几种常用格式和湍流模型在高速流动中的适用性研究

针对高超声速飞行器中存在的强激波、激波/边界层干扰、分离、湍流等复杂流动现象,对比分析了当前计算流体力学中的主要空间离散格式及湍流模型,发现不同格式对强激波的分辨率基本相同,Roe和LDE(low diffusion E-CUSP(convective upwind split pressure))格式对摩擦因数和传热系数的模拟优于其他格式;S-A(Spalart-Allmaras)一方程湍流模型计算的摩擦因数比k-ωSST(shear stress transport)两方程湍流模型高10%左右,而后者预测的分离区约为前者的2倍,且分离点靠前.     

真空绝热板阻隔膜PA/ VMPET/ Al/ PE 热封工艺

真空绝热板阻隔膜PA/ VMPET/ Al/ PE 是一种多层复合阻隔膜,是真空绝热板的重要候选膜材。 通过实验研究了热封温度、时间、压力对其强度的影响,同时采用Matlab 软件对热封工艺参数进行优化,得出 最佳的热封工艺。利用DSC 对PA/ VMPET/ Al/ PE 进行热分析。实验结果表明:热封温度是影响热封强度的 最显著因素,当热封温度为160 ~170℃,热封时间为1. 0 ~2. 0 s,热封压力为0. 2 ~0. 4 MPa 时,热封边的热封 强度良好。Matlab 软件优化最佳热封工艺参数值为:热封温度167℃,热封时间1. 80 s,热封压力0. 34 MPa,该 模拟优化热封工艺参数与实验值一致。     

SINS/GNSS组合导航测试系统用惯导模拟源技术研究

针对光纤陀螺SINS(捷联惯性导航系统)与GNSS(全球卫星导航系统)组合导航产品高动态性能测试难的问题,本文研究了一种组合导航测试系统,并对捷联惯导模拟源进行了重点研究.首先以捷联惯导解算算法为基础逆推出了捷联惯导模拟源算法,然后对捷联惯导模拟源进行了功能实现,可以与导航卫星信号模拟源同步向组合导航计算机发送数据用于组合导航解算.最后对捷联惯导模拟源的功能与性能进行了验证.结果表明,捷联惯导模拟源功能正常,模拟数据的精度达到设计要求.利用此惯导模拟源与导航卫星信号模拟源配套使用,将可满足后续SINS/GNSS组合导航系统的相关性能测试或验证要求.     

高分辨率电流频率转换电路设计

随着惯性技术的发展,对电流频率转换电路的分辨率要求越来越高,以往常用的I/F转换电路已经不能满足要求,本文在传统电路的基础上结合FPGA和DSP提出了一种电路设计思路来提高分辨率.设计了硬件电路和软件电路.根据大量的试验数据分析,此改进电路在不损失电流频率转换电路线性度和稳定性的精度下,把电路的分辨率提高了一个数量级,解决了高精度电流频率转换电路分辨率低的问题,进一步扩大了电流频率转换电路的使用范围.     

浅析运输类飞机经济舱头排旅客座椅头部损伤判据的影响因素

介绍了头部损伤判据HIC的概念、适航要求及影响运输类飞机客舱头排旅客座椅HIC的相关参数;叙述了旅客座椅头排距、头部撞击壁板的刚度、安全带织带伸长率、乘坐摩擦系数等参数的影响和重要程度;对如何设计符合HIC要求的经济舱头排旅客座椅和壁板提出了建议。     

无人直升机悬停低速段的不确定性仿真验证

在无人直升机控制律的设计过程中,需要对无人直升机进行建模,并对飞行中产生的一些不确定性因素进行仿真验证.目前,很多不确定性因素的描述是在非线性的环境中加入一些简单的扰动,然而能够确切地描述无人直升机动态特性的非线性模型在MATLAB中很难搭建.为此,文章从工程研究的角度,提出了在无人直升机线性模型组的基础上进行不确定性仿真验证的方法,从物理特性的角度描述无人直升机在悬停低速飞行时的对象特性不确定性,选择不确定或扰动因子;在MATLAB中建立了仿真模型,进行了无人直升机悬停低速段不确定性的验证.此方法简单、快速,并且能正确地反应无人直升机悬停低速段的不确定性,具有一定的工程意义.     

