基于ISIGHT的某型飞机发动机短舱防火结构设计

以某型发动机短舱为研究对象,依据 CCAR-25-R4适航条款要求,对短舱结构进行了防火区域的界定为考核短舱防火结构的受力状况,建立短舱后段防火结构有限元模型,完成了5种工况下的有限元分析:综合计算结果,选取其中最严重受力工况,结合发动机的安装和维护需求,开展短舱后段防火结构优化分析:最后以短舱中典型的钛合金防火平板、焊接板2种结构为例,开展了结构防火试验。试验结果表明,防火结构有良好的防火性,满足飞机设计要求。通过以上的结构优化、材料性能试验等流程,最终形成了一套短舱防火结构设计方法,降低了结构重量,加快了设计流程。     

连接器支架结构优化设计分析

某型连接器支架普遍出现断裂现象,经判断原因是动强度设计不合理,在振动载荷作用下发生疲劳破坏,为了确保支架不出现结构损伤,保证飞行安全,需要进行结构优化设计分析。基于克希霍夫理论,采用有限元分析手段,通过改变厚度、材料与结构形式的方法,对支架进行模态分析与随机响应分析,最终得到了在满足动强度设计要求的情况下质量最轻的支架。根据分析结果总结了一种结构优化设计分析的流程:先改结构形式,用相对系数判断优劣;再选疲劳性能好的材料;最后选择合适的厚度。该流程在本文中得到有效实施,可在今后用于相似结构的优化设计分析。     

基于复合形与神经网络的机翼结构优化设计

从元件位置和元件尺寸两个方面考虑,提出了一种全局结构优化设计方法。利用NASTRAN完成尺寸优化,利用神经网络对NASTRAN优化结果进行映射,用复合形法进行位置寻优,最终完成了机翼结构的优化。算例表明利用神经网络来预测NASTRAN优化结果有较高的精度与适用性,本文所提方法可行、正确,具有很高的效率。     

复合材料结构健康主动监测中激励信号的优化

利用L am b波频散方程及其数值求解得到的频散曲线,对L am b波模式及激励信号中心频率范围进行预测。建立了试验测试系统,利用集成在复合材料层合板上的PZT压电陶瓷片作为驱动器和传感器,激励并接收结构中激发的L am b波信号。对具有不同函数形式、中心频率和波峰数的信号激励,结构中传播的L am b波模式进行试验研究,为激励信号的选择与优化提供依据。利用H ilbert-Huang变换及H ilbert谱提取传感器信号特征,提出了L am b波信号在结构中传播时的能量衰减率和损伤敏感度两个考察指标,并据此对激励信号进行优化。实验结果表明,优化后的激励信号在结构中能激发出单一模式的L am b波(S0模式),有效地抑制了多模式现象的出现。同时,激发出的L am b波具有最低的能量衰减和最高的损伤灵敏度,响应信号特征明显,便于损伤识别。     

低速溅射小行星表面采样的动力学仿真

开发了适用于小行星环境的大规模三维离散元程序DEMBody,针对低速射弹溅射表层风化层的小行星采样方案,仿真了相同质量不同形状的射弹在微重力环境下垂直射入颗粒床的过程,研究了溅射物质在采样器中的运动历程及最终收集质量与射弹形状的关系。结果表明,90°锥形射弹的采样效率最高。     

复杂动力学模型下星载天线跟瞄控制技术研究

针对星载天线动力学复杂这一问题,从天线系统刚柔耦合动力学建模、指向跟踪控制以及振动抑制等方面研究了柔性星载运动部件的指向控制方法。首先,通过描述系统几何拓扑关系建立系统运动学方程,从而简化动力学建模过程;之后,利用假设模态法,对天线反射面挠性进行建模;最后,将拉格朗日方程与挠性关节模型相结合,从而建立了星载天线非线性刚柔耦合动力学模型。在以上复杂动力学建模的基础上,采用分层设计的思路进行了控制策略设计：先运用基于计算力矩法的滑模控制器得到不考虑挠性关节的耦合控制律,从而保证卫星基体的稳定性以及天线挠性反射面的振动抑制;再使用反步法对挠性关节进行控制,实现对天线反射面的指向精度控制。最后,讨论了动力学参数不确定性对系统跟踪指向控制的影响并采用数学仿真的方式验证了相关动力学模型与控制算法。仿真结果表明该方法能较好地实现对星载天线的指向跟踪控制以及振动抑制,提高星载天线的动态指向精度。     

