The Rumuruti chondrite group

Since 1994, the Rumuruti (R) chondrites have been recognized as a new, well-established chondrite group differing from carbonaceous, ordinary, and enstatite chondrites. The first R chondrite, Carlisle Lakes, was found in Australia in 1977. Meanwhile, the number has increased to 107 (December, 2010). This group is named after the Rumuruti meteorite, the first and so far the only R chondrite fall. Most of the R chondrites are breccias containing a variety of different clasts embedded in a clastic matrix. Some textural and mineralogical characteristics can be summarized as follows: (a) the chondrule abundance in large fragments and in unbrecciated rocks is ∼35–50 vol%; (b) Ca,Al-rich inclusions are rare; (c) the olivine abundance is typically 65–78 vol%; (d) the mean chondrule diameter is ∼400 μm; (e) in unequilibrated R chondrites, low-Ca pyroxene is dominating, whereas in equilibrated R chondrites it is Ca-rich pyroxene; (f) the typical olivine in a metamorphosed lithology is ∼Fa_38–40; (g) matrix olivine in unequilibrated, type 3 fragments and rocks has much higher Fa (∼45–60 mol%) compared to matrix olivines in type 4–6 lithologies (∼Fa_38–41); (h) spinels have a high TiO₂ of ∼5 wt%; (i) abundant different noble metal-bearing phases (metals, sulfides, tellurides, arsenides) occur. The exception is the metamorphosed, type 5/6 R chondrite La Paz Icefield 04840 which contains hornblende, phlogopite, and Ca-poor pyroxene, the latter phase typically occurring in low-grade metamorphosed R chondrites only.In bulk composition, R chondrites have some affinity to ordinary chondrites: (a) the absence of significant depletions in Mn and Na in R chondrites and ordinary chondrites is an important feature to distinguish these groups from carbonaceous chondrites; (b) total Fe (∼24 wt%) of R chondrites is between those of H and L chondrites (27.1 and 21.6 wt%, respectively); (c) the average CI/Mg-normalized lithophile element abundances are ∼0.95 × CI, which is lower than those for carbonaceous chondrites (≥1.0 × CI) and slightly higher than those for ordinary chondrites (∼0.9 × CI); (d) trace element concentrations such as Zn (∼150 ppm) and Se (∼15 ppm) are much higher than in ordinary chondrites; (e) the whole rock Δ¹⁷O of ∼2.7 for R chondrites is the highest among all meteorite groups, and the mean oxygen isotope composition is δ¹⁷O = 5.36 ± 0.43, δ¹⁸O = 5.07 ± 0.86, Δ¹⁷O = +2.72 ± 0.31; (f) noble gas cosmic ray exposure ages of R chondrites range between ∼0.1 and ∼70 Ma. More than half of the R chondrites analyzed for noble gases contain implanted solar wind and, thus, are regolith breccias. The 43 R chondrites from Northern Africa analyzed so far for noble gases seem to represent at least 16 falls. Although the data base is still scarce, the data hint at a major collision event on the R chondrite parent body between 15 and 25 Ma ago.     

基于OpenSees的钢筋混凝土桥墩拟静力试验数值分析

以4个呈弯曲破坏形态的圆形钢筋混凝土桥墩的拟静力试验结果为依据,基于OpenSees中的Beamwith Hinges Element单元,建立了相应的桥墩滞回分析纤维单元模型。由模拟结果与试验结果对比可知,所建立的纤维单元模型对桥墩的骨架曲线及滞回曲线都有良好的模拟效果,且能体现桥墩在反复加载过程中刚度、强度退化现象,表明了模型的有效性。     

