三维旋转式自动进样器的研制

介绍了自行研制的三维旋转式自动进样器的结构和特点，提出了三维模式、气动升降臂、旋转定位的自动进样器解决方案，并成功地用于自动进样器的研制。文章中给出了三维旋转式自动进样器的组成，气动式升降臂控制原理和系统的软件流程。     

深海采矿转臂机构采矿姿态优化研究

针对海底地形不平坦特性,提出了一种变幅机构来自适应海底地形采矿姿态的采矿机构。综合考虑采矿机构采掘头距海底高度对采矿率影响,利用关键点法建立了节臂上的点到海底地形距离的数学模型。在此基础上,建立了以采矿率最高为目标的最优采矿姿态数学模型。以某实际地形为例,采用模拟退火遗传算法优化求解最优采矿姿态。根据其优化后结果可知,其最优采矿姿态与海底地形坡度变化一致,从而证明了采矿姿态模型的正确性。     

两维银河系旋臂对比度

为改善文献上惯用的表现银河系分子谱线巡视结果的完全平滑了方位信息的径向分布方法,我们发展了原子气体或分子云参量的分环银经分布图,(X—l)_i图,它在某种程度上给出了方位信息。用现存旋臂模型结合这种图我们得到的银道面旋臂区和臂间区的E(HI),E(CO),E(~(13)CO)和N/S(~(13)CO)的两维对比度约为1—2。     

浮式油气生产储卸装置风倾力臂解析解及相关线性关系研究

为了建立驳船型浮式生产储卸装置的风倾力臂和船型参数之间的函数关系,构造了与其主尺度及设计工况对应吃水、排水量和正浮状态侧向所受风倾力臂相关的3个无因次量——"相对力臂"、"相对排水量"和"相对吃水",使前二者的乘积与相对吃水呈现出线性变化关系,通过拟合直线得到风倾力臂的解析解,其有效性经6艘我国现役FPSO的设计数据和理论分析验证,结果理想。     

Some statistical properties of spiral galaxies along the Hubble sequence

A statistical study has been made for the variations along the Hubble sequence, os such parameters as the degree of tightness of winding of spiral arm λ, the pitch angle μ, the flatness of the disk H/D₂₅ and the thickness H along the Hubble sequence for 365 spiral galaxies published in A&Ap Supplement Series. The mean values of these quantities for the various Hubble types have been obtained for the first time. The results of the statistics show clearly 1) that the Hubble classification of spiral galaxies is one which has only a qualitative and statistical significance, and 2) that the dispersion relation in the density wave theory is valid for most spiral galaxies, i.e., the arms of most spiral galaxies satisfy the requirements of being tightly wound.     

旋涡星系随Hubble序列的一些统计性质

对发表在Ａ＆ＡｐＳｕｐｐｌｅｍｅｎｔ Ｓｅｒｉｅｓ上３６５个旋涡星系的一些参数（如表示旋臂缠卷松紧程度的参数Λ、切向角ｕ、盘的扁度Ｈ／Ｄ２５以及厚度等）随Ｈｕｂｂｌｅ序列变化的关系进行了统计研究。首次得到这些参量的平均值;并且从统计结果可以明显地看到Ｈｕｂｂｌｅ对旋涡星系的分类只是一种定性的、只有统计意义上的分类;另外,从我们的统计结果看,密度波理论的色散关系对大多数旋涡星系是成立的,即大多数旋涡     

Numerical and Experimental Study of the 3D Effect on Connecting Arm of Vertical Axis Tidal Current Turbine

Vertical axis tidal current turbine is a promising device to extract energy from ocean current. One of the important components of the turbine is the connecting arm, which can bring about a significant effect on the pressure distribution along the span of the turbine blade, herein we call it 3D effect. However, so far the effect is rarely reported in the research, moreover, in numerical simulation. In the present study, a 3D numerical model of the turbine with the connecting arm was developed by using FLUENT software compiling the UDF (User Defined Function) command. The simulation results show that the pressure distribution along the span of blade with the connecting arm model is significantly different from those without the connecting arm. To facilitate the validation of numerical model, the laboratory experiment has been carried out by using three different types of NACA aerofoil connecting arm and circle section connecting arm. And results show that the turbine with NACA0012 connecting arm has the best start-up performance which is 0.346 m/s and the peak point of power conversion coefficient is around 0.33. A further study has been performed and a conclusion is drawn that the aerofoil and thickness of connecting arm are the most important factors on the power conversion coefficient of the vertical axis tidal current turbine.     

基于数据手套和跟踪器的虚拟手臂建模

文中利用数据手套和跟踪器获取手臂各关节运动数据,根据关节运动限制对所获取数据进行处理,建立了符合人体运动规律的虚拟手臂数学模型,实现了虚拟环境中与试验者的手臂同步运动、效果逼真的虚拟手臂模型.     

应用随机方法研究全球气候变暖对东江流域水资源的影响

介绍了全球气候变暖对流域水资源影响研究中流域随机模型的应用.根据IPCC最新公布的2010～2039年和2040～2069年气候变化情景的GCMs模拟结果,计算并讨论了广东东江流域未来相应期内不同保证率径流量可能发生的变化.     

旋涡星系随uUbble序列的一些统计性质

对发表在A＆Ap Supplement Series上的365个旋涡星系的一些参数(如表示旋臂缠卷松紧程度的参数A、切向角μ、盘的扁度H／D25以及厚度等)随Hubble序列变化的关系进行了统计研究．首次得到这些参量的平均值;并且从统计结果可以明显地看到Hubble对旋涡星系的分类只是一种定性的、只有统计意义上的分类;另外,从我们的统计结果看,密度波理论的色散关系对大多数旋涡星系是成立的,即大多数旋涡星系的旋臂满足紧卷螺旋波的要求．