导弹大迎角下非线性诱导滚转力矩数值研究简

 采用计算流体力学（CFD）数值模拟方法,研究战术导弹大迎角状态下涡破裂导致滚转力矩随迎角非线性增长引起舵面控制能力不足的现象。首先通过标准模型的数值分析,验证了所采用的CFD方法具有三角翼前缘涡破裂现象的捕捉能力;然后采用雷诺平均Navier-Stokes方程对某“++”字正常布局导弹构型（含弹翼、弹身、尾舵和整流罩等）进行了数值模拟,结果显示亚声速状态下滚转力矩在迎角大于20°时出现非线性增长,导致全动尾舵的滚转控制能力不足。通过分解各部件对滚转力矩的贡献,并分析流场结构,探明了该现象发生的流动机理,其主要原因是：随着迎角的增长,弹体迎风面的尾舵前缘涡首先发生破裂,导致其平衡诱导滚转力矩的作用被削弱。     

舰载飞机着舰拦阻动力学研究综述简

 拦阻着舰过程通常被认为是舰载飞机事故率最高的阶段,因此,自从有了航空母舰和舰载飞机,拦阻着舰动力学就一直是国内外相关研究人员的研究热点。本文从拦阻钩、拦阻装置和起落架3个关键部件着手,比较详细地论述了舰载飞机着舰拦阻涉及到的关键动力学问题及其研究现状,重点对拦阻钩弹跳动力学及其载荷分析、拦阻索动力学及其载荷分析、下沉速度、非对称拦阻对起落架载荷的影响、拦阻系统动力学等方面进行了综述。最后,对着舰拦阻动力学研究的发展趋势进行了展望。     

气核尺寸对气液同轴离心式喷嘴自激振荡的影响

为了研究气核尺寸对气液同轴离心式喷嘴自激振荡的影响,采用水和空气作为模拟介质,开展了室压条件下冷态喷雾试验。通过试验分析了气核尺寸较大时气液同轴离心式喷嘴自激振荡的喷雾形态,与文献中气核尺寸较小时的喷雾形态进行对比发现气核尺寸不同时,该类喷嘴自激振荡的喷雾形态不同,气核尺寸较大时呈"圣诞树"型分布,气核尺寸较小时呈"串"型分布。气核尺寸对气液同轴离心式喷嘴自激振荡的产生机理有显著影响,由于自激振荡产生机理的不同,喷嘴缩进长度对自激振荡的影响也不同,气核尺寸较大时自激振荡频率随着喷嘴缩进长度呈复杂变化特征,气核尺寸较小时喷嘴缩进长度对自激振荡频率没有影响。气液同轴离心式喷嘴自激振荡频率为2~4kHz,与燃烧室一阶振型接近,喷雾自激振荡可能会诱发燃烧室不稳定燃烧。     

Identification method for helicopter flight dynamics modeling with rotor degrees of freedom

A comprehensive method based on system identification theory for helicopter flight dynamics modeling with rotor degrees of freedom is developed. A fully parameterized rotor flapping equation for identification purpose is derived without using any theoretical model, so the confidence of the identified model is increased, and then the 6 degrees of freedom rigid body model is extended to 9 degrees of freedom high-order model. Bode sensitivity function is derived to increase the accuracy of frequency spectra calculation which influences the accuracy of model parameter identification. Then a frequency domain identification algorithm is established. Acceleration technique is developed furthermore to increase calculation efficiency, and the total identification time is reduced by more than 50% using this technique. A comprehensive two-step method is established for helicopter high-order flight dynamics model identification which increases the numerical stability of model identification compared with single step algorithm. Application of the developed method to identify the flight dynamics model of BO 105 helicopter based on flight test data is implemented. A comparative study between the high-order model and rigid body model is performed at last. The results show that the developed method can be used for helicopter high-order flight dynamics model identification with high accuracy as well as efficiency, and the advantage of identified high-order model is very obvious compared with low-order model.     

