球壳开孔加强的应力分析

本文采用有限元数值解法,对某水下结构内部球面隔壁开孔加强区,在均匀压力作用下的应力状态进行计算分析,力学模型由截顶锥壳单元组成,用作者研制的球壳开孔应力分析专用程序计算。本文给出了球壳开孔区的应力及其分布,与解析解和试验值额为吻合。本文还就孔口加厚板的厚度、宽度等结构参数的变化对应力集中系数的影响,进行了系列计算和分析,给出了相应曲线,可供设计者使用和参考。本文所介绍的方法使用简便,计算效率高,有实用价值。     

自升式海上钻井平台结构的模态分析及地震反应的谱分析

本文对某自升式钻井平台结构进行了模态和地震反应分析。用等效桩腿的处理方法把平台结构简化为空间梁系有限元力学模型,采用我国《海上固定平台入级与建造规范》中规定的标准地震谱曲线.首先计算了平台结构前五阶固有频率和模态,然后用基于模态叠加法的谱分析法求出平台结构和桩腿各部位的最大位移和应力反应。最后给出了该平台结构在30m和50m水深海域、桩腿为插桩式和沉垫式两种固定型式下的计算结果和比较。     

文昌鱼精子发生过程中的超微结构研究

本文在超微结构水平上研究文昌鱼(Branchiostoma belcheri Gray)精子发生过程中细胞形态结构的变化和细胞器的演变规律。观察到精细胞核形态变化的特点、线粒体的演变及其原始结构形式。同时,也观察到精细胞变态过程中高尔基体的演变、顶体的形成及超微结构的特点和微管的重组。此外,我们还首次观察到尾丝外膜上有特殊的刺状结构。对以上观察结果,进行了讨论。     

Impact-generated atmospheres over Titan, Ganymede, and Callisto

The competition between impact erosion and impact supply of volatiles to planetary atmospheres can determine whether a planet or satellite accumulates an atmosphere. In the absence of other processes (e.g., outgassing), we find either that a planetary atmosphere should be thick, or that there should be no atmosphere at all. The boundary between the two extreme cases is set by the mass and velocity distributions and intrinsic volatile content of the impactors. We apply our model specifically to Titan, Callisto, and Ganymede. The impacting population is identified with comets, either in the form of stray Uranus-Neptune planetesimals or as dislodged Kuiper belt comets. Systematically lower impact velocities on Titan allow it to retain a thick atmosphere, while Callisto and Ganymede get nothing. Titan's atmosphere may therefore be an expression of a late-accreting, volatile-rich veneer. An impact origin for Titan's atmosphere naturally accounts for the high D/H ratio it shares with Earth, the carbonaceous meteorites, and Halley. It also accounts for the general similarity of Titan's atmosphere to those of Triton and Pluto, which is otherwise puzzling in view of the radically different histories and bulk compositions of these objects.     

基于矿物学方法评价浙江省土壤中Pb污染状况

利用土壤重金属元素环境质量矿物学评价方法,对淅江省全境土壤中不同土壤类型(或亚类)表层、不同母质表层和剖面中的Pb进行环境质量评价的结果表明,土壤中Pb的实测量和土壤对Pb的固持量决定了土壤中Pb的环境质量,浙江省土壤中Pb的污染度有正负值,说明土壤中的Pb对有些地区产生了污染,而对有些地区则没有产生污染.研究结果揭示,土壤矿物对Pb具有一定的固定与容纳能力,超过其固定与容纳能力,土壤中的Pb会对环境造成污染.这一旨在揭示土壤中重金属元素与各种矿物之间环境平衡关系的方法,可为评价土壤环境质量提供科学依据和技术支撑.     

Will the Russians return from the near abroad?

The author "examines a range of issues surrounding the involuntary migration of Russian populations from the non-Russian republics of the former USSR. Among the questions addressed are possible magnitudes of in-migration into Russia (with special attention paid to conditions in one of the major source regions, Central Asia), attitudes in Russia regarding appropriate policy with respect to treatment of co-nationals in the near abroad and whether their return to Russia would have a positive or negative impact, and conditions in areas of Russia that presently are absorbing the greatest numbers of migrants. The assertion that Russian policy should seek aggressively to prevent the out-migration of Russian populations [from] the near abroad is assessed critically."     

Coupled atmosphere-ocean models of Titan's past

We have developed a coupled atmosphere and ocean model of Titan's surface. The atmospheric model is a 1-D spectrally-resolved radiative-convective model. The ocean thermodynamics are based upon solution theory. The ocean, initially composed of CH4, becomes progressively enriched in ethane over time. The partial pressures of N2 and CH4 in the atmosphere are dependent on the ocean temperature and composition. We find that the resulting system is stable against a runaway greenhouse. Accounting for the decreased solar luminosity, we find that Titan's surface temperature was about 20 K colder 4 Gyr ago. Without an ocean, but only small CH4 lakes, the temperature change is 12 K. In both cases we find that the surface of Titan may have been ice covered about 3 Gyr ago. In the lakes case condensation of N2 provides the ice, whereas in the ocean case the ocean freezes. The dominant factor influencing the evolution of Titan's surface temperature is the change in the solar constant--amplified, if an ocean is present, by the temperature dependence of the solubility of N2. Accretional heating can dramatically alter the surface temperature; a surface thermal flux of 500 erg cm-2 sec-1, representative of small levels of accretional heating, results in a approximately 20 K change in surface temperatures.     

海南岛东南海岸带景观生态规划

对海南岛东南海岸带进行了景观生态规划。根据海南岛东南海岸带的自然资源条件与经济运行特点，将研究区划分为4个生态区：近岸热带海洋旅游区；海水养殖区；海岸平原粮牧生态区；生态林业区。各区的生态与社会经济特征不同，在利用与管理各生态区的过程中应该采取不同的对策措施，即加强宣传教育与宏观管理，以重点项目建设为契机，加快生态经济建设，优化生态经济结构。建立生物多样性管护区。     

江西彭山锡多金属矿田地质地球化学特征研究

彭山锡多金属矿田位于长江中下游的九瑞地区，是近年来发现的一个以富锡、铅、锌矿产为主的大型矿田。以黑云母二长花岗岩与二云母碱长化岗岩组成的彭山隐伏岩体为中心，各类金属矿床呈“晕圈式”分布。矿床的形成分为2个成矿期共7个阶段，通过对彭山岩体、典型矿床及围岩中的硫同位素、铅同位素、包裹体及稀土资料进行分析，反映出燕山晚期钙碱性花岗岩体的缦位与多金属矿床的形成有着密切的联系，岩浆活动为本区提供了大量的成矿物质。     

青海气候条件对牧草再生性影响的研究

选取1994～2001年河南、甘德两站牧草再生草资料及同期气象资料，通过分析同一地区不同时期及同一时期不同地区气候条件对牧草再生性的影响，建立了牧草再生草产量气候模式，讨论了再生草增、减产的气候条件。研究得出：同一地区不同时期和同一时期不同地区因气候条件不同，割草不一定能增产。