可倾瓦径向滑动轴承绝热瞬态过程分析

为了研究可倾瓦径向轴承在载荷扰动下的绝热瞬态行为.对瞬态油膜压力和温度分布采用了时变的Reynolds方程和能量方程, 建立了轴颈及瓦块动力学方程.应用有限差分及Newton-Raphson法对方程联立求解, 模拟了阶跃载荷冲击工况下可倾瓦径向轴承热瞬态非线性响应过程.给出瞬态过程中油膜最高温度、最小膜厚等参数的变化规律.结论认为瞬态过程中, 油膜温度和膜厚变化量较大, 油膜温度和膜厚响应有一定的超调量, 瞬态过程中有可能因油膜温升过高或膜厚太小而导致失效.      

基于混合战略均衡双寡头航空公司定价博弈研究

利用产品差异化理论和博弈理论,建立了双寡头航空公司市场竞争定价的不完全信息静态博弈模型,假定双方经营相同航线、选择相同机型、面临相同旅客,而在产品价格和服务水平方面存在差异性,在文献【1】中证明了这种博弈不存在纯策略均衡,按照纳什均衡解存在性理论,对混合战略均衡进行求证,得出结论：双方价格和服务水平的大小关系一致时,其市场份额和期望利润的关系与之相同;双方两因素关系随机变化时,其市场份额及期望利润同其变化程度有关,即结果不确定。     

限制励磁方法在无刷交流发电机数字电压调节器中的应用

分析了限制励磁电流功能对无刷交流发电机加载过渡过程的影响,得到了设置励磁电流限制值的方法。采用了曲线拟合的方法对变速无刷交流发电机的励磁电流限制值进行了设置,而且拟合公式是与理论推导相一致的。按照本文的励磁电流限制值拟合方法可以保证无刷交流发电机在整个转速范围内都有良好的加载动态性能。     

Io’s Atmosphere and Surface-Atmosphere Interactions

Our knowledge of Io’s atmosphere has improved dramatically in the last fifteen years, with a wealth of new observational data at millimeter, UV and IR wavelengths, and the development of numerous models describing its horizontal and vertical structure, composition, photochemistry and plasma interaction. Io’s atmosphere is dominantly composed of SO2, present mostly at low-tomid latitudes with column densities of a few 1016 cm⁻² and important (factors of 5-10) longitudinal variations. Minor compounds include SO, S₂, and NaCl. Sublimation equilibrium with SO₂ frost and direct volcanic output coexist to maintain Io’s atmosphere against condensation, photolytic and escape losses.     

复合材料喷管非线性瞬态热应力分析

本文给出了热弹性力学的理论公式．在考虑高温下复合材料参数随温度变化而变化的非线性因素的前提下，推导了结构瞬态温度场和热应力的有限元公式，并对一C／C复合材料火箭发动机喷管进行了温度场和热应力的分析。结果表明，在考虑非线性后，结构各处应力均较低，但在不同材料交界面附近出现很高应力，这在设计中应予以考虑。本算法思路简单且实用，在工程中有较大的参考意义。     

叶片非线性瞬态响应计算方法与参数选择

在计算叶片的岛撞击响应时，为提高计算精度及降低计算成本，需要为待解的非线性动力方程组制定一个合理的求解方案，这包括选择系数矩阵的算法与非线性动力方程组的解法，以及选择主要计算参数，本文介绍了当使用ＡＤＩＮＡ程序计算平板叶片在冲载荷下的非线性瞬态响应时，对计算方法与计算参数的选择，算例说明了时间步长的重要影响作用。     

用于推进的驻定斜爆轰的基本特征

基于驻定斜爆轰的基本守恒方程、多组元状态方程和考虑化学平衡移动的组元守恒方程，根据本文推导的迭代公式，计算了不同强度的驻定爆轰波后的平衡组分、反应热和绝热指数，讨论了驻定斜爆轰的基本特点、驻定条件和影响驻定的各种因素。     

Distributed online mission planning for multi-player space pursuit and evasion

There are three important roles in evasion conflict: pursuer, target and defender. Pur-suers’ mission is to access targets;targets’ mission is to escape from pursuers’ capture;defenders’ mission is to intercept pursuers who are potentially dangerous to targets. In this paper, a distributed online mission plan (DOMP) algorithm for pursuers is proposed based on fuzzy evaluation and Nash equilibrium. First, an integrated effectiveness evaluation model is given. Then, the details of collaborative mission planning which includes the co-optimization of task distributing, trajectory and corresponding maneuvering scheme are presented. Finally, the convergence and steadiness of DOMP are discussed with simulation results. Compared with centralized mission planning, DOMP is more robust and can greatly improve the effectiveness of pursuing. It can be applied to dynamic scenario due to its distributed architecture.     

Shear flow energy redistribution stipulated by the internal-gravity wavy structures in the dissipative ionosphere

The linear mechanism of generation, intensification and further nonlinear dynamics of internal gravity waves (IGW) in stably stratified dissipative ionosphere with non-uniform zonal wind (shear flow) is studied. In case of the shear flows the operators of linear problem are non-selfadjoint, and the corresponding Eigen functions – nonorthogonal. Thus, canonical – modal approach is of less use studying such motions. Non-modal mathematical analysis becomes more adequate for such problems. On the basis of non-modal approach, the equations of dynamics and the energy transfer of IGW disturbances in the ionosphere with a shear flow is obtained. Exact analytical solutions of the linear as well as the nonlinear dynamic equations of the problem are built. The increment of shear instability of IGW is defined. It is revealed that the transient amplification of IGW disturbances due time does not flow exponentially, but in algebraic – power law manner. The effectiveness of the linear amplification mechanism of IGW at interaction with non-uniform zonal wind is analyzed. It is shown that at initial linear stage of evolution IGW effectively temporarily draws energy from the shear flow significantly increasing (by an order of magnitude) own amplitude and energy. With amplitude growth the nonlinear mechanism turns on and the process ends with self-organization of nonlinear solitary, strongly localized IGW vortex structures (the monopole vortex, the transverse vortex chain or the longitudinal vortex street). Accumulation of these vortices in the ionospheric medium can create the strongly turbulent state.     

Stability and shape analysis of relative equilibrium for three-spacecraft electromagnetic formation

The invariant shapes for close formation flying with inter-craft electromagnetic force ensure several potential space applications. However, the 6-DOF relative equilibrium problem has not been systematically investigated. This paper mainly analyzes the invariant shapes of relative equilibrium for the three-spacecraft electromagnetic formation, and studies the families of invariant shape solutions with real and constant magnetic moments as well as their linear stability. The problem is examined based on the full nonlinear coupled dynamic models for collinear and general triangular configurations. The relative equilibrium conditions are analyzed to determine whether an invariant shape do exist, and the corresponding families of invariant shape solutions are identified for static and spinning configurations respectively. Finally, the linear stability of such invariant shapes is numerically discussed, which have shown that most invariant shapes are unstable and controllable.