弧翼飞行器柔性飞行动力学研究

以一种弧翼布局飞行器为背景,介绍了飞行器的特性;建立了线性分布式气动力模型,添加到全机的三维有限元柔性模型上,进行飞行动力学的仿真分析。研究了分布式气动力模型对弧翼布局飞行器的柔性飞行动力学特性造成的影响。通过对不同响应情况下的飞行状态的仿真计算与分析,总结出了采用分布式气动力建模的大展弦比弧翼飞行器的柔性飞行动力学的变化规律。     

超声速隐身歼轰机概念设计数值模拟

为了提高军用飞机的空战和对面攻击能力,对歼轰机进行总体设计。采用CATIA软件,设计出隐身歼轰机的三维数字样机和武器挂载方案;基于物理光学法和等效电磁流法,采用自编的RCSAnsys软件,数值模拟歼轰机的数字样机在X、S和UHF波段下的RCS特性和强度分布特性;基于湍流模型的k-ε方程和控制理论的N-S方程,采用Fluent软件,数值模拟歼轰机的数字样机所在空气流场的压强和速度分布云图,得出整机的升阻特性。概念设计数值模拟结果表明：内置弹舱的歼轰机前向±30°的RCS均值≤-4.728 dBsm,超声速飞行时歼轰机的升阻比约等于5.6337。     

空间平台发射拦截器动力学与最优脉冲拦截

研究了空间平台发射拦截器的两体耦合动力学,以及拦截器拦截目标星的最优脉冲控制问题。平台首先与目标星形成绕飞关系,保持其发射筒轴线始终瞄准目标星。接到发射指令后,拦截器从发射筒中射出,本文采用拉格朗日第二类方程建立了发射过程平台-拦截器两体动力学模型。因为两体耦合影响,平台姿态偏转,拦截器出筒时的速度已经不能瞄准目标星。通过小型火箭发动机给其施加速度脉冲,使其进入拦截轨道,保证拦截的同时,将脉冲速度最小化以节省燃料,本文将其归结为一个非线性规划问题,采用三级优化的策略来求解。在拦截飞行时间相较于平台绕飞目标星的周期是小量的条件下,可以视绕飞平均角速度为小参数,采用正则摄动方法求出非线性规划的一阶近似解,然后以此为迭代初值,寻找最优真解。最后进行了数值仿真验证。     

Modeling Multifractality of the Solar Wind

The question of multifractality is of great importance because it allows us to investigate interplanetary hydromagnetic turbulence. The multifractal spectrum has been investigated with Voyager (magnetic field) data in the outer heliosphere and with Helios (plasma) data in the inner heliosphere. We use the Grassberger and Procaccia method that allows calculation of the generalized dimensions of the solar wind attractor in the phase space directly from the cleaned experimental signal. We analyze time series of plasma parameters of the low-speed streams of the solar wind measured in situ by Helios in the inner heliosphere. The resulting spectrum of dimensions shows a multifractal structure of the solar wind attractor. In order to quantify that multifractality, we use a simple analytical model of the dynamical system. Namely, we consider the generalized self-similar baker’s map with two parameters describing uniform compression and natural invariant measure on the attractor of the system. The action of this map exhibits stretching and folding properties leading to sensitive dependence on initial conditions. The obtained solar wind singularity spectrum is consistent with that for the multifractal measure on the weighted baker’s map.     

航天飞机系统两体分离问题的探讨

本文简要地叙述了美国研究轨道器与外挂贮油箱,轨道器与载机分离问题的概况。对垂直起飞两级入轨的并联两机的分离问题,提出了研究模型并作了具体分析,着重提出了实现两机安全分离需要解决的技术难点。 二级航天飞机的两机分离问题,是未来航天高技术领域的关键技术之一,本文阐述了解决两体并联分离问题我国现有的技术水平,并提出了解决该问题的技术方案。     

PC-index fluctuations and intermittency of the magnetospheric dynamics

One minute resolution Polar Cap (PC) index was used for the analysis of magnetospheric dynamics. The 1995–2000 time series analysis revealed that the power spectrum of the PC-index fluctuations is a power law in a wide range of frequencies. However, the obtained exponents differ for low and high frequency regions. The probability distribution functions of the PC-index fluctuations show a strong non-gaussian shape, depending on the time of increment. This indicates that the PC-index exhibits intermittency, previously detected in solar wind and auroral electrojet index fluctuations. The PC-index probability distribution functions were fitted by the functional form proposed by Castaing et al. [Velocity probability density functions of high Reynolds number turbulence. Physica D. 46, 177–200, 1990] to describe intermittency phenomena in ordinary turbulent fluid flows. The agreement between the fitting parameters obtained for the PC index and those reported before for solar wind magnetic field fluctuations is within 30%; which is noticeably less than the difference between the same parameters of solar wind and the AE-index fluctuations. This fact indicates that the PC index reflects the solar wind influence on the high-latitude magnetosphere, especially during the summer.