老挝长山成矿带与花岗岩有关的铜金铁矿床的成矿模式

老挝作为＂特提斯成矿域＂的重要组成部分,具有丰富的矿产资源,尤其是铜、金、铁、铝、钾盐等优势矿产与中国具有很强的互补性。初步论述了老挝的成矿地质背景和近年来发现的与花岗岩类有关的斑岩型铜-金矿床、矽卡岩型铁矿床的矿化地质特征、矿石矿物特征、矿化与岩体的空间关系,在此基础上初步建立了其成矿模式。基于同位素定年数据和Hf-Rb-Ta元素判别图,推测这些花岗岩及与其相关的矿床形成于晚石炭世华南地块向印支地块俯冲产生的火山岛弧环境。     

类锂离子C^3 光电离过程的研究

使用Ｒ－矩阵方法,采用三态密耦图像计算了类锂离子Ｃ＾３＋激发态１ｓ＾２２ｐ＾２Ｐ的光电离截面,并给出了不同过程及不同分波的截面。计算结果揭示了光电离过程中的Ｒｙｄｂｅｒｇ系列共振。     

Star formation in the Cepheus Flare region – II. A-type stars associated with IRAS sources

In order to reveal the star-forming history of the molecular cloud complex we studied the intermediate mass stellar population in the Cepheus Flare region. (Paper I dealt with the distance and the young stellar object candidates of the region.) Correlating the IRAS Point Source Catalogue and Faint Source Catalogue positions with those of 1214 B8–A8 and 1760 F0–F5 type stars brighter than     and classified during an objective prism survey, we identified 19 stars showing far-infrared excess emission in the Cepheus Flare region. In addition to the 16 stars whose counterparts are given in the IRAS catalogues, we found three more stars with infrared excess not recognized before. In order to identify the young medium-mass stars associated with the Cepheus Flare molecular clouds we observed the optical spectra of the IR-excess stars, and using published optical photometry and the IRAS data we examined their spectral energy distributions (SEDs) and IRAS two-colour diagram. The observations resulted in the discovery of a new Herbig Ae/Be star, BD +68°1118, coinciding with IRAS 21169+6842. More evolved HAe/Be stars may be SAO 19953, BD +67°1314 and BD +69°1231, whose H α lines showed weak emission components. Possible β Pictoris- or Vega-type stars may be HD 203854, HD 212826 and HD 216486, whereas the far-infrared fluxes at the positions of BD +72°1018, HD 210806 and HD 217903 can be attributed to the heating of the interstellar environment. We used distances and radial velocities of the stars derived from the spectroscopy and published optical photometry as indicators of their relations to the clouds. Information on the environment of the observed stars deduced from the diffuse interstellar band at λ 6613 is briefly discussed.     

Wavelength dependence of angular diameters of M giants: an observational perspective

We discuss the wavelength dependence of angular diameters of M giants from an observational perspective. Observers cannot directly measure an optical-depth radius for a star, despite this being a common theoretical definition. Instead, they can use an interferometer to measure the square of the fringe visibility. We present new plots of the wavelength-dependent centre-to-limb variation (CLV) of intensity of the stellar disc as well as visibility for Mira and non-Mira M giant models. We use the terms 'CLV spectra' and 'visibility spectra' for these plots. We discuss a model-predicted extreme limb-darkening effect (also called the narrow-bright-core effect) in very strong TiO bands which can lead to a misinterpretation of the size of a star in these bands. We find no evidence as yet that this effect occurs in real stars. Our CLV spectra can explain the similarity in visibilities of R Dor (M8IIIe) that have been observed recently, despite the use of two different passbands. We compare several observations with models, and find that the models generally underestimate the observed variation in visibility with wavelength. We present CLV and visibility spectra for a model that is applicable to the M supergiant α Ori.     

