基于相似理论的航空发动机转速自适应PID控制

根据航空发动机在相似坐标系中特性不变的特点，提出一种基于相似理论的航空发动机转速自适应PID控制。该方案采用衰减曲线法进行换算PID参数整定，获得自适应调节律。仿真结果表明控制器具有良好的动静态性能，自适应性和鲁俸性。所得参数变化规律对数控系统全包线内PID控制器的参数选择具有一定的指导意义。     

高位垂直进气径向出流旋转盘腔风阻效应的实验

用实验的方法对高位垂直进气转静系旋转盘的风阻效应进行了研究,研究结果表明:转盘无量纲力矩系数随着旋转雷诺数的增加而减小;转盘无量纲力矩系数随着流量系数的增加而增加;且与冷却的具体结构有关;在高旋转雷诺数时,转盘无量纲力矩系数小于自由盘无量纲力矩系数;当流量为0时,无量纲力矩系数的数值全部小于自由盘之值.     

旋转盘腔紊流流动的数值研究

为了比较近壁紊流模型对旋转盘腔内流动特征模拟精度的影响，采用在核心区选用标准k-ε模型、在近壁区选用单方程和Launder-Sharma两方程两种低雷诺数模型的区域紊流模化方法，对具有径向出流的转-静盘腔和具有径向出流的共旋盘腔结构的流动进行了数值计算研究，计算结果表明：在计算的两个算例中，前者采用近壁单方程模型要稍优于两方程模型，后者采用近壁两方程模型要明显优于单方程模型，因此近壁区紊流特性的处理对旋转盘腔内的流场模拟精度具有重要的影响。     

涡扇发动机转速鲁棒控制器设计及试验

在分析某型涡扇发动机试验数据的基础上，给出了涡扇发动机在不同转速下频率特性的变化，得到了涡扇发动机数学模型参数摄动的权函数，设计了一个满足给定鲁棒性能指标的控制器。通过试验验证了涡扇发动机控制系统的鲁棒性能。     

Comparative Study of the Dynamics of the Outer Planets

The two classes of outer planets, Gas Giants and Ice Giants, have distinctly different global circulation patterns and internal structure. Ongoing ground-based observations of the Ice Giants provide clues to better understanding and Galileo and Cassini data will generate constraints for Gas Giant modeling. The composition below the cloud levels, the depths to which the winds penetrate and the processes that sustain the zonal winds and weather systems are not understood. Basic questions concerning the structure, composition and atmospheric dynamics that are sustained on the four giants could be answered by a combination of orbiters and probes. Future missions that could answer these questions are not currently under development.     

轴流压气机中喘振和旋转失速的数值模拟

基于轴流压气机逐级过失速特性，建立了多级轴流压气机过失速瞬态，包括喘振或旋转失速的分析模型。发展了分析轴流压气机过失速响应的动态滞后方法，并确定了压气机过失速响应的统一时间滞后常数。对一实验轴流压气机的过失速瞬态进行了数值模拟，与实验结果的一致性较好。     

双组元轨控发动机声腔技术方案及试验验证

作为解决小推力双组元发动机高频不稳定燃烧的主要技术途径,本文主要对发动机声腔技术方案进行了研究,研究工作包括发动机结构固有频率分析、声腔型式的选择、声腔结构方案设计及全尺寸热试验证。研究结果表明,发动机主要抑制振型为一阶切向振型和一切一纵复合振型。对发动机的工作稳定性进行了评价,验证了发动机固有频率计算结果并对三种声腔结构方案进行了比较。     

旋转梁的动力学建模及其反馈控制

利用哈密尔顿原理,推导了刚柔耦合形式的旋转欧位－伯努利梁的动力学方程,并在小转速的假设下,给出了线性化近似方程的解析解;讨论了由直流电机和压电陶瓷组成的控制系统,并从动力学稳定的角度出发,利用Lyapunov第一方法设计系统的反馈控制实现了动力学稳定性。最后通过计算机仿真证明控制策略的有效性。     

X-ray observations of black-hole accretion disks

Our current theoretical and observational understandings of the accretion disks around Galactic black-holes are reviewed. Historically, a simple phenomenological accretion disk model has been used to interpret X-ray observations. Although such a phenomenological interpretation is still useful, high quality X-ray data from contemporary instruments allow us to test more realistic accretion disk models. In a simple and ideal case, the standard optically thick accretion disk model is successful to explain observations, such that the inner disk radius is constant at three times the Schwarzschild radius over large luminosity variations. However, when disk luminosity is close to or exceeds the Eddington luminosity, the standard disk model breaks, and we have to consider the “slim disk” solution in which radial energy advection is dominant. Recent observations of Ultra-luminous X-ray sources (ULXs), which may not be explained by the standard disk model, strongly suggest the slim disk solution. We compare theoretical X-ray spectra from the slim disk with observed X-ray spectra of ULXs. We have found that the slim disk model is successful to explain ULX spectra, in terms of the massive stellar black-holes with several tens of solar mass and the super-Eddington mass accretion rates. In order to explain the large luminosities (>10⁴⁰ ergs s⁻¹) of ULXs, “intermediate black-holes” (>100M) are not required. Slim disks around massive stellar black-holes of up to several tens of solar mass would naturally explain the observed properties of ULXs.     

小型固体发动机旋转试验用微型点火控制与数据采集系统

为适应固体火箭发动机旋转试验的需要,以MCS—96单片机为主机,设计了一种微型的点火控制与数据采集系统。该系统直接安装在旋转试验台内部。省去了传统的集流环,为以后开展悬浮试验创造了条件。