Wave diffraction and near-trapping by a multi-column gravity-based structure

This paper is concerned with the diffraction of water waves by offshore structures, with the ultimate aim of proposing tools for guiding airgap design. The diffraction of monochromatic waves by an array of four bottom mounted cylinders and a gravity-based structure is studied in detail using linear and second order theory. The phenomenon of near-trapping is investigated, allowing guidelines for airgap design to be established. When contemplating airgap design, however, it is crucially important that consideration is given to the largest waves in a sea state. Therefore, in this study a design wave, called NewWave, is proposed as a realistic model for large ocean waves and is used as the incident wave field in the wave-structure diffraction analysis.     

基于短波红外技术的西藏多龙矿集区铁格隆南矿床荣那矿段及其外围蚀变填图-勘查模型构建

采用短波红外技术测量西藏多龙矿集区铁格隆南矿区地表岩石样本,发现蚀变矿物主要有绢云母和绿泥石,并在地表形成了一套从绢英岩化带-青磐岩化带的具有斑岩特点的蚀变矿物组合特征。通过测量地下ZK0804,ZK1604,ZK2404,ZK3204四个钻孔岩心的短波红外特征,发现钻孔岩心中存在大量明矾石、高岭石、地开石和绢云母,在东西向展布的过程中,绢云母数量及厚度明显增大,有继续向下延伸的趋势,说明矿体向深部逐渐从富含明矾石、地开石、高岭石的高硫、低温类型的矿物组合向绢英岩化带转变,并构成了规律的蚀变分带系统。根据地表、地下岩（矿）石的短波红外光谱特征及蚀变矿物分布趋势,构建了基于短波红外勘查技术的多龙矿集区斑岩-高硫浅成低温热液型铜（金）矿床找矿勘查模型,总结了从钾化带-绢英岩化带-泥化带-高级泥化带（明矾石-地开石-高岭石组合）-青磐岩化带的一套完整蚀变矿物组合及光谱特征。     

港口工程对粉砂淤泥质岸滩的影响

渤海湾西南岸粉砂淤泥质海岸处于岸滩蚀退状态,利用ECOMSED数值模拟方法,分析了港口工程建设对水动力和海底蚀淤的影响。研究结果表明,近岸海域-2 m等深线以内以侵蚀为主,侵蚀速率一般小于10 cm/a;-2~-6 m等深线以淤积为主,淤积速率一般在10 cm/a以下,局部大于20 cm/a,-6 m等深线侵蚀速率小于10 cm/a。黄骅港导沙堤建设后淤积区整体向海扩展,延伸至约-8 m等深线,面积增加约5.4%;航道最大淤积速率由61.9 cm/a减小为46.8 cm/a;导沙堤堤头受挑流作用冲刷速率达到29.7~30.2 cm/a。     

Theoretical ion densities in the lower ionosphere

We have solved the coupled momentum and continuity equations for NO⁺, O₂⁺, and O⁺ions in the E- and F-regions of the ionosphere. This theoretical model has enabled us to examine the relative importance of various processes that affect molecular ion densities. We find that transport processes are not important during the day; the molecular ions are in chemical equilibrium at all altitudes. At night, however, both diffusion and vertical drifts induced by winds or electric fields are important in determining molecular ion densities below about 200 km. Molecular ion densities are insensitive to the O⁺ density distribution and so are little affected by decay of the nocturnal F-region or by processes, such as a protonospheric flux, that retard this decay. The O⁺ density profile, on the other hand, is insensitive to molecular ion densities, although the O⁺ diffusion equation is formally coupled to molecular ion densities by the polarization electrostatic field. Nitric oxide plays an important role in determining the NO⁺ to O₂⁺ ratio in the E-region, particularly at night. Nocturnal sources of ionization are required to maintain the E-region through the night. Vertical velocities induced by expansion and contraction of the neutral atmosphere are too small to affect ion densities at any altitude.     

单一地层平台插桩地基土破坏模式及插桩深度有限元分析

自升式平台插桩是地基土在桩靴荷载作用下发生连续塑性破坏的过程,当地基极限承载力等于桩靴荷载时插桩完成。经典土力学极限承载力理论对土体潜在滑动面做了假设,无法有效分析土体内部的破坏过程。因而,研究采用有限元极限分析法对单一地层中插桩时地基土渐进破坏过程进行了模拟,并与Skempton、Terzaghi公式计算的极限承载力进行了对比,取得了较为一致的结果,同时对插桩深度进行了预测。     

极区冰基拖曳式海洋剖面浮标系统低功耗设计与实现

针对极区冰基拖曳式海洋剖面浮标长期稳定获取极区水文和气象数据的工作需求,进行了浮标系统的低功耗方案设计。该方案基于超低功耗51系列微处理器,根据最低功耗工作模式与最短工作时间原则,采用高效的电源管理机制对浮标系统各个部分的能量消耗进行合理的分配与管理,并应用了Argos卫星通讯模块ARGOS-3 PMT-RFM的BPSK调制低速数据传输模式,可有效降低浮标系统的整体能耗。该浮标在北极冰站上长达1年的运行情况表明该系统工作稳定,所采用的低功耗能量管理方案实现了浮标系统长期连续观测的需求。该浮标的成功试验和推广应用有助于极地研究人员更准确地分析海冰变化过程。     

HST colour–magnitude diagrams of six old globular clusters in the LMC

We report on HST observations of six candidate old globular clusters in the Large Magellanic Cloud (LMC): NGC 1754, 1835, 1898, 1916, 2005 and 2019. Deep exposures with the F555W and F814W filters provide us with colour–magnitude diagrams that reach to an apparent magnitude in V of ∼25, well below the main-sequence turn-off. These particular clusters are associated with significantly high LMC field star densities and care was taken to subtract the field stars from the cluster colour–magnitude diagrams accurately. In two cases there is significant variable reddening across at least part of the image, but only for NGC 1916 does the differential reddening preclude accurate measurements of the CMD characteristics. The morphologies of the colour–magnitude diagrams match well those of Galactic globular clusters of similar metallicity. All six have well-developed horizontal branches, while four clearly have stars on both sides of the RR Lyrae gap. The abundances obtained from measurements of the height of the red giant branch above the level of the horizontal branch are 0.3 dex higher, on average, than previously measured spectroscopic abundances. Detailed comparisons with Galactic globular cluster fiducials show that all six clusters are old objects, very similar in age to classical Galactic globulars such as M5, with little age spread among the clusters. This result is consistent with ages derived by measuring the magnitude difference between the horizontal branch and main-sequence turn-off. We also find a similar chronology by comparing the horizontal branch morphologies and abundances with the horizontal branch evolutionary tracks of Lee, Demarque &38; Zinn. Our results imply that the LMC formed at the same time as the Milky Way Galaxy.     

On the stability of close binaries in hierarchical three-body systems

The Hill-type stability (cf. closure of the zero-velocity curves in the circular restricted three-body problem) of general hierarchical three-body systems is examined analytically in the case where the total mass of the binary is small in comparison to the mass of the external body (e.g. systems of the type Planet-Satellite-Sun, Planet-Planet-Star, etc.). This is compared with results derived by Szebehely, Markellos and Roy in the Planet-Satellite-Sun case of the circular restricted three-body problem. It is demonstrated how the Hill-type stability is affected by the sense of revolution of the binary, i.e. corotational or contrarotational, and the mass ratio within the binary. The effect of the difference in longitudes of the bodies in their orbits is also examined.