GAP／AN推进剂的应用与研制进展

概述了ＧＡＰ／ＡＮ推进剂的特性，研制状况及发展潜力，针对目前该推进剂的各项性能水平（能量性能，燃烧性能，力学性能）提出了该推进剂存在的问题及改善方法。     

Thermospheric neutral density response to solar forcing

Recent measurements by the Solar EUV (Extreme Ultra Violet) Experiment (SEE) aboard the Thermosphere–Ionosphere–Mesosphere Energetics and Dynamics satellite (TIMED) provide solar EUV spectral irradiance with adequate spectral and temporal resolution, and thus the opportunity to use solar measurements directly in upper atmospheric general circulation models. Thermospheric neutral density is simulated with the NCAR Thermosphere–Ionosphere–Electrodynamic General Circulation Model (TIEGCM) using TIMED/SEE measurements and using the EUVAC solar proxy model. Neutral density is also calculated using the NRLMSISE-00 empirical model. These modeled densities are then compared to density measurements derived from satellite drag data. It is found that using measured solar irradiance in the general circulation model can improve density calculations compared to using the solar proxy model. It is also found that the general circulation model can improve upon the empirical model in simulating geomagnetic storm effects and the solar cycle variation of neutral density.     

小展弦比压气机转子叶片颤振研究

针对小展弦比压气机转子叶片特点,在能量法计算基础上提出了两种颤振评判方法,即首先利用结构动力学分析结果对叶片频率分离度、振型和共振进行分析,判断某压气机小展弦比转子叶片存在高阶耦合颤振的可能;然后将结构动力学得到的振动位移插值到气动网格上,进行三维非定常黏性流场计算,得到非定常气动功,判断叶片是否存在失速颤振的可能.最后综合利用两部分分析结果和试验及断口分析情况,综合给出该小展弦比压气机叶片因失速颤振和耦合颤振共同作用,导致叶片在短时间内出现了裂纹.      

计算域大小对大涡模拟计算结果的影响

为了节省计算资源,提升计算效率,在保证计算结果准确的前提下,尽可能选取较小的计算域显得尤为重要。针对该问题,分别沿槽道的展向和流向选取不同的计算尺度(053πδ×2δ×0177πδ、πδ×2δ×05πδ、2πδ×2δ×πδ、3πδ×2δ×15πδ,δ为槽高的一半),在相同的计算条件且设置均满足大涡模拟计算要求的前提下,对摩擦雷诺数为540和930两种摩擦雷诺数下计算域大小对大涡模拟数值计算结果的影响进行了研究。结果发现:计算尺度不小于2πδ×2δ×πδ的计算域能很好的呈现湍流计算结果。此外,在摩擦雷诺数为930时,相同计算域下所能检测的范围均有所提升,得到的计算结果更加准确。     

用能量法研究玻璃幕墙面板的非线性弯曲

由于玻璃面板是典型的双模量材料板,所以应该采用双模量弹性理论研究玻璃面板在侧向力作用下的大位移问题。玻璃面板在侧向力作用下发生变形时,会形成各向同性的拉伸区和压缩区。因此,可把玻璃面板看成两种各向同性材料组成的层合板,采用双模量弹性理论建立了玻璃面板在侧向力作用下的静力平衡方程,利用静力平衡方程确定了玻璃面板的中性面位置。在此基础上,采用能量法研究了玻璃面板在侧向力作用下大位移问题,把能量法的计算结果与有限元计算结果进行了比较,验证了能量法的计算结果是可靠的。算例分析表明,玻璃面板拉压弹性模量相差较大,其挠度计算不宜采用相同弹性模量经典弹性理论,而应该采用双模量弹性理论。     

The first new application of the Mathematical Theory of Stochastic Processes to lunar and planetary science: Topography-Profile Diagrams of Mars

