基于混沌搜索的三级倒立摆LQ控制器设计

研究利用混沌优化的LQ控制方法对三级倒立摆系统进行闭环控制.首先将混沌变量引入LQ控制器的权矩阵参数域,并进行全局范围内直接寻优,当获得全局近似最优解后,再缩小寻优区间,在次优解附近继续寻优,得到全局最优权矩阵参数.仿真结果表明了该方法的有效性和具有良好的抗干扰能力.     

二自由度平面并联机床的柔度与变形分析

文中对一种新型平面并联机床的速度,力与变形关系进行分析,得到其速度、力雅可比矩阵进而得到其柔度矩阵,提出该并联机床柔度评价指标,并给出了该评价指标在工作空间内的分布情况,为该并联机床的设计与应用提供了有益参考。     

一种摩擦阻尼器在整体叶盘结构的应用

介绍了一种应用于整体叶盘结构的摩擦阻尼器,即在轮缘下方加工销孔,安装阻尼销.工作时,由于离心载荷的作用,阻尼销与轮缘相互摩擦,从而消耗振动能量.这种阻尼器被应用于两台发动机的涡轮整体叶盘减振方案中,试验结果显示:其减振效率差异较大.数值模拟分析证明,这种阻尼器的减振效率和振动能量在叶-盘间的传递有关.对于叶-盘强耦合振型,这种阻尼器可以获取较高的减振效率,叶片振动应力水平下降了约70%;但对于叶-盘弱耦合振型,叶片振动应力幅值没有明显下降趋势.      

基于背景纹影技术的随机介质折射率场测量

针对光线通过复杂流场时产生的光传输效应问题,提出了基于背景纹影技术的复杂折射率场测量方法,给出了根据粒子图像偏移量求解折射率场分布的计算方法和推导过程,并对该方法的分辨率与灵敏度进行了理论分析。在此基础上,对火焰上方折射率场的分布进行了实验测量,利用粒子图像测量(PIV)技术对实验图像进行处理。结果表明:实验测量得到的空气折射率最大值为100029,最小值为100009,测量有效值小于00001。表明该方法具有较高的测量精度,能够有效实现复杂折射率场的实时精确测量。      

基于地球红外背景模拟的 水云大气影响初步分析

为支持地球红外背景的模拟研究,以天基观测为前提,计算了2个大气窗口下,4个具有典型大气和地表特征的区域在水云大气下的路径透过率和各成分辐射亮度。通过相对变化比例,讨论了地球背景模拟中水云与地表的图像区分以及地域的影响。结果表明,水云对地球背景辐射传输影响显著:云层下方辐射会被强烈衰减,同时观测路径中的散射辐射大幅增强。在同一选定区域下,积云大气的观测路径亮度相对无云大气下变化最大,在相同水云类型条件下,大气散射和太阳散射亮度在不同区域区别较大,说明在模拟水云地球背景时不能忽略地域的影响。计算和分析结果可为地球背景模拟中的水云红外图像生成提供一定的数据基础和技术支持。     

AIRCRAFT CONCEPT EVALUATION AND EFFECTIVENESS-BASED DECISION-MAKING

Based on effectiveness analysis, a novel method is presented for combat aircraft top-hierarchy concept evaluation and decision-making. Applying multi-criterion decision-making （MCDM） and analytic hierarchy process, the new method can help to overcome the limitations of existing evaluation systems and decision-make methods. The proposed method includes the following process~ （1） Establish a multi-criterion and multi-hierarchy evaluation attribute system by introducing combat effectiveness~ （2） Assign weight to the attributes and normalize them; （3） Evaluate and decision-make top-hierarchy aircraft concept based on effectiveness to reach a satisfactory design by comprehensively applying four multi-criterion decision-making methodologies, i.e. grey correlation pro- jection method, weighted summation method, weighted quadrature method and ideal solution decision-making method, while considering the attribute hierarchy system and the logical relations among the attributes. Finally, an example is given to indicate the validity and feasibility of the proposed method.     

Numerical modeling of inhomogeneous orographic wave influence on planetary waves in the middle atmosphere

Parameterization of dynamical and thermal effects of stationary orographic gravity waves (OGWs) generated by the Earth’s surface topography is incorporated into a numerical model of general circulation of the middle and upper atmosphere. Responses of atmospheric general circulation and characteristics of planetary waves at altitudes from the troposphere up to the thermosphere to the effects of OGWs propagating from the earth surface are studied. Changes in atmospheric circulation and amplitudes of planetary waves due to variations of OGW generation and propagation in different seasons are considered. It is shown that during solstices the main OGW dynamical and heat effects occur in the middle atmosphere of winter hemispheres, where changes in planetary wave amplitudes due to OGWs may reach up to 50%. During equinoxes OGW effects are distributed more homogeneously between northern and southern hemispheres.     

An ion analyzer for the lunar surface with E-parallel–B

We present a novel instrument concept to measure the energy and mass spectra of ions incident on the lunar surface, based on the E-parallel–B or Thomson-parabola device used extensively as a diagnostic in the plasma fusion community. The Apollo-era Suprathermal Ion Detector Experiment (SIDE) was the first instrument package to perform in-situ measurements of ions incident on the lunar surface. The ions can originate from a variety of sources, including the solar wind, the Earth’s magnetotail, and photoionization of the thin lunar atmosphere. The species and energy distribution of ions arriving at the lunar surface depend in a complicated and poorly-understood fashion on the phase of the lunar day, the position of the Moon with respect to the Earth, and on the local plasma environment.     

Photolytic behaviour of methane at Lyman-α and 248 nm: Studies in the frame of a simulation program of Titan’s atmosphere (S.E.T.U.P.)

This paper first describes briefly some of the forefront global simulations of Titan’s atmosphere that have been carried out up to now. In these experiments, an initial gaseous mixture of N₂/CH₄ is submitted to a single energy source and the retrieved gas and/or solid phase(s) is/are analyzed by different techniques.     

Electromagnetic waves observed by Venus Express at periapsis: Detection and analysis techniques

The magnetometer on Venus Express was designed to be able to obtain 128 Hz samples of the magnetic field from two sensors in a gradiometer configuration. This mode is used around periapsis to determine whether the signals reported at low altitudes near 100 Hz, had the properties of electromagnetic waves generated by electric discharges in the Venus atmosphere. The lack of a magnetic cleanliness program and the shortness of the magnetometer boom make this a challenging measurement. Fortunately the signals are sufficiently strong that they can be easily resolved with rather straightforward analysis techniques.