天体运行轨道的背景介质理论导引与自相似分形测度计算的分维微积分基础

通过讨论天体运行背景介质理论的连续轨道及离散轨道这二个研究方向的基础假设,介绍了天体运行轨道的具体方程形式及理论框架概要;进一步地通过讨论天体运行轨道Binet方程的一般形式及其行星近日点进动角的解,给出了连续轨道理论与Newton理论及Einstein广义相对论的联系与区别;通过讨论天体运行轨道的分维扩展方程,给出了包括太阳系行星、天王星卫星、地球卫星、绕月航天器等在内的离散轨道（稳定性轨道）方程及其预言数据.特别地,作为对天体在较为广泛区域作用曲线的初步探讨推论,指出仅由天体引力难以形成质量密度趋于无穷大的理想黑洞.通过讨论一般函数的分维导数的位置假设及幂函数的分维导数的形式假设,进一步明晰了幂函数的分维导数、分维微分及分维积分的具体方程形式,给出分维导数与分数阶导数的区别,随后讨论了基于一般分形测度的分维微积分形式定义导出的自相似分形的测度计算方程具体形式,给出了其与目前Hausdorff测度方法（覆盖方法）的区别,并对包括三分Cantor集合、Koch曲线、Sierpinski垫片及正交十字星形等自相似分形在内的测度进行了计算分析.     

金矿测年方法讨论及定年中存在的问题

准确的成岩成矿年代测定是矿床研究和对比的基础。然而近几年来 ,不同的研究者对同一矿床采用不同的定年方法得出了相差十分悬殊的成岩成矿年龄的报道屡见不鲜。为此笔者在分析了不同定年方法适用性的同时 ,强调了在金矿定年中要加强对金矿成岩成矿地质背景的研究 ,重视不同地质体与成矿的先后关系 ,确定标志性地质体 ,选择合适的定年方法 ,测定标志性地质体和矿体的成岩成矿年代 ,使成岩成矿年代互为限定 ,得到高质量的年代学数据。     

青海湖地区生态环境动态变化遥感监测

由于青海湖地区的生态环境较为脆弱，且人类活动进一步加剧，人口、资源与环境的矛盾日渐突出，因此，近年来．青海湖及其周边地区的生态环境出现了明显变化，主要表现在水位下降及水域面积减小、草原退化、沙质荒漠化土地面积扩大等。文章采用1975年MSS卫星图像及1987、2000年TM卫星图像作为遥感信息源，并结合地理信息系统方法，旨在查明青海满地区耕地、沙质荒漠化土地和水域等生态环境要素的时空演化规律，为青海湖地区实现资源开发与环境协调发展提供科学依据。监测结果表明，25a来，青海湖地区的耕地及沙质荒漠化土地面积出现明显的扩大，而水域面积出现明显缩小，同时由于湖周各河流土壤侵蚀的加剧，在部分河流入湖处泥沙淤积较为严重，生态环境出现明显恶化。     

Evaluation of bending moments and shear forces at unit connections of very large floating structures using hydroelastic and rigid body analyses

This paper investigates the characteristics of bending moments, shear forces and stresses at unit connections of very large floating structures (VLFS) under wave loads. The responses of VLFS are calculated by solving multi-body motion equation considering hydroelasticity and connection stiffness. Hydroelastic responses are calculated by the direct method. Higher-order boundary element method (HOBEM) is used for fluid analysis and finite element method (FEM) is introduced for structural analysis. The equation of motion is modified to describe the unit connections by employing spring elements. Bending moments and shear forces at the connections are obtained from the dynamic equilibrium condition for pressures and inertia forces. Two types of VLFS units such as tandem arranged units and side-by-side arranged units are considered in the numerical examples. The influences of connection stiffness, wave frequency and heading angle on responses of VLFS are investigated through the numerical examples. Rigid body analysis along with hydroelastic analysis is also carried out in the numerical analysis and comparison of those two approaches is discussed.     