类蛛网状盘式谐振微陀螺的抗冲击性能与结构误差仿真分析

具有导航级潜能的盘式谐振微陀螺是国际研究最热门的一类微机械陀螺,在此基础上设计了一款频率裂解小的类蛛网状盘式谐振微陀螺。通过有限元仿真软件进行了模态分析和冲击分析,仿真结果表明类蛛网状盘式谐振微陀螺工作模态与寄生模态最小频差为3.9kHz,可承受的冲击载荷加速度高达25000g。此外,开展了晶向误差和工艺误差等结构误差对频率裂解影响的仿真研究,结果表明,其比圆环状盘式谐振陀螺在频率裂解上具有更低的结构误差敏感度。综上说明该结构能有效抑制寄生模态干扰、抗冲击性能强且结构误差鲁棒性好,具有较好的发展前景。     

Modeling novel methodologies for unmanned aerial systems–Applications to the UAS-S4 Ehecatl and the UAS-S45 Bálaam

The rising demand for Unmanned Aerial Systems(UASs) to perform tasks in hostile environments has emphasized the need for their simulation models for the preliminary evaluations of their missions. The efficiency of the UAS model is directly related to its capacity to estimate its flight dynamics with minimum computational resources. The literature describes several techniques to estimate accurate aircraft flight dynamics. Most of them are based on system identification. This paper presents an alternative methodology to obtain complete model of the S4 and S45 unmanned aerial systems. The UAS-S4 and the UAS-S45 models were divided into four sub-models, each corresponding to a specific discipline: aerodynamics, propulsion, mass and inertia, and actuator. The‘‘aerodynamic" sub-model was built using the Fderivatives in-house code, which is an improvement of the classical DATCOM procedure. The ‘‘propulsion" sub-model was obtained by coupling a two-stroke engine model based on the ideal Otto cycle and a Blade Element Theory(BET) analysis of the propeller. The ‘‘mass and the inertia" sub-model was designed utilizing the Raymer and DATCOM methodologies. A sub-model of an actuator using servomotor characteristics was employed to complete the model. The total model was then checked by validation of each submodel with numerical and experimental data. The results indicate that the obtained model was accurate and could be used to design a flight simulator.     

一种温度动态调节方法及其动态性能仿真研究

航空气源模拟试验台主要用于模拟不同飞行状态时发动机给空气管理系统的供气,由于飞机爬升、降落时发动机供气参数会急剧变化,因此航空气源模拟试验台需具备动态能力.基于一种温度动态调节方法,在合理简化的基础之上采用NHT方法对其温度动态性能进行了仿真研究,仿真结果表明该温度动态调节方法能够满足温度动态性能需求,对动态航空气源模拟试验台的设计选型有较高的参考价值.     

Observations of a quasi-90-day oscillation in the MLT winds and tides over an equatorial station using meteor radar winds

An evident signature of a least studied quasi-90-day oscillation is found in the winds and tides in the MLT from an equatorial station, São João do Cariri (7.4°S, 36.5°W). The oscillation is found to appear mainly in certain intervals with small but appreciable seasonal (fourth harmonic of annual oscillation) contribution. The maximum amplitude of the oscillation is found to be around 10 m/s in the zonal wind. The enhancement peak of the oscillation exhibits downward movement indicating a plausible role of upward moving waves/tides in carrying its imprint from below to the MLT. Similar oscillation feature in the tropospheric zonal wind and ozone may imply its lower atmospheric origin as a component of the intraseasonal oscillation (ISO) that moves upward by modulating the tides. Subsequently, the propagating tides (mainly semidiurnal) are enhanced by the ozone in the stratosphere through absorption of solar UV radiation and finally manifest the oscillation in the MLT. Consistency of the present findings with the past investigations are observed in some aspects of the oscillation, whereas existing mismatches in others are believed to be due to geophysical variability depending on space and time among various locations on the globe.