非均匀入口与化学非平衡效应对尾喷管性能的影响研究

基于煤油燃料超燃冲压发动机尾喷管,对均匀入口和非均匀入口、冻结流动模型和化学非平衡模型下的尾喷管内流动进行数值模拟,采用两方程RNG k-ε湍流模型对三维NS方程组进行求解,获得非均匀入口与化学非平衡效应对尾喷管性能的影响。计算结果表明,尾喷管内流动非均匀性由尾喷管非对称膨胀和燃烧室出口非均匀等因素构成,尾喷管入口流动参数非均匀分布对尾喷管推力、升力及俯仰力矩均有影响,算例中非均匀入口使得尾喷管净推力相对于均匀入口增加了1.2%左右;尾喷管性能受化学非平衡效应的影响,非平衡流动模型下的其净推力计算结果相对于冻结流动模型增加3%~4%。     

基于ANSYS的机翼动力学分析

针对无人机在挂载导弹飞行和发射导弹时,无人机机翼由于受到多种载荷影响所产生的应力应变,应用ANSYS软件动力学分析,计算模拟了机翼在受到多种载荷影响时所产生的应力分布和应变量。分析结果表明,由于外挂物重量和机翼周围气动流场的影响,机翼会产生不同程度的颤振和扭转,其研究结果对合理设计机翼结构具有一定的参考意义。     

风洞模型投放试验轻模型法重力效应影响

风洞模型投放试验是研究超声速机弹分离问题的一种有效手段，相似参数的选取是影响试验准度的关键因素。有初始弹射速度的超声速机弹分离研究中，通常采用"轻模型法"得到模型的运动学及动力学相似参数，但该相似参数中模型重力模拟不足。为了研究重力效应对投放试验结果的影响，采用CTS试验技术对全尺寸真实参数与缩比尺寸轻模型法相似参数条件下得到的结果进行了对比研究。研究结果表明：在载弹与载机分离过程中，载弹位姿相互耦合，垂直下落位移的快慢会影响载弹姿态角的变化；轻模型法相似参数条件下，载弹垂直下落位移较慢，虚拟重力的修正方法只能近似修正下落位移，不能对导弹姿态角进行修正，而姿态角会影响下落的位移；机弹分离安全性方面，轻模型法相似参数条件下的试验结果较真实参数偏危险。     

Monitoring the thermal condition of permanent-magnet synchronousmotors

This paper describes a novel approach to monitoring the condition of small permanent-magnet synchronous motors (PMSM) operating under thermal stress. The approach begins with the estimation of temperature-dependent motor parameters from measurements of line voltages and currents. The parameters are then used to derive estimates of motor temperatures. Next, the electrically estimated temperatures are combined with a surface measurement of motor temperature and a dynamic thermal model of the motor to yield an observer that is a Kalman filter. The temperatures estimated by the observer are used for failure prevention. Finally, by modifying the observer, it is tuned to use the geometric properties of its innovation for failure detection. The innovation, that is, the difference between the thermally and electrically estimated temperatures, is monitored and compared against appropriate thresholds to detect failures. Failure detection is demonstrated experimentally, and shown to be capable of distinguishing the conditions of normal operation, and operation with obstructed cooling     

基于正弦基础激励的航天器结构模型修正方法

正弦振动试验是航天器系统级和单机产品需要开展的常规试验,充分利用工程中积累的正弦试验数据进行结构模型修正具有重要的工程意义。文章首先介绍了基础激励下结构模型修正方法,通过矩阵分块、待修正参数归一化、参与修正的频率点选择等步骤,推导出基于基础激励的模型修正公式;然后对国际通用算例GARTEUR桁架结构的有限元模型进行修正,分析修正后模型在修正频段内和修正频段外计算所得模态频率,验证修正后模型对模态频率的复现和预示能力,通过对比试验模型、分析模型和修正后模型中4个典型节点的响应曲线,检验修正后模型精度。结果表明:修正后模型的模态频率和响应曲线均与试验模型趋于一致,证实了该修正方法对GARTEUR结构修正的有效性。     

用Kane方法建立末敏弹减速和稳态扫描段模型

引入多刚体运动模型，详细分析了伞刚体和弹刚体的受力和运动特性，运用Kane方法建立末敏弹在减速运动和稳态扫描段的完整运动模型，并进行数字仿真，仿真结果与实验结果有很好的一致性，并充分显示了该模型在数字仿真中的优越性。     

