旋翼跨音速非定常黏性绕流的高效CFD模拟方法

为提高旋翼跨音速黏性绕流CFD模拟的效率,建立了一套基于隐式LU-SGS算法和OpenMP并行策略的旋翼非定常流场高效数值求解方法。首先,基于二维剖面翼型的Poisson方程求解和网格插值、翻折方法生成绕桨叶的O-C-O型贴体正交网格,并采用高效的"扰动衍射"(Disturbance diffraction method,DDM)挖洞方法、并行化″Inverse map″(IM)的贡献单元搜索方法,构建了旋翼运动嵌套网格系统。在此基础上,以耦合S-A湍流模型的非定常RANS方程为主控方程,对流通量采用高精度的Roe-MUSCL格式进行离散,时间推进采用隐式LU-SGS双时间方法,同时采用OpenMP并行策略加速旋翼流场求解。最后,运用所建立的方法分别对悬停ONERA 7A旋翼、前飞Caradonna-Tung(C-T)旋翼无升力状态及SA349/2旋翼有升力状态的气动特性及涡尾迹特征进行了模拟,通过与试验值对比验证了文中方法在旋翼非定常流场CFD模拟中的有效性和高效性。     

LXI仪器的LAN设置及控制

在介绍了LXI仪器类型、Non Auto-MDIX含义、Agilent33220A函数发生器性能和功能的基础上,以33220A函数/任意波形发生器的LAN接口设置为例,描述了其LAN接口DHCP,Auto IP,IP Address,SubnetMask,Default Gateway,Host Name,Domain Name,DNS Server,Password等参数的含义、设置方法,介绍了充分利用其提供的接口功能,达到远程控制其输出的方法。该方法达到了通过GPIB控制函数/任意波形发生器的同样效果,利用其LAN接口组建分布式测试系统,对程序设计者具有较高的参考借鉴价值。     

Onboard orbit determination using GPS observations based on the unscented Kalman filter

Spaceborne GPS receivers are used for real-time navigation by most low Earth orbit (LEO) satellites. In general, the position and velocity accuracy of GPS navigation solutions without a dynamic filter are 25 m (1σ) and 0.5 m/s (1σ), respectively. However, GPS navigation solutions, which consist of position, velocity, and GPS receiver clock bias, have many abnormal excursions from the normal error range for space operation. These excursions lessen the accuracy of attitude control and onboard time synchronization. In this research, a new onboard orbit determination algorithm designed with the unscented Kalman filter (UKF) was developed to improve the performance. Because the UKF is able to obtain the posterior mean and covariance accurately by using the second-order Taylor series expansion through the sampled sigma points that are propagated by using the true nonlinear system, its performance can be better than that of the extended Kalman filter (EKF), which uses the linearized state transition matrix to predict the covariance. The dynamic models for orbit propagation applied perturbations due to the 40 × 40 geo-potential, the gravity of the Sun and Moon, solar radiation pressure, and atmospheric drag. The 7(8)th-order Runge–Kutta numerical integration was applied for orbit propagation. Two types of observations, navigation solutions and C/A code pseudorange, can be used at the user’s discretion. The performances of the onboard orbit determination were verified using real GPS data of the CHAMP and KOMPSAT-2 satellites. The results of the orbit determination were compared with the precision orbit ephemeris (POE) of the CHAMP and KOMPSAT-2 satellites.     

基于μC/OS-Ⅱ的串口通信在S3C2410A上的实现

文章在三星公司的嵌入式处理器S3C2410A为核心的硬件平台上,将嵌入式实时操作系统μC/OS-Ⅱ和μC/GUI在ARM9上整合实现,成功地实现了基于μC/OS-Ⅱ在S3C2410A上的双向串口通信功能。     

Height of shock formation in the solar corona inferred from observations of type II radio bursts and coronal mass ejections

Employing coronagraphic and EUV observations close to the solar surface made by the Solar Terrestrial Relations Observatory (STEREO) mission, we determined the heliocentric distance of coronal mass ejections (CMEs) at the starting time of associated metric type II bursts. We used the wave diameter and leading edge methods and measured the CME heights for a set of 32 metric type II bursts from solar cycle 24. We minimized the projection effects by making the measurements from a view that is roughly orthogonal to the direction of the ejection. We also chose image frames close to the onset times of the type II bursts, so no extrapolation was necessary. We found that the CMEs were located in the heliocentric distance range from 1.20 to 1.93 solar radii (Rs), with mean and median values of 1.43 and 1.38 Rs, respectively. We conclusively find that the shock formation can occur at heights substantially below 1.5 Rs. In a few cases, the CME height at type II onset was close to 2 Rs. In these cases, the starting frequency of the type II bursts was very low, in the range 25–40 MHz, which confirms that the shock can also form at larger heights. The starting frequencies of metric type II bursts have a weak correlation with the measured CME/shock heights and are consistent with the rapid decline of density with height in the inner corona.     

均匀化处理对7A55铝合金组织与性能的影响

研究了单级均匀化和双级均匀化工艺对铸态7A55铝合金组织和性能的影响规律.结果表明,经450℃单级均匀化处理后,合金中的残留共晶仍然较多,保温60h时合金中残留共晶比例由铸态合金的15.2%减少至7.2%,合金硬度由72HRB降低至60HRB,伸长率则由2.1%增大至11.2%;经450℃/60h+470℃双级均匀化处...     

大型民用窄体客机液压系统分析探讨

分析和对比了同座级的空客A320和波音737的液压系统,并研究了民机液压系统的发展趋势。     

基于GJB 5000A二级的航天系统软件配置管理解决方案

军用软件研制能力成熟度模型(GJB 5000A-2008)作为一种标准只是提出了软件过程要达到一定成熟度能力的要求,给出了软件过程改进的阶梯式进化框架,但是并没有具体地告知该如何去做、怎么去做,这成为航天军工企业软件过程改进的一个难点。为解决航天系统软件配置管理工作中存在的问题,提出一种基于GJB 5000A标准的适于航天系统软件实施配置管理的解决方案。项目实践效果表明,与没有实施软件配置管理时相比,在规范管理、团队工作效率、知识库建立、软件安全性和可靠性等方面都有很大的提高。     

星箭锁紧装置黏滞摩擦系数的影响因素研究

星箭锁紧装置是卫星与火箭连接的关键机构。装置中的V形卡块在预紧力施加过程中,易发生偏斜,使得星箭分离配合面接触不均匀,产生应力集中,导致星箭分离面黏着磨损。研究了星箭锁紧装置中的V形卡块和上下端框的铝合金摩擦副在不同影响因素下摩擦系数的变化,探究了温度、正压力以及铝合金表面粗糙度对界面黏着和黏滞摩擦系数的影响。研究结果表明,硫酸阳极化处理的2A14T6-2A14T6比较适合作为摩擦副材料,在加工和锁紧过程中,应合理控制其粗糙度、温度和正压力,以避免黏着磨损。     

A320驾驶舱人为错误的管理

防止驾驶舱人为错误是保障飞行安全的有效措施。根据Helmreich操作类型分类法,统计分析了国航浙江公司A320飞机QAR三级超限事件连续三年的数据,并结合问题调查等数据,对该公司的人为错误进行研究,并给出了可操作性的人为错误管理策略,探索了利用QAR数据开展航空公司人为错误研究的方法,为国航浙江公司A320飞机的人为错误管理提出了建议。对提高飞行安全减小人为错误具有积极意义。