反推力装置运动学与动力学仿真

为了研究叶栅式反推力装置各部件在工作过程中的运动学与动力学特性,根据机构运动原理对反推力装置进行简化并建立了运动学与动力学数学模型。以滑动整流罩位移与阻流门所受气动负荷为输入进行运动学与动力学仿真,得到了反推力装置各部件的位移、速度及受力特性曲线,并对比分析了在不同尺寸参数下各部件特征点的运动轨迹和反推力装置负载力变化。结果表明:运动学及动力学仿真结果与工程实际相符；反推力装置机构参数选择不合理时,各设计点会发生干涉现象并导致机构无法运动;机构参数变化对负载力最大值影响尤为突出,在阻流门AC段长度值增大6%,阻流门CB段长度值减小9%的情况下,负载力正向最大值将增大19.53%,负向最大值增大12.67%。研究方法及研究结果可为反推力装置运动学及动力学分析,以及为反推力装置机构优化设计提供参考。      

基于TLE的弹道系数计算方法及应用分析

针对仅使用两行要素（Two Line Element，TLE）作为数据源的应用需求，研究了基于TLE轨道衰减的弹道系数计算方法。介绍了一种常用的基于两组TLE的直接计算法，分析TLE选取间隔对结果精度的影响；提出了一种基于多组TLE的迭代计算方法，以降低异常TLE对计算结果的影响；从弹道系数计算效果、在再入预报中的应用等方面对这两种方法进行比较分析。结果表明，两种方法各有优劣，基于多组TLE的迭代计算法稳定性更高、受TLE精度的影响更小；由于数据区间更短，基于两组TLE的计算结果对短期轨道衰减特性反应得更准确，用于临近再入时的预报效果更好。     

Investigating the Coronal Mass Ejections associated with DH type-II radio bursts and solar flares during the ascending phase of the solar cycle 24

We studied a set of 74 CMEs, with shedding the light on the halo-CMEs (HCMEs), that are associated with decametric – hectometric (DH) type-II radio bursts (1–16?MHz) and solar flares during the period 2008–2014. The events were classified into 3 groups (disk, intermediate, and limb events) based on their longitudinal distribution.We found that the events are mostly distributed around 15.32° and 15.97° at the northern and southern solar hemispheres, respectively. We found that there is a clear dependence between the longitude and the CME’s width, speed, acceleration, mass, and kinetic energy. For the CMEs’ widths, most of the events were HCMEs (～62%), while the partial HCMEs comprised ～35% and the rest of events were CMEs with widths less than 120°. For the CMEs’ speeds, masses, and kinetic energies, the mean values showed a direct proportionality with the longitude, in which the limb events had the highest speeds, the largest masses, and the highest kinetic energies. The mean peak flux of the solar flares for different longitudes was comparable, but the disk flares were more energetic. The intermediate flares were considered as gradual flares since they tended to last longer, while the limb flares were considered as impulsive flares since they tended to last shorter.A weak correlation (R?=?0.32) between the kinetic energy of the CMEs and the duration of the associated flares has been noticed, while there was a good correlation (R?=?0.76) between the kinetic energy of the CMEs and the peak flux of the associated flares. We found a fair correlation (R?=?0.58) between the kinetic energy of the CMEs and the duration of the associated DH type-II radio bursts.     

激光动态液位测量技术研究

如今,运载火箭大量使用液氧、煤油等液体推进剂,其液位测量技术主要有浮子式、激光式、电容式、雷达式等。介绍并实现了一种激光液位测量系统,该系统体积小、功耗低,可适应多种测量环境,能满足航天燃料液位测量高精度、高动态、连续稳定测量的要求。系统利用相位式激光测距技术,通过测量激光回波信号的相位延迟,计算激光光程从而得到距离数据并通过客户端进行直观展示和数据存储。系统最大测量距离可达100 m,精度为±1 mm。该系统为非接触测量,耐腐蚀,通过加入反射板可实现透明、非透明液体测量。     

基于区间灰色不确定语言的工作类型优化方法

针对飞机维修任务工作类型优化过程中的模糊与灰色问题,采用区间灰色不确定语言变量建立工作类型的评价指标和决策模型,提出了军机维修任务工作类型优化方法。对优化方法进行了实例分析,工作类型排序结果和数据对比结果验证了优化方法的可行性与有效性。在某军机上对优化方法进行了工程应用,完成192项初始维修任务工作类型优化,应用结果表明了该优化方法具备良好的工程应用价值,可有效提升工作类型合理性。     

WSO-UV project

During last three decades, astronomers have enjoyed continuous access to the 100–300 nm ultraviolet (UV) spectral range where the resonance transitions of the most abundant atoms and ions (at temperatures between 3000 and 300 000 K) reside. This UV range is not accessible from ground-based facilities. The successful International Ultraviolet Explorer (IUE) observatory, the Russian ASTRON mission and successor instruments such as the Galaxy Evolution Explorer (GALEX) mission or the COS and STIS spectrographs on-board the Hubble Space Telescope (HST) prove the major impact of observations in the UV wavelength range in modern astronomy. Future access to space-based observatories is expected to be very limited. For the next decade, the post-HST era, the World Space Observatory – Ultraviolet (WSO–UV) will be the only 2-m class UV telescope with capabilities similar to the HST. WSO–UV will be equipped with instruments for imaging and spectroscopy and it will be a facility dedicated, full-time, to UV astronomy. In this article, we briefly outline the current status of the WSO–UV mission and the science management plan.     

有翼再入飞行器气动外形集成设计优化

气动外形设计是有翼再入飞行器（RV-W）的关键技术之一。分析了气动参数对再入飞行性能的影响,探讨了有翼再入飞行器气动外形设计的规律和准则。基于上述设计准则,以类X-37B飞行器为研究对象,集成几何参数化建模、气动力、气动热、热防护等学科快速分析方法,采用多学科设计优化方法,以最优气动特性为目标对飞行器气动外形进行了优化;得到优化气动外形后,对飞行器热防护系统（TPS）进行了轻量化设计优化。结果表明,优化外形的气动特性相比初始外形得到了较大的提升,设计优化得到的热防护系统重量占比（8.7%）优于同类飞行器的热防护系统重量占比统计数据,说明了本文有翼再入飞行器气动外形集成设计优化方法的有效性,可为同类飞行器提供参考。     

基于任务科目的直升机飞行品质评定试飞技术研究

主要对ADS-33E中飞行品质评定的要求进行分析,从任务科目、响应类型和可用感示环境3个维度进行飞行品质的等级评定研究,提出了直升机飞行品质综合评定的试飞技术研究思路,并对某型号直升机的试飞结果和有关问题进行了初步分析。     

结冰对民用飞机飞行性能的影响分析

在获取民用飞机适航合格审定证明前,必须通过飞行试验,并在试验中演示验证民用飞机能在CCAR25部附录C确定的连续和间断的最大结冰状态下安全运行。基于此背景,计算并得到某型机两种构型在45min待机冰型下的飞行性能,与无冰状态下对应构型的飞行性能进行对比分析。结果表明,结冰对飞机的飞行性能具有较大的影响。     

抑波槽宽度对水陆两栖飞机喷溅性能影响对比试验研究

抑波槽宽度合理性直接影响抑制喷溅的效果。通过两个抑波槽宽度的单船身模型拖曳水池对比试验,比较同一状态两者喷溅包络线,分析抑波槽宽度变化对飞机喷溅性能影响,表明减小抑波槽宽度使螺旋桨处喷溅高度增加19%以上,使襟翼处喷溅高度降低54%。