四轴惯性平台随动框架控制策略研究

三框架四轴平台系统的随动回路依靠控制随动框架转动使内环框架角始终保持在零位附近,用以保证载体在内环轴方向上具备全方位机动的能力.然而当外环框架角工作在±90°附近时,随动回路会失去正常功能,进入不稳定状态.为了解决这个问题,提出了一种新的随动框架控制方案,保证外环框架角在±90°时随动框架处于稳定状态,同时内环轴所指方向仍然可以进行大范围机动,从而使得三框架四轴平台实现真正的全方位机动能力.     

双 Y移 30°永磁同步电动机串联系统的仿真

双Y移30°永磁同步电动机串联系统可以实现同一变频电源供电和同一套控制平台下2台电机的解耦运行,节省了控制装置和外围电路,降低控制系统的体积、重量与成本。文章给出了双Y移30°永磁同步电动机串联系统的矢量控制策略,建立了仿真数学模型,并进行了变负载运行的仿真,结果验证了该串联系统解耦运行的可行性。     

高职院校学生心理健康调查报告

为全面、定量了解刚入学的学生心理健康状况，采用SCL-90临床症状自评量表对刚入学的全体大一新生进行心理健康情况测定，结果显示学院学生总体的健康状况要好于全国健康平均水平，数据结果还反映出高职大专生常见的心理障碍或心理问题：强迫、人际关系障碍和抑郁。从调查结果我们可以总结出一些规律性的结论，这些结论给学院学生教育和管理工作提供一些参考作用。     

涡轮级燃气入侵的理论分析及数值模拟

为了分析航空发动机涡轮级中的燃气入侵现象,提出一种研究封严间隙处流动规律的理论方法,并采用全环模型进行了数值模拟。在该理论方法中,动盘旋转、封严冷气、外环主流对流动的影响用三个特征速度来表征;它们的相互作用用速度比来描述。数值模拟结果表明:随着速度比的变化,封严间隙处呈现燃气沿静盘入侵、燃气基本不入侵以及燃气沿动盘入侵等三种流动形式。利用速度比的影响规律,可初步判断封严间隙处的燃气入侵情况以及最小封严冷气流量。     

Numerical integration of stochastic differential equations: A parallel cosmic ray modulation implementation on Africa’s fastest computer

Three-dimensional studies of the transport and modulation of cosmic ray particles in turbulent astrospheres require large-scale simulations using specialized scientific codes. Essentially, a multi-dimensional Fokker-Planck type equation (a parabolic diffusion equation) must be integrated numerically. One such approach is to convert the relevant transport equation into a set of stochastic differential equations (SDEs), with the latter much easier to handle numerically. Due to the growing demand for high performance computing resources, research into the application of effective and suitable numerical algorithms to solve such equations is needed. We present a case study of the performance of a custom-written FORTRAN SDE numerical solver on the CHPC (Centre for High Performance Computing) Lengau cluster in South Africa for a realistic test problem with different set-ups. It is shown that SDE codes can scale very well on large parallel computing platforms. Finally, we consider an extremely computationally expensive application of the SDE approach to cosmic ray modulation, studying the behaviour of galactic cosmic ray proton latitude gradients and relative amplitudes in a physics-first manner. This is done using a modulation code that employs diffusion coefficients derived from first principles, which in turn are functions of turbulence quantities in reasonable agreement with spacecraft observations and modelled using a two-component turbulence transport model (TTM). We show that this approach leads to reduced latitude gradients qualitatively in line with spacecraft observations of the same, without making ad hoc assumptions as to anisotropic perpendicular diffusion coefficients as are often made in many cosmic ray modulation studies.     

旋转状态下S型带肋通道流动特性数值研究

为了更好地了解涡轮叶片内冷完整通道中流体的流动特性,数值研究了肋、转弯以及旋转对完整S型带肋通道流动特性的影响.雷诺数为17000,3个出口的出流比分别为27%,49%,24%,旋转数取0,0.03,0.06,0.09.结果表明:通道1靠近前缘侧阻塞比高,肋的扰流作用强,流体速度较低.转弯引起流体流动分离,使转弯下游通道中的主流发生偏移,通道3靠近分隔板侧存在较大范围低速区.旋转产生的切向哥氏力使流体向哥氏力指向面偏移,通道2与通道3主流分别偏向吸力面与压力面.旋转影响通道中二次流的分布,增强转弯下游低速回流涡区域流体的流动.