正弦高斯涡旋光束的远场传输特性

根据角谱法和稳相法,推导了正弦高斯涡旋光束TE波和TM波在远场传输和能流密度的解析表达式,研究了正弦高斯涡旋光束在远场中的相位奇点和能流密度分布.结果表明:正弦高斯涡旋光束的远场特性与高斯光束的束腰宽度、涡旋离轴量、坐标位置以及与正弦项相关的参量有关.在一定条件下,远场中会出现相位奇点和能流密度黑核;当控制参量改变时,相位奇点和黑核的位置会发生移动,但原点处不受影响.相位奇点和能流密度的对称性主要受涡旋离轴量影响,当涡旋离轴量为0时,相位奇点和能流密度分布关于原点对称;当涡旋离轴量改变时,相位奇点和能流密度分布呈现出非对称性.     

Study on the spatial coherence of vortex Gaussian beams passed atmospheric turbulence

In this paper, the spectral degree of coherence formula was derived by using the generalized Huygens–Fresnel principle and the method of Rytov phase structure function quadratic approximation. The spatial coherence of vortex Gaussian beams passed atmospheric turbulence was studied. It showed that the spatial coherence was mainly affected by the coherence of light source, the number of topological charges and the transmission distance. The distance of transmission was farther, the spatial coherence of beam was better. The number of topological charges were more, the spatial coherence of beam was better. In a certain transmission distance, the coherence of light source was better, the spatial coherence of beam was worse. In addition, there were coherent vortexes which spectral degree of coherence was zero after the partially coherent vortex beams getting through atmospheric turbulence transmission.     

基于涡旋光束的超快速角向集束匀滑方案

针对惯性约束聚变装置对激光集束辐照均匀性的需求,提出了一种基于涡旋光束的超快速角向匀滑方案,即利用螺旋相位板使2×2集束中的两子束由超高斯光束变换为涡旋光束,而其余两子束不变,进而通过对子束偏振态和中心波长的调控,使集束中的涡旋光束和超高斯光束在靶面两两相干叠加.相干叠加后的焦斑以皮秒量级为周期超快速旋转,从而在极短时间内快速抹平焦斑强度调制,改善靶面辐照均匀性.通过建立基于螺旋相位板的激光超快速角向集束匀滑方案的物理模型,分析了其角向匀滑特性,并与光谱角色散技术和径向匀滑技术进行了比较分析.结果表明,这一新型激光集束匀滑方案能实现对焦斑的超快速角向匀滑,且能在数皮秒时间内达到最佳辐照均匀性.     

涡运动:混沌与混合机理

本文综述了利用非线性动力学方法研究有涡流动的进展,并讨论了它们在流体混合机理研究中的应用.     

Spiral rainband in a numerically simulated tropical cyclone

Spiral rainband is a prominent structure of tropical cyclone. Though its forming mechanism, vortex Rossby wave theory, has been widely accepted in recent years,its internal structural features are still not well known. The spiral rainband in the severe tropical storm Kammuri (2002),which caused heavy rainfall in southeast China, is simulated using the mesoscale model MM5 (V3). Results show that the simulated spiral rainband propagates azimuthally at a speed close to that of vortex Rossby wave in theory, and is accompanied with energy dispersion in the radial direction. The structural features of simulated spiral rainband are analyzed with the high-resolution model output including the full physical process. Positive vorticity, ascending motion, horizontal momentum and so on are highly concentrated in the spiral rainband. The convergent moisture of spiral rainband comes mostly from the planetary boundary layer under 1 km.Airflow from the outside of spiral rainband is convective instability, which can provide instability energy for convection development. However, the atmospheric stratification in the inside of spiral rainband is neutral, implying that the instability energy has been released. There is a mesoscale strong wind band just near the spiral rainband in the outer side with a maximum wind speed exceeding 30 m/s, which results from the pressure force acceleration when the air flows into the spiral rainband along the gradient of pressure.     

新西兰的高等职业教育及其特点

简要介绍了新西兰高等职业教育的情况、新西兰提供高等职业教育的机构。着重介绍提供高等职业教育的国有机构——多种技术学院的概况、入学条件、颁发的学历证书的种类、灵活的课程时间安排、授课方式以及开设课程所覆盖的学科;还介绍了新西兰多种技术学院的特点,为我国高等职业教育的改革和发展提供一些参考和借鉴。     

磁化等离子体中的涡旋湍流和反常扩散

研究磁化等离子体中短波漂移阿尔芬波涡旋结构．采用涡旋气体动力学模型，估计出等离子体涡旋湍流谱，并求出反常扩散系数．研究结果表明，涡旋湍流产生的反常扩散系数与扰动场振幅的平方根成正比．     

Topological Vortices in the Modified Two-Dimensional Gross—Pitaevskii Theory

It is shown that there exists an elementary vortex topological current in the modified two-dimensional Gross—Pitaevskii theory. An explicit expression for the vortex velocity field as a function of the order parameter is derived. The evolution of vortices is studied from the topological properties of the order parameter field. It is found that vortices generate or annihilate at the limit points and encounter, split, or merge at the bifurcation points of the order parameter field .     

中国东部地区一个中尺度对流涡旋的涡度收支分析

中尺度对流涡旋(MCV),与其他中尺度涡旋不同,有着其独特的动力机制与发展途径.一旦MCV形成,极易产生灾害性天气过程.为了解我国的MCV,使用非静力中尺度模式天气预报和研究模式对中国东部2003年7月4至5日降水过程进行了高分辨率的双向三重嵌套的数值模拟.与观测资料比较,模拟结果较为准确地再现了当时的大气状况.采用了空间滤波的方法对模式结果进行了大尺度背景场与中尺度扰动场的尺度分离,对MCV的结构与移动进行分析,并追随MCV的活动对其的涡度收支情况进行诊断分析.分析表明,大尺度背景场与中尺度扰动场对MCV的作用有着明显的差异.MCV的移动由大尺度背景风场引导;其中辐合作用直接决定了MCV的形成与发展,大尺度水平运动对中尺度涡度的水平输送为水平平流项的主要部分.而由垂直风速的水平变化所导致的水平涡度的倾斜作用在此MCV形成与发展阶段作用并不明显.成熟时的MCV与成熟时的中尺度对流复合体类似有着3个明显的环流,在对流层高层与低层均为辐散反气旋性环流,对流层中层则为较为深厚的气旋性环流.