硬质合金钎头胎体表面渗硼强化实验研究

对钎头胎体表面渗硼方法和工艺进行了实验研究,给出了有关工艺参数与方法。它对提高硬质合金钎头胎体表面和耐磨性,延长钎头的使用寿命具有积极的意义。     

抽水对银川台伸缩仪观测资料干扰的探讨与分析

通过对银川台伸缩仪观测资料的综合对比分析,系统地论述了抽水对银川台伸缩仪观测资料的干扰机制,并提出了消除干扰的方法。     

2010—2015年中东北非政局变动中的“政治性民意势力”及其影响

援引批判地缘政治学话语权和地缘政治想象分析方法,在对“民意”“政治性民意”“政治性民意势力”内涵界定的基础上,分析了2010—2015年中东北非地区相关国家政局变动中“政治性民意势力”的形成背景、过程及其影响。结果表明：中东北非国家“政治性民意势力”的形成有着深厚的国内背景和复杂的国际背景;“政治性民意势力”的形成经历了从民意事件客体的呈现,到民众聚集并上升为政治性议题,再到国内外势力借力博弈形成挑动抗议、推动政变的政治力量的过程;“政治性民意势力”形成以后,多行为体借力博弈下,在国别、区域上呈现不同的扩散轨迹和规律;“政治性民意势力”一方面造成了中东北非相关国家的政局变换,另一方面则推动区域地缘政治格局的变迁。这是对民意事件的地缘政治理论解读和分析,是一次较为有意义的尝试。     

Roche volume filling and the dissolution of open star clusters

From direct N‐body simulations we find that the dynamical evolution of star clusters is strongly influenced by the Roche volume filling factor. We present a parameter study of the dissolution of open star clusters with different Roche volume filling factors and different particle numbers. We study both Roche volume underfilling and overfilling models and compare with the Roche volume filling case. We find that in the Roche volume overfilling limit of our simulations two‐body relaxation is no longer the dominant dissolution mechanism but the changing cluster potential. We call this mechanism “mass‐loss driven dissolution” in contrast to “two‐body relaxation driven dissolution” which occurs in the Roche volume underfilling regime. We have measured scaling exponents of the dissolution time with the two‐body relaxation time. In this experimental study we find a decreasing scaling exponent with increasing Roche volume filling factor. The evolution of the escaper number in the Roche volume overfilling limit can be described by a log‐logistic differential equation. We report the finding of a resonance condition which may play a role for the evolution of star clusters and may be calibrated by the main periodic orbit in the large island of retrograde quasiperiodic orbits in the Poincaré surfaces of section. We also report on the existence of a stability curve which may be of relevance with respect to the structure of star clusters. (© 2015 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

A new method for testing pile by sin- gle-impact energy and P-S curve

Introduction Through many year's practices by vast numbers of scientific and technological workers andefforts from all aspects, the dynamic testing method of high-low strain has formally entered intothe technical code of foundation pile test of construction at last (The Industry Standards of thePeople's Republic of China, 2003). The striking mode of the dynamic testing method of high strainis stipulated as hammer in the code, the striking of rocket can also be used. The latter is widely…     

养殖大菱鲆细菌性红体病病原菌的分离与鉴定

从患有红体病的养殖大菱鲆(Scophthalmus maximus)的肌肉中分离得到一株优势菌并记为H1.经人工注射感染证实H1即为引起养殖大菱鲆红体病的病原菌,其半致死量LD50为2.82×105CFU/mL,而低浓度(1.41×103 CFU/mL)没有造成死亡,但注射部位有脓肿现象,注射相同体积1.5%无菌生理盐水的对照组没有明显的症状,注射部位也无异常.革兰氏染色显示该菌为革兰氏阴性,菌体呈杆状,周生鞭毛.综合该菌的形态、常规生理生化特征和API32E鉴定结果,发现H1与迟钝爱德华氏菌的表性特征非常相似,相似率迭到99.9%.在分子水平上对其16SRNA基因序列的测定,同源性分析,结果表明H1与迟钝爱德华氏菌的亲缘关系最近,相似度达到99%.综合上述研究结果,将该菌株初步鉴定为迟钝爱德华氏茵(Edwardsiella tarda).