大型挠性充液卫星的动力学模型

研究了带有多个挠性附件和液体燃料贮箱的中继卫星系统的动力学建模问题。给出了微重力下小幅线性晃动等效模型基本参数，用混合坐标法描述中继卫星系统的构形，利用虚功原理推导出的矩阵形式的中继卫星动力学模型简洁且具有一般性，适用于许多开链飞行器系统。     

固体微推力器设计与数值分析

设计了两种基于微光机电技术的固体微推力器结构,其中一种结构具有不连续的非正常拉瓦尔喷管。采用数值计算方法对不同的设计进行了内弹道、燃气流动过程和热损失的数值分析。结果表明:不连续的非正常拉瓦尔喷管同样能够将推进剂燃气加速到超声速,其比冲性能与正常拉瓦尔喷管相当;微光机电技术常用的硅材料会造成推力器比冲性能较大量级的下降,而绝热性能良好的玻璃或陶瓷材料可以有效提高微推力器的比冲性能。     

舰载机前起落架突伸的动力学分析

研究了舰载机前起落架的突伸运动，针对这个问题，文中建立了一个两自由度的质量－弹簧－阻尼器的力学模型。推导出突伸运动方程以及两种不同形式的双气室缓冲器的非线性气体弹簧力和油液阻尼力的计算公式，并通过对已有试验结果的验算说明了本模型的可行性，利用该模型，用数值方法分析，校核了某舰载机的初步设计方案，计算得到了前起落架突伸运动的位置，速度曲线，并给出突伸期间飞机在甲板上的滑行距离和攻角的增量。文中还讨论     

航天飞行中的稀薄气体动力学

飞船、宇航探测器、航天飞机等复杂外形航天器给气体动力学，包括稀薄气体动力学提出了新的要求。本文简要介绍了为计算过渡领域中气动力与热而发展的基于位置元概念的DSMC方法的通用算法。该方法解决了计算物面通量量的技术难点并已用于模拟圆球、飞船、类航天飞机的绕流。正在进行的航天实践，如麦哲伦飞船对金星的探测、行星大气中的气动制动、伽利略飞船的木星之行、尾屏蔽在太空中获得高真空的实验等等提出了新的气动力问题，稀薄气体动力学和DSMC方法是有力的工具。     

考虑高载和阻尼介质时刚塑性圆板的塑性动力分析

本文研究了阻尼介质对刚塑性圆板在高载(冲击荷载)作用下塑性动力响应的影响,得到了解析解并对此解进行了讨论。当阻尼介质参数趋于零时,本文结果与无阻尼解一致。文中还画出了荷载与阻尼介质对圆板运动时间和板中心点残余挠度的影响曲线。     

基于多体分析的对接机构结构锁动力学仿真研究

分析了周边式空间对接机构结构锁的执行机构的特点，以及运用现有动力学分析软件解决此问题的困难；继而采用多体动力学建模方法，建立了结构锁执行机构的动力学模型，并针对本模型的特殊性采用了变步长的广义坐标分块求解算法；最后通过求解模型得到了机构的动力学特性曲线，证明了滚珠丝杆和弹簧复合机构作为结构锁执行部件是可行的．     

微重力下管肋式空间辐射器的整体优化分析

建立了向一重力环境下管肋式空间辐射器传热过程的数学模型，并以单质量散热量最大和热载体驱动功率最小为优化目标，对管式空间辐射器进行了优化分析。     

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.