多通道控制／检测操纵台

本操纵台可以对６４个通道或号位的综合参数，如温度、压力、温度、物位、流量等刊物民检测，它具有两种功能；（１）对６４个地点的进行自动巡回控制／检测；（２）可随意对任意地的参数进行优化控制／检测。     

Lateral Flight Technical Error Estimation Model for Performance Based Navigation

Flight technical error (FTE) combined with navigation system error (NSE) is the main part of total system error (TSE) in performance based navigation (PBN).The implementation of PBN requires pre-flight prediction and en-route short-term dynamical prediction of the TSE.Once the sum of predicted lateral FTE and NSE is greater than the specified PBN value,the PBN cannot operate.Thus,accurate modeling and thorough analysis of lateral FTE are indispensible.Multiple-input multiple-output (MIMO) lateral track control system of a transport aircraft is designed using linear quadratic Gaussian and loop transfer recovery (LQG/LTR) method,and the lateral FTE of a turbulence disturbed approach operation is analyzed.The error estimation mapping function of latera FTE and its bound estimation algorithm are proposed based on singular value theory.According to the forming mechanism of lateral FTE,the algorithm considers environmental turbulence fluctuation disturbance,aircraft dynamics and control system parameters.Real-data-based Monte-Carlo simulation validates the theoretical analysis of FTE.It also shows that FTE is mainly caused by turbulence fluctuation disturbance when automatic flight control system (AFCS) is engaged and would increase with escalating environmental turbulence intensity.     

钛合金熔模精铸氧化锆陶瓷型壳／金属界面反应研究

通过实际浇注和真空扩散连接分别制取了钛／型壳界面，借助ＳＥＭ、ＥＰＭＡ和显微硬度仪等分析测试手段对所得界面进行了深入研究，初步提出了以Ｚｒ、Ｏ元素向钛基体内的扩散为主导的界面反应机制。实验结果表明，界面反应并非在整个界面上均衡推进，而是在浓度、温度、能量起伏、以及陶瓷颗粒位向适宜的区域优先发生界面反应     

Solar cycle and latitude dependence of high-beta suprathermal plasma conditions in interplanetary space between 1.3 and 5.4 AU

The analysis of energetic particles and magnetic field measurements from the Ulysses spacecraft has shown that in a series of events, the energy density contained in the suprathermal tail particle distribution is comparable to or larger than that of the magnetic field, creating conditions of high-beta plasma. In this work we analyze periods of high-beta suprathermal plasma occurrences (β_ep > 1) in interplanetary space, using the ratio (β_ep) of the energetic particle (20 keV to ∼5 MeV) and magnetic field energy densities from measurements covering the entire Ulysses mission lifetime (1990–2009) in order to reveal new or to reconfirm some recently defined interesting characteristics. The main key-results of the work are summarized as follows: (i) we verify that high-beta events are detected within well identified regions corresponding mainly to the vicinity of shock surfaces and magnetic structures, and associated with energetic particle intensity enhancements due to (a) reacceleration at shock-fronts and (b) unusually large magnetic field depressions. (ii) We define three considerable features for the high-beta events, concentrated on the next points: (a) there is an appreciable solar-activity influence on the high-beta events, during the maximum and middle solar-cycle phase, (b) the annual peak magnitude and the number of occurrences of high events are well correlated with the sunspot number, (c) the high-beta suprathermal plasma events present a spatial distribution in heliographic latitudes (HL) up to ∼±80°, and a specific important concentration on the low (−25° ? HL < −6°, 6° < HL ? 25°) and median (−45° ? HL < −25°, 25° < HL ? 45°) latitudes. We also reconfirm by a statistical analysis the results of Marhavilas and Sarris (2011), that the high-beta suprathermal plasma (β_ep > 1) events are characterized by a very large parameter β_ep (up to 1732.5), a great total duration (406 days) and a large percentage of the Ulysses-mission lifetime (which is equal to 6.34% of the total duration with usable measurements, and 11.3% of the duration in presence of suprathermal particles events).