The Mathematical Statistics Theory (MST) and the Mathematical Theory of Stochastic Processes (MTSP) are different branches of the more general Mathematical Probability Theory (MPT) that can be used to investigate physical processes through mathematics. Each model of a stochastic process, according to MTSP, can provide one or more interpretations in the MST domain. A large body of work on impact crater statistics according to MST exists, showing cumulative crater frequency (N km⁻²) as a function of age (years) for some particular crater diameter. However, this is only one possible representation in the MST domain of the bombardment of the planetary surface modeled as a stochastic process according to MTSP. The idea that other representations are possible in the MST domain of the same stochastic process from MTSP has been recently presented. The importance of the approach is that each such mathematical-based interpretation can provide a large amount of new information. Coupled with MOLA data, Topography-Profile Diagrams (TPD) are one of the many examples that can provide a large amount of new information regarding the history of Mars. TPD consists of: (1) Topography-Profile Curve (TPC), which is a representation of the planet’s topography, (2) Density-of-Craters Curve (DCC), which represents density of craters, (3) Filtered-DCC (FDCC), which represents DCC filtered by a low-pass filter, included with the purpose of reducing the noise, and (4) Level-of-Substance-Over-Time Curve (LSOTC), which represents interpretation of the influence on the distribution of craters shown by FDCC. TPC uniquely corresponds to the computation of TPD, whereas DCC depends on algorithms for computing the elevation of each crater according to the topography, center coordinates, and radius of impact crater, and FDCC relies on the architecture of the custom designed low-pass filter for filtering DCC. However, all variations of DCC and FDCC, which includes the various impact crater data sets, showed a correlation among the density of craters and elevation over 70–80% of the planet surface. Additionally, if we assume that the ocean primarily caused the noted correlation, LSOTC offers a mathematical approach for estimating topographic change of the ocean’s extent over time. Accordingly, TPD is the first new practical application of MTSP to lunar and planetary sciences, showing correlation of topography to a physical process.     

高速无刷直流电机在磁悬浮惯性执行机构中的应用研究进展

为了满足新一代卫星平台高精度、高稳定度的需求,研制了一种磁悬浮惯性执行机构用功耗低、精度高、体积小、重量轻的高速无刷直流电机,提出了多约束条件下电机定子结构和转子磁体结构的设计优化原则及方法,并就高精度的锁相速度控制以及铁耗和转矩脉动的抑制方法进行了研究.对比分析了国内外高速永磁无刷直流电机在磁悬浮惯性执行机构中的应用研究现状,指明了所提出的设计原则和控制方法对提高磁悬浮惯性执行机构整体性能的有效性.     

双定子盘式永磁同步电机控制策略

对一种具有双定子的盘式永磁同步电机进行了讨论、分析与试验验证。双定子电机因其具有的高转矩密度、控制灵活等特点受到了越来越多的关注,然而在实际应用中,如何进行双定子的能量分配以使系统效率最优也成为了一个难点。因此,提出一种基于MAP图的转矩分配策略,并在以TMS320F28335为主控芯片的试验平台上对电机进行了试验验证。试验结果表明所提出的控制分配策略能有效地保证双定子电机系统高效运行。     

基于ADAMS的行星齿轮系刚柔耦合仿真局部缺陷识别

针对行星齿轮系在工作过程中出现的局部缺陷,将引起齿轮啮合异常,并导致冲击异常,其特征频率就会发生变化。现用ADAMS与ANSYS建立行星齿轮系的刚柔耦合模型,通过快速傅里叶变换（FFT）得到其啮合力的频域曲线,并分析无缺陷行星齿轮系的特征频率、行星轮齿局部缺陷的特征频率、太阳轮齿局部缺陷的特征频率。仿真结果与理论值吻合,说明了所建虚拟样机模型可靠,得到无缺陷行星齿轮系的特征频率是265.34Hz,行星轮齿局部缺陷的特征频率是17.67Hz,太阳轮齿局部缺陷的特征频率是36.13Hz,可用于识别行星齿轮系的行星轮或太阳轮局部缺陷。对行星齿轮系振动特性、可靠性的研究具有一定的指导意义。     

基于第二动力技术的TBCC综合能源展望

飞行器电能、液压能和气压能的功率需求由第二动力系统单独做功或提取发动机主轴功率供应。TBCC发动机模态转换后,第二动力系统无法从发动机主轴提取功率。因此,需要解决空天飞行器第二动力系统长时间大功率能量输出的问题。分析航空蓄电池、起动发电机、APU、GTS、ATS和RAT的技术特点、发展现状以及第二动力的发展趋势,结合高超声速飞行器的发展趋势,提出ATS/RAT组合和多电超导发动机/大比能的储能装置技术组合是实现空天高超声速飞行器综合能源的技术路线。