可伸缩挠性结构的稳定性研究

研究了一类可伸缩挠性梁结构的稳定性。主要结论有：一般可伸缩挠性梁结构的动力学可由刚体姿态运动、挠性体振动和梁伸缩运动相耦合的混合偏微分方程和常微分方程描述;结构振动与转动能量的耗散与积聚取决于梁的伸缩运动,在伸展过程中系统的能量被耗散,在收缩过程中系统能量被积聚,在平台保持过程系统能量维持不变。因此,梁的伸展过程是稳定的,梁的收缩过程是不稳定的,而平台保持过程是临界稳定的。     

数控系统在S域和P域的分析设计方法

讨论一种典型的采样控制系统──直接数字控制（ＤＤＣ）系统（简称数控系统）在Ｓ域和Ｐ域的分析设计方法。根据采样控制系统理论,从数控系统在Ｚ平面的稳定性判据出发,利用ｔｕｓｔｉｎ变换（Ｐ变换）,通过Ｚ平面、Ｓ平面和Ｐ平面之间的映像关系,导出数控系统在Ｓ域和Ｐ域的稳定性判据,进而提出了数控系统在Ｓ域和Ｐ域的分析设计方法,并详细说明了这两种设计方法的具体方法与步骤。     

基于拓扑优化的航空发动机滑油箱支架设计

支架是航空发动机滑油箱组件中的重要部件,用于连接和固定滑油箱组件中的箍带.但现有支架设计会引起与之相连的箍带承受偏心拉力,导致结构应力水平偏高进而发生疲劳破坏.本文提出了一种考虑结构局部刚度的拓扑优化方法,能够在提升支架整体刚度的同时兼顾局部刚度,使支架的刚度分布更加合理,进而显著降低与之相连的箍带的应力水平.利用该优...     

粉末GH4169 合金中的原始颗粒边界问题

探讨了粉末GH4169高温合金中的原始颗粒边界的形成机理、其对合金组织性能的影响以及消除措施等。结果表明:粉末GH4169合金中原始颗粒边界组织主要由MC碳化物构成,而在粉末成型前进行预热处理可以有效抑制原始颗粒边界组织的生成,提高合金综合性能。     

整级环境下涡轮叶片型面加工几何偏差影响的不确定性分析

加工等过程中产生的几何偏差会导致涡轮叶片气动性能及工作状态发生显著变化,对该影响的准确评估与合理分析具有重要意义.本文提出了一种考虑三维型面几何偏差对气动性能影响的不确定性计算分析方法,包括随机叶型几何建模、不确定性量化计算和敏感性分析等,并结合某一单级高压涡轮进行分析.基于随机过程理论和主成分分析法,参考现有叶片加工...     

Upgrading CCIR's foF2 maps using available ionosondes and genetic algorithms

We have developed a new approach towards a new database of the ionospheric parameter $f_{o}F2$. This parameter, being the frequency of the maximum of the ionospheric electronic density profile and its main modeller, is of great interest not only in atmospheric studies but also in the realm of radio propagation. The current databases, generated by CCIR (Committee Consultative for Ionospheric Radiowave propagation) and URSI (International Union of Radio Science), and used by the IRI (International Reference Ionosphere) model, are based on Fourier expansions and have been built in the 60s from the available ionosondes at that time. The main goal of this work is to upgrade the databases by using new available ionosonde data. To this end we used the IRI diurnal/spherical expansions to represent the $f_{o}F2$ variability, and computed its coefficients by means of a genetic algorithm (GA). In order to test the performance of the proposed methodology, we applied it to the South American region with data obtained by RAPEAS (Red Argentina para el Estudio de la Atmósfera Superior, i.e. Argentine Network for the Study of the Upper Atmosphere) during the years 1958–2009. The new GA coefficients provide a global better fit of the IRI model to the observed $f_{o}F2$ than the CCIR coefficients. Since the same formulae and the same number of coefficients were used, the overall integrity of IRI’s typical ionospheric feature representation was preserved. The best improvements with respect to CCIR are obtained at low solar activities, at large (in absolute value) modip latitudes, and at night-time. The new method is flexible in the sense that can be applied either globally or regionally. It is also very easy to recompute the coefficients when new data is available. The computation of a third set of coefficients corresponding to days of medium solar activity in order to avoid the interpolation between low and high activities is suggested. The same procedure as for $f_{o}F2$ can be perfomed to obtain the ionospheric parameter M(3000)F2.     

