技巧在中国古典舞学科中的作用

技巧是一切舞蹈训练的基础,具有舞蹈的一般性和共性特点。中国古典舞学科包含了广义上舞蹈学习必备的技巧共性特点,也体现了自身的个性特点。文章通过探讨技巧在中国古典舞中所起到的作用,使舞者通过掌握技巧找到自己的发展方向。重点研究了技巧的种类,研究跳、转、翻等技巧的特点,在中国古典舞中的作用以及在舞蹈表演中的运用,并以古典舞蹈为例,分析中国古典舞技巧在舞蹈内容、情感表达以及人物形象塑造中的作用。     

旋转工况下小型液冷源设计

设计了一种适用于旋转工况的小型液冷源,该液冷源采用强迫风冷换热器的原理。液冷源液路循环采用闭式系统设计以适应旋转工况的要求,液位检测采用光电式液位传感器,通过单向阀和电磁阀的组合使用可有效防止水锤效应。该系统具有体积小、重量轻、环境适应性强等优点。     

成岩作用与成岩储集相研究——科尔沁油田交2断决区九佛堂组（J3jf）下段

为了对科尔沁油田交2断块区九佛堂组(J3jf)下段的成岩作用与成岩储集相有一个明确的认识，在沉积相研究工作的基础上，利用取心井岩心系统观察及各类薄片鉴定(常规薄片和铸体薄片)、X—衍射、阴极发光、扫描电镜及电子探针能谱、图像分析等实验分析测试资料，对九佛堂组储层成岩作用类型进行研究，并实现了定量评价；研究结果确定了该区3类成岩储集相类型，即：杂基支撑强压实细—粉砂岩相，碳酸盐强胶结砂岩相及不稳定矿物强溶蚀成岩储集相．其中不稳定矿物强溶蚀成岩储集相为最有利于油气储集的成岩储集相类型．     

Form Invariance and Noether Symmetries of Rotational Relativistic Birkhoff Systems

Under the infinitesimal transformations of groups,a form invariance of rotational relativistic Birkhoff systems is studied and the definition and criteria are given,In view of the invariance of rotational relativistic Pfaff-Birkhoff-D‘ Alembert principle under the infinitesimal transformations of groups,the theory of Noether symmetries of rotational relativistic Birkhoff systems are constructed.The relation between the form invariance and the Noether symmetries is studied ,and the conserved quantities of rotational relativistic Birkhoff systems are obtained.     

基于旋转描述的三维几何造型方法

提出了一种能用凸四边形表示并可作平面展开的三维实体造型的设计方法。该方法用旋转描述表把二维平面展开图和三维实体联系起来，模拟人工折叠过程，由二维平面展开图逐次旋转变换完成三维造型重建。造型重建后，再通过纹理映射将平面设计图案映射到实体的各个面上，完成对实体着色渲染，生成具有真实感的三维实体。     

Gamow—Teller Resonance of 90Zr in a Relaztivistic Approach

We establish the formalism of nuclear spin-isospin excitations,especially the Gamow-Teller resonance in a fully consstent relativistic random-phase approximation.A relativistic form of the Landau-Migdal parameter g‘ is adopted as a residual spin-isospin correlation force.In the non-relativistic limit it reproduces the excitation energy of the giant Gamow-Teller resonance state obtained in the non-relativistic model.The Gamow-Teller resonance for finite nuclei is investigated in a relativistic approach for the first time.It is found that the Ikeda sum rule of 90Zr is quenched about 8% in the Hartree as well as the correlated strengths due to the poles of the negative Dirac states at energies above 1 GeV.     

Rotational Deformation of Neutron Stars

The rotational deformations of two kinds of neutron stars are calculated by using Hartle‘s slow-rotation formulism. The results show that only the faster rotating neutron star gives an obvious deformation. For the slow rotating neutron star with a period larger than hundreds of millisecond, the rotating deformation is very weak.