Evolution of the periodicities in 2S 0114+650

We have analysed 9 years of data from the All Sky Monitor on the Rossi X-ray Timing Explorer for 2S 0114+650 to study the evolution of its spin, binary, and super-orbital periods. The spin history of the neutron star in this system exhibits torque reversals lasting 1 year. The newly discovered super-orbital period has remained stable over the 9-year span, making 2S 0114+650 the fourth known system to exhibit stable super-orbital modulation. We compare its super-orbital period evolution with those of the other three such systems.     

一类空间对称6R机构的运动学研究及组合应用

可展开平板机构已广泛应用于平板天线、太阳翼等航天机构产品。为提高可展开平板机构的刚度和展收比,将空间对称6R机构应用于可展开平板机构设计。首先,根据约束条件,计算后给出了一种空间3R运动链的几何参数关系;然后,结合螺旋理论,分析了该3R运动链的约束螺旋系;进而根据对称性,研究了空间对称6R机构的自由度、奇异性等运动特征;在此基础上,提出了一种特殊的空间对称6R转动机构;最后,研究了空间对称6R机构的组合方法,设计出一种新型单自由度可展开平板组合机构,并对其进行了运动学仿真验证。该可展机构具有二维方向的展开收拢能力,为可展开平板机构的创新设计提供了有益参考。     

S形蒙皮零件成形工艺

通过运用S3F软件对S形蒙皮拉形过程进行模拟仿真分析,评估S蒙皮拉形工艺性;预测拉形过程中将产生的缺陷;制定合理工艺方案;优化零件设计和模具结构;实现了该蒙皮零件在数控蒙皮拉伸机上的拉形。     

Near infrared studies of the massive X-ray binary 2S 0114+65

We present near-infrared spectroscopy of the massive X-ray binary 2S 0114+650. These observations covering the spectral range 1.08–2.35 μm span the region where Paschen and Brackett series recombination lines of hydrogen are expected to be seen, namely, Paβ , Brγ and Br 10–17 lines. The absence of any of these lines in emission supports earlier inferences that the optical component in 2S 0114+650 is unlikely to be a Be star but rather a B type supergiant. Near-IR photometry gives J = 8.78, H = 8.53 and K = 7.96; these values show marginal variations from earlier reported measurements.     

宇航矢量伺服控制器在SiP中的设计与实现

磁场导向控制FOC（field-oriented control）矢量控制算法在伺服驱动控制系统中一般由CPU或DSP实现，难以满足航天应用中实时性较高场景下的需求。为提高宇航电机系统控制的实时性与可靠性，从FOC矢量控制算法的硬件加速角度出发，详细介绍了伺服控制器的设计，给出了一种全数字、高性能的伺服控制器硬件加速设计方案，并在具有可编程逻辑功能的宇航级SiP6117S芯片上进行了验证。仿真实验表明，相比于前人的设计，通过调整观测数据的量化精度来降低硬件加速过程中的处理延时，能有效改善多级流水延迟并在一定程度上提升算法的实时性。     

机载32位计算机指令系统结构军标分析

随着国际形势的缓和,美国国防工业及半导体制造业发生着微妙的变化,于是美国防部果断地提出军杯改革。面对这种情况,国内机载计算机造型、指令系统结构标准的制定和选择目前变成一个热门话题。本文介绍了几种典型的32位计算机指令系统结构标准和美国此方面的应用现状和特点,给出了机载计算机指令系统结构标准确定的可行性与途径。     

R141b在矩形微尺度通道中的两相流传热特性

设计搭建水力直径分别为1mm和0.5mm的矩形微尺度通道实验台,研究了以R141b型制冷剂作为工质的两相流沸腾传热特性。实验取热流密度为1～16kW/m2、质量流速为111.1～333.3kg/(m2·s)和质量干度为0～1,分析了三者对平均传热系数的影响,探究影响换热的主导因素。结果表明:热流密度较高时,平均传热系数随热流密度增加而减小,流动换热主要受到沸腾传热的影响;当质量流速较大且热流密度较低时,平均传热系数随热流密度增加而有所增长;热流密度较低时,平均传热系数随质量流速变化明显,热流密度升高到一定值后,质量流速对平均传热系数的影响很小;当质量流速处于111.1～333.3kg/(m2·s)时,平均传热系数随质量干度的增加而减小。      

Analytic and numerical treatment of motion of dust grain particle around triangular equilibrium points with post-AGB binary star and disc

This paper investigates the motion around the triangular equilibrium points, of a passively gravitating dust particle in the gravitational field of a low-mass post-AGB binary system, surrounded by circumbinary disc. The two bodies of the binary are modeled as a triaxial star and a radiating-oblate star. Due to small deviation of disc stars on circular orbits, we have assumed that the Coriolis and centrifugal forces of the stars are slightly perturbed. The triangular equilibrium points of the particle are found. These points are defined by, triaxiality of the primary star, oblateness and radiation of the secondary one and the gravitational potential from the disc mass. Further, when the disc mass increases, the particle moves nearer to the stars and farther away from the disc. In general, these equilibrium points are linearly stable when μ < μ_C; where μ is the mass ratio and μ_C is the critical mass function, defined by the parameters of the system. The effects of each of these parameters on the size of the stability region are stated, and the periodic motion around the stable points is examined. It is seen that the orbits are ellipses, and the orientation, eccentricities, lengths of the semi-major and semi-minor axes are influenced by the parameters of the problem. In particular, for our numerical linear stability analysis, we have taken an extremely depleted pulsating star, IRAS 11472-0800 as the post-AGB triaxial star, with a weakly-radiating young white dwarf star; G29-38 as the secondary. For this system, the stability result of the triangular points comes out different. Here, μ_C < μ throughout the entire range of the mass ratio and the critical mass function. Hence, the triangular equilibrium points are unstable. The stability of the orbits is tested using the Poincaré surfaces of section (Pss). The region of stability is controlled by the introduced parameters and the Jacobi constant.     

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。     

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。