3）

本对１９９７年２月２７日巴基斯坦地震（Ｍｓ＝７．３）进行了分析研究,该地震发生在巴鲁奇斯坦（Ｂａｌｕｃｈｉｓｔａｎ）省的剪切带内。１９９７年２月２７日至３月２２日记录的余震分布图,提出了破裂长度及破裂取向及破裂取向的第一手资料。破裂区范围为２２ｋｍ×１１０ｋｍ,在剪切带西部呈北西走向,与区域构造趋势一致。采用Ｋｉｋｕｃｈｉ Ｋａｎａｍｏｒｉ（１９９１）公式计算震源机制解,表明西北－南东向冲断层为     

基于欧盟新《电池法》对我国有色金属工业标准体系构建的思考

有色金属作为新能源电池的关键基础材料,其产业发展与电池产业的发展息息相关。欧盟新《电池法》的颁布在以法令形式倒逼欧盟电池产业低碳发展的同时,提高了中国新能源电池进入欧洲市场的门槛,也对产业链上游的有色金属相关产品和工程建设提出特殊要求。本文介绍了欧盟新《电池法》的内容和出台背景,针对法案中电池全生命周期碳足迹、原材料循环利用的有关内容对有色金属工业及标准体系的影响,结合我国有色金属工业现有标准体系的构成,提出了加快建立碳足迹核算和评价标准体系、完善回收循环利用标准体系、进一步强化标准国际合作的建议。     

气象卫星对大兴安岭森林大火的监测

1987年5月6日至6月2日在我国黑龙江省大兴安岭林区发生了一场历时28天的特大森林火灾,损失惨重。国家气象局卫星气象中心监测了这场大火的全过程。     

Calculations concerning interstellar isomeric abundance ratios for C3H and C3H2

The syntheses of interstellar c-C3H2, H2CCC, c-C3H, and HCCC, where "c" stands for the cyclic isomer, are thought to proceed via dissociative recombination of the precursor ions c-C3H3+ and H2CCCH+, which are themselves produced mainly via the radiative association reaction between C3H+ and H2. We have utilized ab initio methods to study the potential energy surface (PES) for the association of the linear ion C3H+ and H2 to form the isomers c-C3H3+ and H2CCCH+. The overall rate coefficient for radiative association has been calculated as a function of temperature via the phase space method. Our ab initio calculations show that the H2CCCH+ isomer is formed directly without an activation barrier from reactants, and that isomerization between the two isomers can occur readily via a low-energy pathway consisting of two transition states (saddle points on the PES) and one intermediate (local minimum on the PES). Calculations of the equilibrium coefficient for the isomerization H2CCCH+ <-> c-C3H3+ as a function of energy shows that equal abundances of these two ions should be produced as relaxation proceeds, in agreement with experimental measurements at high pressure. Our results confirm the important point that a simple ion-molecule association reaction can produce a cyclic hydrocarbon. If dissociative recombination reactions involving c-C3H3+ and H2CCCH+ maintain the carbon skeletal structure of the ions and produce roughly similar C3H/C3H2 branching ratios, then abundance ratios of unity are produced between the cyclic and noncyclic isomers of C3H and C3H2 via this mechanism. The large abundance ratio of c-C3H2 to H2CCC observed in TMC-1 can then be explained by differential destruction rates.     

The 825-1110 angstroms EUV spectrum of Venus

On 15 August 1994 we launched the EUVS sounding rocket payload to observe the 825-1110 angstrom region of Venus's far ultraviolet airglow spectrum. The EUVS telescope/spectrograph obtained good data at five times higher spectral resolution than was previously available in the far ultraviolet. We present these data and compare our results to those obtained by the Galileo UVS and Venera 11/12 UV spectrophotometers. We identify several new spectral emission features, including both singly ionized nitrogen and molecular nitrogen in Venus's spectrum. We also see evidence for electron-impact-induced emission from CO. Finally, the EUVS data indicate that the "Ar" emissions detected in Venus's far ultraviolet spectrum by Venera 11/12 spectrophotometers are in fact not due to argon, thus eliminating the discrepancy between in situ and remote sensing measurements.