理论地层学先驱 中国地层学的领路人──缅怀老师尹赞勋

本文作者曾在尹赞勋教授指导和关怀下工作２７年,深受老师的谆谆教诲和支持信任,在先生逝世１０周年之际,著文缅怀前辈,以寄托崇敬和感激之情。文章联系中国第四纪研究,通过《地层规范草案及地层规范草案说明书》和《中国地层指南及中国地层指南说明书》的产生,以及工具书的编纂和《中国地层典(七)石炭系》的创编工作,回顾了尹赞勋教授对中国地层学理论和实践所做划时代的卓越贡献,认为他是当之无愧的理论地层学先驱和中国地层学的领路人。     

Nitrogen sulfide in quiescent dark clouds

We report the first detection of interstellar nitrogen sulfide (NS) in cold dark clouds. Several components of the 2 pi 1/2, J = 3/2 --> 1/2 and J = 5/2 --> 3/2 transitions were observed in TMC-1 and L134N. The inferred column density for TMC-1 is NNS approximately 8 x 10(12)cm-2 toward the NH3 peak in that cloud, and in L134N is NNS approximately 3 x 10(12)cm-2 toward the position of peak NH3 emission. These values correspond to fractional abundances relative to molecular hydrogen of fNS approximately 8 x 10(-10) for TMC-1, and fNS approximately 6 x 10(-10) for L134N. The NS emission is extended along the TMC-1 ridge and is also extended in L134N. The measured abundances are significantly higher than those predicted by some recent gas phase ion-molecule models.     

浅论军用土地统计计算机应用系统设计方法问题

本文在解放军土地管理局研制的“军用土地管理信息系统”的基础上,从系统设计和应用的角度出发,明确了系统应包括的基本功能,提出了改进和完善系统的方法。     

Theoretical infrared spectra of some model polycyclic aromatic hydrocarbons: effect of ionization

In order to test the hypothesis of ionized polycyclic aromatic hydrocarbons (PAHs) as possible carriers of the UIR bands, we realized a computational exploration on selected PAHs of small dimension in order to identify which changes ionization would induce on their IR spectra. In this study we performed ab initio calculations of the spectra of neutral and positively ionized naphthalene, anthracene, and pyrene. The results are significantly important. The frequencies in the cations are slightly shifted with respect to the neutral species, but no general conclusion can be reached from the three molecules considered. By contrast, the relative intensities of most vibrations are strongly affected by ionization, leading to a much better agreement between the calculated CH/CC vibration intensity ratios and those deduced from observations.     

西昆仑“玛尔坎苏式”富锰矿主控因素及成矿模式

锰矿是我国战略性紧缺矿种，寻找锰矿尤其是富锰矿是我国地质工作者的迫切任务。在西昆仑造山带的西北段玛尔坎苏地区石炭纪沉积岩系中探明的大型碳酸锰成矿带，是我国近年最重要的富锰矿找矿新发现。然而，目前对该富锰矿带的成矿主要控制因素、形成机制及展布规律等地质问题的认识尚不深入，严重制约了该矿带深部及外围进一步找矿预测工作。本文从成矿地质背景入手，以典型锰矿床地质和地球化学特征的剖析为切入点，通过对比研究国内外典型锰矿的成矿特征，总结出西昆仑玛尔坎苏富锰矿带的控制因素主要包括伸展型边缘盆地、丰富多源的锰质来源、海洋氧化—还原界面的变化、有机质深度参与成岩成矿过程等；初步建立了“玛尔坎苏式”富锰矿的成矿模式，并提出了需要进一步研究的科学问题，这对丰富锰矿成矿理论及进一步找矿预测具有重要意义。     

早期矿业发展与地质学的诞生

石头是人类由蒙昧走向智慧的启蒙，彩石和矿物颜料开启了人类对美的认识和追求。人类在使用矿物岩石中相继出现的武器、农耕时代、陶器、金属冶炼、人类聚落和城邦，标志着人类智慧的爆发和文明根基的建立。遍布全球的规模性采掘和矿业活动为早期人类社会的发展奠定了工业和经济基础，给人类认识矿物岩石和探索地球的奥秘打开了大门。东西方先哲们最早观察和思索天地万物、物质组成和变化、探索石头和金属的形成，炼丹术和炼金术、早期博物学、早期医学对金属、矿物和岩石的进一步探索与实践，孕育了现代矿物学和地质学。中世纪矿业的繁荣带动了地质科学研究的复兴，矿床学和矿物学的确立、化石研究与地层层序的确立、岩石成因的水火之争、山脉成因的垂向升降和水平挤压之争导致了地质学的诞生和确立。     

在应用计算机解释印度拉贾斯坦邦西部贾伊萨梅尔地区比尔马尼亚盆地地质特征中地质数据的分析

最近十年来研究的地质数据包括比尔马尼亚盆地岩相的地层、岩性、岩石、粒度和地球化学资料。这些数据已进入专用的“Ｆｏｘｓｅｄｂａ”数据表以建立比尔马尼亚盆地的数据总库。采用Ｈａｒｗａｒｄ制图法在ｘ－ｙ轴（粒度参数和地球化学数据）上作图。该盆地各种岩相的环境解释模式都配备有“图象”软件。最后,上述资料被用来解释所推断的比尔马尼亚盆地各种岩相的沉积环境。该盆地的沉积充填物含硅质碎屑、碳酸盐和磷块岩相的混合组合,指示变幻不定的沉积环境,即有若干具间歇海进事件的沉积海退事件。结果,磷块岩主要形成一种浅水正化学沉积和异化学沉积的复杂组合。     

华亭煤产地含煤岩系成因地层分析及主煤层成因

本文以成因地层分析理论、盆地分析理论为指导,参照地震地层学思路,重新厘定了华亭煤产地地层划分与对比,探讨了富县组、延安组沉积环境,结合煤岩学特征阐述了华亭煤产地巨厚煤层是由“填积型”煤层、“退积型”煤层叠加形成的。     

Numerical simulation of the general circulation of the atmosphere of Titan

The atmospheric circulation of Titan is investigated with a general circulation model. The representation of the large-scale dynamics is based on a grid point model developed and used at Laboratoire de Météorologie Dynamique for climate studies. The code also includes an accurate representation of radiative heating and cooling by molecular gases and haze as well as a parametrization of the vertical turbulent mixing of momentum and potential temperature. Long-term simulations of the atmospheric circulation are presented. Starting from a state of rest, the model spontaneously produces a strong superrotation with prograde equatorial winds (i.e., in the same sense as the assumed rotation of the solid body) increasing from the surface to reach 100 m sec-1 near the 1-mbar pressure level. Those equatorial winds are in very good agreement with some indirect observations, especially those of the 1989 occultation of Star 28-Sgr by Titan. On the other hand, the model simulates latitudinal temperature contrasts in the stratosphere that are significantly weaker than those observed by Voyager 1 which, we suggest, may be partly due to the nonrepresentation of the spatial and temporal variations of the abundances of molecular species and haze. We present diagnostics of the simulated atmospheric circulation underlying the importance of the seasonal cycle and a tentative explanation for the creation and maintenance of the atmospheric superrotation based on a careful angular momentum budget.     

黄海北部长山群岛海洋农牧化分区探讨

本文采用主成分-聚类分析等定量方法,并通过对长山群岛海域的资源、环境、生产条件等的相似性和差异性分析,将其划分为三个海洋农牧化区域,为海水养殖业的合理布局提供科学依据。