沉积盆地异常低压(负压)与油气分布

在沉积盆地油气勘探过程中,异常压力与油气聚集的关系愈显密切,而异常压力不仅仅是指异常高压,国内外在发现许多异常高压油气藏的同时,也发现了相当数量的异常低压油气藏,而且异常低压在世界许多盆地中均有分布.因此,深入研究异常低压的形成机理及与油气分布的关系,同样重要和不容忽视.本文介绍了异常低压的概念、特征和分类,详细分析了异常低压的形成机制:地层剥蚀卸载后的弹性回返(反弹)作用、流体的供排不平衡、轻烃的扩散作用、断裂和不整合面的压力释放作用、渗透作用和温度变化等;最后论述了异常低压与油气分布的关系.     

基于性能的结构抗风设计理论框架

提出了基于性能的结构抗风设计理论框架,将风压强度划分为4个设计风压等级（弱风压、中风压、强风压及超强风压）,将人体振动舒适度划分为6个等级（无振感、轻微振感、中等振感、烦恼、非常烦恼和无法忍受）、三种振动水平（与人的舒适感相关的振动水平、与人正常工作和操作有关的振动水平、与人的生理健康直接相关的振动水平）。结合不同类别建筑物的性能需求及人体振动舒适度的要求,将结构风振性能水准划分为4种状态（性能健康、性能亚健康、性能病态及性能丧失）,将结构风振性能目标划分为5个等级（A、B、C、D、E）。提出了结构抗风概念设计与计算分析的一般原则,给出了结构性能抗风安全性评价及社会经济评价基本内容的建议。     

斜坡降雨入渗在Flac中模拟

为了简化分析,在模拟斜坡降雨入渗暂态渗流时,通常没有考虑入渗和产流的耦合过程,通过施加流量边界或零水头边界进行地下水渗流计算,通过在FALC中利用内嵌的fish语言,考虑地表径流和地下渗流的耦合以及雨向影响下斜坡降雨入渗过程,并通过算例分析了考虑和不考虑耦合、对斜坡孔隙水压力分布以及考虑各种雨向作用下对坡面积水深度的影响。     

提高钻孔桩桩底压浆工效及保证质量的技术措施

钻孔桩桩底压浆技术是向钻孔灌注桩桩底沉渣和围岩土体内压入一定量水泥浆,使桩底沉渣和桩底一定范围土体孔隙内充满水泥浆液,经物理、化学作用使其强度大幅提高,从而实现单桩竖向承载力的提高。结合高铁钻孔桩桩底压浆施工实践,介绍了2种压浆工艺过程,阐明了提高压浆工效、保证注浆质量关键技术措施实施的重要性。     

Long-periodic and secular perturbations to the orbits of Explorer 19 and Lageos due to direct solar radiation pressure

A theory for the long-term variations in the orbit of a spherically symmetric satellite due to direct solar radiation pressure is tested using two satellite orbit analyses. The first of these analyses is in terms of mean elements for the balloon satellite Explorer 19. The results are compared with the expected theoretical variations with short-period terms omitted. The second analysis utilises satellite laser ranging observations of the geodetic satellite, Lageos. A novel long-term analysis technique is developed primarily for laser ranging studies. The technique is tested along with the solar radiation pressure perturbation theory by comparing the results from the theory and the analysis.     

Dynamics of Mars-orbiting dust: Effects of light pressure and planetary oblateness

This paper deals with dynamics of impact ejecta from Phobos and Deimos initially on near-circular equatorial orbits around Mars. For particles emitted in a wide size regime of 1 micron and greater, and taking into account the typical particle lifetimes to be less than 100 years, the motion is governed by two perturbing forces: solar radiation pressure and influence of Mars' oblateness. The equations of motion of particles in Lagrangian non-singular elements are deduced and solved, both analytically and numerically, for different-sized ejecta. We state that the coupled effect of both forces above is essential so that on no account can the oblateness of Mars are be neglected. The dynamics of grains prove to be quite different for the ejecta of Phobos and Deimos. For Deimos, the qualitative results are relatively simple and imply oscillations of eccentricity and long-term variations of orbital inclination, with amplitudes and periods both depending on grain size. For Phobos, the dynamics are shown to be much more complicated, and we discuss it in detail. We have found an intriguous peculiar behavior of debris near 300 µm in size. Another finding is that almost all the Phobos ejecta with radii less than 30 µm (against the values of 5 to 20 µm adopted earlier by many authors) should be rapidly lost by collisions with martian surface. The results of the paper may be the base for constructing an improved model of dust belts that presumably exist around Mars.     

Thermal conduction between an accretion disc and a corona in active galactic nuclei: vertical structure of the transition layer

We study the vertical structure of the transition layer between an accretion disc and a corona in the context of the existence of a two-phase medium in thermally unstable regions. The disc is illuminated by hard X-ray radiation, and satisfies the condition of hydrostatic equilibrium. We take into account the energy exchange between the hot, Compton-heated corona (∼10⁸ K) and cool disc (∼10⁴ K) arising from both radiative processes and thermal conduction. In the case including thermal conduction, we perform a local stability analysis, and conclude that thermal conduction does not suppress thermal instability. In spite of the continuous temperature profile T ( τ ) there are regions of strong temperature gradient, in which spontaneous perturbations can lead to cloud condensation in the transition layer. We determine the minimum size λ _TC of such a perturbation.     

压力分散型预应力锚索张拉试验及应力损失探讨

以某边坡工程压力分散型预预应力锚索的张拉试验为基础,介绍了压力分散型预应力锚索工作机理及张拉试验过程,并对应力损失、预应力筋的伸长量及桩身变形进行分析和初步探讨。     

铣削斜楔形区域形成及其对流场负压区的影响规律

【目的】研究在内喷淋冷却高速铣孔加工中,铣削斜楔形区域的形成对流场负压区的影响。【方法】对高速湿式铣削加工区域建立三维流场模型,应用计算流体力学软件Fluent,采用非结构化四面体网格单元,利用滑移网格技术对高速铣削过程进行三维瞬态计算。【结果】得到不同刃数、不同转速的立铣刀对同一孔径工件进行切削时流场的压力分布情况。三刃立铣刀斜楔形对流场负压影响最大,当立铣刀刃数增加时,此斜楔形区缩小,负压减小,转速为10 000～20 000 r/min时增长速度逐渐降低,20 000～35 000 r/min时增长速度逐渐增高。【结论】从流场角度分析,流场中最大负压值与转速呈正相关,转速的提高增加了抑制空化的难度;增加铣刀刃数,可减小流场斜楔形区面积,减小空化可能。