论企业有共同社会责任与灵活创新网络

企业家共同社会责任是指一个企业或“企业公民”对社会应该承担的义务,涉及到企业与相关利益群体之间的相互关系和价值观、操守以及对人的尊重、社群和企业的环境政策等各个方面。很明显,这一概念的核心是企业对基于经济、社会和环境可持续发展的一种责任和承诺,以改善和提高利益相关方的生活水准和条件。当前,企业家共同社会责任不再仅仅是一种道德伦理而已,而且已经成为一种制度性的自律和规定行为。目前的共识是,在运营过程中一个企业必须时刻关注它对客户、员工、股东、社群、地区发展和环境的经济、社会和道德后果,并使它们取得一个比较好的前景。基于这一观点和理念,本文以跨国公司企业家共同社会责任为视角,主要探讨了跨国公司研发活动与上海浦东新区——我国新经济的高地之一——发展的相互作用,以探索跨国公司研发活动、地区经济增长以及它们在形成灵活创新网络、促进可持续发展中的不同功能和共同作用。内容包括六个部分：1）企业家共同社会责任的相关概念及其关系;2）跨国公司在浦东研发活动的现状和态势;3）跨国公司研发活动与地区经济的联系模式和紧密程度;4）跨国公司在浦东研发活动中存在的主要问题;5）地区灵活创新网络的内涵;6）形成灵活创新网络的方式和途径。     

三峡库区四方碑滑坡稳定性与变形趋势预测

三峡水库建成后,库水位周期性涨落和暴雨产生的渗流作用导致大量古滑坡的复活或新滑坡的发生。以库区近水平层状结构的四方碑滑坡为例,依据库水位实际调动,将水位从175 m至145 m不同降速与50年一遇暴雨进行工况组合,计算4种工况下滑坡的稳定性及破坏概率。然后采用Geo-studio软件的Sigma模块对滑坡进行变形模拟,运用R/S分析方法判断滑坡的变形持续性,并结合野外调查情况,综合评价分析四方碑滑坡的稳定性。结果表明:滑坡在各工况下整体均处于基本稳定状态,具有低危险性;变形模拟结果显示滑坡前缘位移最大,与野外调查情况一致;各监测点Hurst指数均介于0.5~1,表明时间序列具有正持续性,在研究的时间限度内滑坡的局部破坏增强,应在汛期加强对滑坡前缘的巡查和预警。     

山东大尹格庄金矿蚀变岩中矿体分布稳定性的动力学控制参量探讨

元素品位分布的相依性指标--赫斯特指数（Hurst指数）是矿体分布稳定性的动力学控制参量,重标极差（R/S）分析是相依性分析的有效方法.利用R/S分析对胶东大尹格庄金矿黄铁绢英岩内不同勘探线金元素品位系列的Hurst指数计算发现,Hurst指数主要介于0.59至0.89之间,均值为0.75,标准差为0.09,均大于随机行走经验Hurst指数的均值与标准差;计算结果说明元素品位分布存在正相关性,但由于受多种因素影响,其空间分布的相依性具有一定波动.元素品位分布的正相依性显示在特定的地质背景内,矿体连续分布或者间断出现,发育相对稳定,其与大尹格庄金矿的地质事实相吻合.     

近45年5-9月阿勒泰地区强降水气候变化趋势与突变特征

利用1970—2019年内蒙古地区110个国家站降水量资料,采用经验正交函数(EOF）分析、重标极差分析(R/S)和非周期循环分析,统计四季和年降水量时间序列的Hurst指数(H)、分维数(D)和非周期循环的平均循环长度,分析降水量变化趋势和记忆周期。结果表明：(1)内蒙古地区年降水量变化呈增多趋势,其中在东部的偏东地区增多最显著,变化趋势具有持续性特征,持续时间为8 a,但在内蒙古西部的偏南地区和东部的局地区域年降水量呈减少趋势;(2)春季、秋季和冬季年降水量的年代变化呈增多趋势,夏季呈减少趋势,特别是冬季在东部的偏北地区的个别区域Hurst指数H=1,呈现完全预测特征,降水量未来趋势为增多趋势且通过95%的显著性检验;(3)四季降水量过去的增量与未来的增量都呈正相关,夏季降水量减少趋势的持续性最弱,冬季降水量增多趋势的持续性最强,春季、夏季、秋季和冬季的记忆长度分别为8 a、8 a、9 a和10 a。