Design and construction progress of BRIF

A new RIB project, the Beijing Radioactive Ion-beam Facility (BRIF), has been running at CIAE since 2004. In this project, a 100 MeV H-cyclotron, CYCIAE-100, is selected as the driving accelerator providing a 75-100 MeV, 200-500 μA proton beam. An ISOL system employs two stage separators to reach the mass resolution of 20000. Its RIB beam will be injected into the existing Tandem and a superconducting booster installed down stream of the Tandem will increase the energy by 2 MeV/q. The progress of BRIF, giving special emphasis to CYCIAE-100, will be introduced in this paper.     

非对称圆环拍的特性研究

建立微小非对称圆环点冲击下拍的理论模型,通过实验验证其有效性。微小非对称圆环是分析大钟拍现象的简化模型,微小非对称圆环的每一对径向振动模态的固有频率非常接近,这对模态互相干涉下出现拍现象。最后利用拍的理论模型绘制沿圆周拍的分布图,详细分析拍的分布特性,为校正钟的拍频声提供理论依据。     

火箭上面级星敏感器/陀螺组合定姿实时仿真系统

针对运载火箭上面级惯性导航设备提供的姿态信息随时间累积而误差逐渐增大的问题,提出了基于扩展卡尔曼滤波的星敏感器/陀螺组合姿态确定算法,并为加快工程样机研制设计了基于Matlab/dSPACE平台的实时仿真系统。基于地心第二轨道坐标系和上面级体坐标系,给出了姿态角定义,推导了姿态转换矩阵。通过分析组合定姿方案和姿态状态估计方法,设计了基于误差四元数的滤波器;为减少算法的计算量,采用了离线计算次优增益矩阵的方法。进行了星敏感器在回路中的半实物仿真。仿真结果表明组合定姿精度优于50″,且能够准确估计陀螺常值漂移。该算法精度高,速度快,实时仿真系统具有很好的参考和应用价值。     

运动壁面槽道流动的直接数值模拟

采用谱方法,在曲线坐标系下对不可压缩Newton流体的N-S方程进行求解,采用定义在物理空间中的流动物理量以避免使用协变、逆变形式的控制方程．在计算空间采用Fourier-Chebyshev谱方法进行空间离散,时间推进采用高精度时间分裂法．为了减小时间分裂带来的误差,采用了高精度的压力边界条件．与其他求解协变、逆变形式控制方程的谱方法相比,该方法在保持谱精度的同时减小了计算量．首先通过静止波形壁面和行波壁面槽道湍流的直接数值模拟,对该数值方法进行了验证;其次,作为初步应用,利用该方法研究了槽道湍流中周期振动凹坑所产生的流动结构．     

现行电力系统热经济性状态方程

本文用系统工程观点,定义了热力发电厂热经济性系统状态方程。指出,状态方程的结构与系统的结构一一对应,系统的热经济性取决于系统的结构及系统所处热力学状态。该方程的出现为电厂热经济性的计算、分析与综合提供了新的基础和研究方法。     

紫外分光光度法测定维生素B_6

本文建立了以 0 .0 35 mol/ L HAc(醋酸 )为介质 ,采用紫外分光光度法测定维生素 B6的新方法。该方法体系简单 ,操作方便、快速、灵敏 ,其表观摩尔吸光系数ε为 9.37× 10 4 L· mol-1· cm-1。线性范围为0 .61— 4 0 .10μg/ m L。用于 VB6片剂和针剂测定 ,回收率为 10 0 .82 %— 10 1.90 %     

Statistical analysis of Fe abundances gradients in the Galaxy

Using the high precision data of the proper motions and parallaxes from Hipparcos catalogue, we obtained the orbital parameters of 1302 stars in the Galaxy based on the mass distribution model provided by Allen and Santillón. Fe abundances of 1295 stars among our samples were analyzed. With the correlation analyses between [Fe/H] and orbital parameters, we obtained that the Fe gradient is - 0.057 ± 0.007 dex/kpc along the direction of the maximum galactocentric distance (hereafter DG_max) in the range of 8.5 kpc < DG_max < 17 kpc. We also got the result that the vertical gradient is steeper than the radial gradient. Furthermore, we divided the samples into two subgroups: giants and dwarfs; F, G and K stars; and then analyzed them respectively. Our results show that the gradient becomes flatter and flatter from giants to dwarfs, from F type to G and K type stars. We also divided the samples into disk and halo stars using maximum vertical distance Z_max = 1 kpc as the criterion and got the result that the abundances of the disk stars are much higher than that of the halo stars. Our work suggests the existence of the galactic gradient and supports those chemlcal evolution medels which show that the halo was formed before the disk at the early stage of the Galaxy.     

热分析法评价反应性热溶胶的初粘强度

热粘指数;热分析法评价反应性热溶胶的初粘强度     

Analysis of Mitochondrial DNA from the Ancient Tombs of Turfan

IntroductionIn general,inferences aboutpopulation historyare drawn from the studies of genetic diversity incontemporary populations.However,the retrievalof ancient DNA from archaeological remains holdsthe promise to add a temporal component to suchstudies. With the invention of polymerase chairreaction(PCR) ,significant amounts of geneticinformation can be recovered from ancient relic.The analysis of DNA from ancient bones can giveimportant implication for anthropology,archaeology and mole…     

高折射率环氧和环硫型光学树脂的研究进展

环氧树脂;环硫化合物;高折射率环氧和环硫型光学树脂的研究进展