宽高比及表面粗糙度对矩形微尺度通道流动特性的影响

实验研究了不同宽高比矩形金属微尺度通道的流动特性,并与硅通道对比来探究表面粗糙度的影响。金属微尺度通道宽为0.4mm,通道宽高比分别为0.50、0.67、和1.00,相对表面粗糙度范围为0.1609%~0.2145%。硅通道宽度及高度都为0.4mm,相对表面粗糙度为0.00325%。实验工质为空气,实验的雷诺数范围是250~3000。实验结果表明:在粗糙微尺度通道会发生转捩提前,并且转捩雷诺数随着宽高比增大而减小。在层流区,微尺度矩形通道摩擦因数随着雷诺数增大而减小,在转捩区出现明显增大后再减小。表面粗糙度很小时,未发现转捩提前现象。      

基于雷诺平均Navier-Stokes方程的表面传热系数计算

采用有限体积法数值求解控制二维绕流的雷诺平均Navier-Stokes(RANS)方程组,计算了光滑和粗糙NACA0012翼型以及圆柱表面的局部表面传热系数.分析了近壁面网格间距、湍流模式和表面粗糙度模型对数值计算结果的影响.结果表明:切应力输运(SST)湍流模型能够区分层流和湍流边界层的对流传热特性,并能预测转捩的发生;采用Spalart-Allmaras(S-A) 扩展模型能够计算粗糙壁面的对流传热系数,但采用忽略转捩函数的S-A模型不能有效计算层流边界层的传热系数.当近壁面网格间距接近10-5量级的黏性子层时,在光滑和粗糙壁面都能得到准确的传热系数分布.结合合适的近壁面网格间距,湍流模式和表面粗糙度模型可以得到与实验数据十分接近的表面传热系数曲线.通过与求解不可压缩RANS方程得到的结果比较后发现,不可压缩RANS方程主要忽略了压缩和黏性耗散效应,这种效应可以通过绝热升温项的形式并入总体热分析.      

Grinding force and surface quality in creep feed profile grinding of turbine blade root of nickel-based superalloy with microcrystalline alumina abrasive wheels

Creep feed profile grinding of the fir-tree blade root forms of single crystal nickel-based superalloy was conducted using microcrystalline alumina abrasive wheels in the present study. The grinding force and the surface quality in terms of surface topography, subsurface microstructure, microhardness and residual stress obtained under different grinding conditions were evaluated comparatively. Experimental results indicated that the grinding force was influenced significantly by the competing predominance between the grinding parameters and the cross-sectional root workpiece profile. In addition, the root workpiece surface, including the root peak and valley regions, was produced with the large difference in surface quality due to the nonuniform grinding loads along the root workpiece profile in normal section. Detailed results showed that the surface roughness, subsurface plastic deformation and work hardening level of the root valley region were higher by up to 25%, 20% and 7% in average than those obtained in the root peak region, respectively, in the current investigation. Finally, the superior parameters were recommended in the creep feed profile grinding of the fir-tree blade root forms. This study is helpful to provide industry guidance to optimize the machining process for the high-valued parts with complicated profiles.     

Investigation of ionospheric response to two moderate geomagnetic storms using GPS–TEC measurements in the South American and African sectors during the ascending phase of solar cycle 24

The responses of the ionospheric F region using GPS–TEC measurements during two moderate geomagnetic storms at equatorial, low-, and mid-latitude regions over the South American and African sectors in May 2010, during the ascending phase of solar cycle 24, are investigated. The first moderate geomagnetic storm studied reached a minimum Dst value of −64 nT at 1500 UT on 02 May 2010 and the second moderate geomagnetic storm reached a minimum Dst value of −85 nT at 1400 UT on 29 May 2010. In this paper, we present vertical total electron content (VTEC) and phase fluctuations (in TECU/min) from Global Positioning System (GPS) observations from the equatorial to mid-latitude regions in the South American and African sectors. Our results obtained during these two moderate geomagnetic storms from both sectors show significant positive ionospheric storms during daytime hours at the equatorial, low-, and mid-latitude regions during the main and recovery phases of the storms. The thermospheric wind circulation change towards the equator is a strong indicator that suggests an important mechanism is responsible for these positive phases at these regions. A pre-storm event that was observed in the African sector from low- to the mid-latitude regions on 01 May 2010 was absent in the South American sector. This study also showed that there was no generation or suppression of ionospheric irregularities by storm events. Therefore, knowledge about the suppression and generation of ionospheric irregularities during moderate geomagnetic storms is still unclear.