C~n中Dirichlet型空间和Bloch型空间上的加权Cesàro算子

本文在Cn中单位球上讨论了Dirichlet型空间Dp,Bloch型空间βp以及Lipschitz空间Ap上加权Cesaro算子Tg的有界性和紧性.得到当P<0,q≤P 2或P>n,q≤P 2时,Tg是Dp到Dq的有界算子或紧算子的充要条件;对所有的P,q,获得了Tg是βp到βq之有界算子和紧算子的充要条件及Tg是β0p到β0q之有界算子的充要条件等.     

氯苯的同步辐射光电离研究

利用真空紫外同步辐射和反射式飞行时间质谱仪对氯苯进行了光电离研究,通过测量各离子的光电离效率(PIE)曲线,得到了氯苯的电离势为(9.11±0.05)eV及两种主要碎片离子C6H+5和C4H+3的出现势分别为(12.96±0.05)和(16.27±0.05)eV.结合有关文献的热力学数据,推导出C6H5Cl+、C6H+5及C4H+3的离子生成焓及一些键的解离能.实验获得了118.0nm同步辐射光电离下氯苯的质谱图.     

垂直上升管内非牛顿流体流动沸腾的壁温工况和临界热负荷

本文研究了一种非牛顿流体-高聚物水溶液在垂直上升管内强制流动沸腾过程中的壁温沿管长变化及临界热负荷的特点，并考察了高聚物种类、浓度、质量流速等对临界热负荷和壁温工况的影响。     

Numerical solutions of general-relativistic field equations for rapidly rotating neutron stars

Stationary axial symmetric equilibrium configurations rapidly rotating with uniform angular velocity in the framework of general relativity are considered. Sequences of models are numerically computed by means of a computer code that solves the full Einstein equations exactly. This code employs Neugebauer’s minimal surface formalism, where the field equations are equivalent to two-dimensional minimal surface equations for 4 metric potentials. The calculations are based upon 10 different equations of state. Results of various structures of neutron stars and the rotational effects on stellar structures and properties are reported. Finally some limits to equations of state of neutron stars and the stability for rapidly rotating relativistic neutron stars are discussed.     

用数字干涉仪测量变形镜影响函数的实验研究

分析了变形反射镜面形影响函数的意义，鉴于自适应光学系统中波前探测大都以测量波前斜率为基础的特点，提出应研究斜率影响函数，并在此基础上构成波前复原矩阵。还介绍了用数字干涉仪测量变形镜影响函数的方法和结果，并对测量结果进行了分析，得到了影响函数的各种参数，例如：交连值，高斯指数，特征宽度等。并将干涉法测量斜率影响函数的结果与实际的哈特探测器的测试结果进行了比较。     

卧式螺旋管内油－气两相流流型的研究

本文在两种不同尺寸的卧式螺旋管内进行了油－气两相流流型的实验研究，得到了流型图，并对各种流型之间的转变机理进行了讨论和分析，同时给出了各流型之间转变的准则关系式。     

Weighted composition operators between μ -bloch spaces on the unit ball

In this paper, necessary and sufficient conditions are given for the weighted composition operator T _ψ,φ to be bounded or compact from the space β_μ to β_υ (or β_μ,0 to β _υ,0)on the unit ball of C ^rn. At the same time, a series of corollaries are also obtained.     

37-element solar adaptive optics for 26-cm solar fine structure telescope at Yunnan Astronomical Observatory

A 37-element solar adaptive optics （AO） system was built and installed at the 26-cm solar fine structure telescope of Yunnan Astronomical Observatory. The AO system is composed of a fine tracking loop with a tip/tilt mirror and a correlation tracker, a high-order correction loop with a 37-element deformable mirror, a correlating Shack-Hartmann wavefront sensor based on the absolute difference algorithm, and a real time controller. The system was completed on Sep. 28, 2009 and was used to obtain AO-corrected high-resolution solar images. The contrast and resolution of the images are clearly improved after wavefront correction by AO. To the best of out knowledge, this system is the first solar AO system in China.