V.L.A. observations of flare build-up in coronal loops

Very Large Array (V.L.A.) measurements at 20 cm wavelength map emission from coronal loops with second-of-arc angular resolution at time intervals as short as 3.3 seconds. The total intensity of the 20 cm emission describes the evolution and structure of the hot plasma that is detected by satellite X-ray observations of coronal loops. The circular polarization of the 20 cm emission describes the evolution, strength and structure of the coronal magnetic field. Preburst heating and magnetic changes that precede burst emission on time scales of between 1 and 30 minutes are discussed. Simultaneous 20 cm and soft X-ray observations indicate an electron temperature $\text{T}{}_{\mathrm{e}}\textcolor{red}{}\text{2.5 × 10}{}^7\text{K}$ and electron density $\text{N}{}_{\mathrm{e}}\textcolor{red}{}\text{10}{}^{10}\text{cm}{}^{\mathrm{?3}}$ during preburst heating in a coronal loop that was also associated with twisting of the entire loop in space. We also discuss the successive triggering of bursts from adjacent coronal loops; highly polarized emission from the legs of loops with large intensity changes over a 32 MHz change in observing frequency; and apparent motions of hot plasma within coronal loops at velocities V > 2,000 kilometerspersecond.     

Multiple wavelength observations of flaring active regions

We present observations of flaring active regions with the Very Large Array (V.L.A. at 6 cm and 20 cm wavelengths) and the Westerbork Synthesis Radio Telescope (W.S.R.T. at 6 cm wavelength). These are compared with photospheric magnetograms (Meudon) and with Hα and offband Hα photographs (Big Bear and Ottawa River Solar Observatories). The 6 cm radiation of these active regions marks the legs of dipolar loops which have their footpoints in lower-lying sunspots. The intense, million degree radiation at 6 cm lies above sunspot umbrae in coronal regions where the longitudinal magnetic field strength H_? = 600 Gauss and the height above the sunspot umbrae h = 3.5±0.5 × 10⁹ cm. Circularly polarized horseshoe structures at 6 cm ring the sunspot umbrae. The high degree of circular polarization (?_c = 95%) of the horseshoes is attributed to gyroresonant emission above sunspot^? penumbrae. The 20 cm radiation of these active regions exhibits looplike coronal structures which extend across regions of opposite magnetic polarity in the underlying photosphere. The 20 cm loops are the radio wavelength counterparts of the X-ray coronal loops. We infer semilengths L = 5 × 10⁹ cm, maximum electron temperatures T_e(max) = 3 × 10⁶ K, emission measures ∫N_e²d$\text{l}$ = 10²⁸ cm^?5, and electron densities N_e = 10⁹ cm^?3 (or pressures p = 1 dyn cm^?2) for the 20 cm bremsstrahlung. A total of eight solar bursts were observed at 6 cm or 20 cm wavelength with second-of-arc angular resolution. The regions of burst energy were all resolved with angular sizes between 5″ and 30″, brightness temperatures between 2 × 10⁷ K and 2 × 10⁸ K, and degrees of circular polarization between 10% and 90%. The impulsive phase of the radio bursts are located near the magnetic neutral lines of the active regions, and between the flaring Hα kernels which mark the footpoints of magnetic loops. In one case there was preburst heating in the coronal loop in which a burst occurred. Snapshot maps at 10 s intervals reveal interesting burst evolution including rapid changes of circular polarization and an impulsive burst which was physically separated from both the preburst radio emission and the gradual decay phase of the burst.     

超临界碳氢燃料蒸汽重整一维模型研究

为了获得关键参数对超临界碳氢燃料蒸汽重整化学热沉分布特性的影响,建立了超临界碳氢燃料蒸汽重整非稳态一维计算模型,通过与实验数据的对比验证了模型的准确性,并基于该模型采用RP-3的四组分替代模型对RP-3蒸汽重整过程中入口流速、压力和含水量等关键参数对热沉沿流向分布特性的影响进行了研究。结果表明：随着入口流速的增加,蒸汽重整反应化学热沉的峰值减小,且出现峰值的位置逐渐向出口移动。随着压力的升高,相同位置处的化学热沉都减少,但是出现峰值的位置不变。在入口含水量由5%增大到12%的过程中,微通道同一位置处的化学热沉增大,且化学热沉的最大值也是增大的,峰值出现的位置向微通道出口移动。