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51.
本文通过对该型教练机现有航空电子系统构型、驾驶员操作程序、接口控制文件深入研究,结合未来功能扩展需求,给出了合理的系统构型分析、功能分配、数据流规划、原相关系统软件改动分析,在此基础上还设计出了嵌入式训练系统技术方案.依据方案研制的嵌入式训练系统原理样机通过系统动态试验、航电系统地面综合试验和飞机地面通电试验,证明系统... 相似文献
52.
An algorithm of analyzing the design parameters for a thin-walled wing from composite material based on the efficient distribution
of structural material between load-carrying elements is described. We consider the problems of convergence acceleration for
the iteration design analysis. Also presented are the examples of determining the design parameters for a superlight aircraft
wing and the rational parameters of the filler in the form of a three-dimensional rod structure. 相似文献
53.
We considered the influence of temperature on the nitric oxide emission under combustion of the near-stoichiometric mixtures
with and without water feed. We revealed the advantage of the method of fuel-water-air mixture combustion over that of the
leaned mixture combustion. 相似文献
54.
在航空发动机机匣安装边装配过程中,不同位置螺栓之间会产生弹性交互作用,不同加载方案会使装配后的螺栓预紧力存在一定的分散度。针对这一问题,建立了3层带止口机匣安装边3维接触有限元模型,研究不同加载方案下螺栓预紧力的施加方法。基于有限元模型数值模拟了3层机匣安装边分别在顺序加载方案、交叉加载方案和正反顺序2轮加载方案下螺栓预紧力的分散度。搭建了相应的试验装置,分别对3种加载方案的预紧力分散度进行试验验证。结果表明:采用正反顺序2轮加载后的螺栓预紧力分散度最小,在3层止口机匣安装边上采用正反顺序2轮加载方案后的螺栓预紧力分散度较小,在有限元仿真中螺栓预紧力分散度为2.43%,在试验中螺栓预紧力分散度为4.98%。采用此方案加载后,止口机匣安装边能达到更好的密封效果和较好的刚度对称性。 相似文献
55.
考虑陀螺效应的转子动力学相似准则 总被引:1,自引:2,他引:1
针对考虑陀螺力矩的转子系统缩尺相似模型与原型是否满足动力学相似的问题,采用量纲分析法推导了考虑陀螺力矩的转子-简单支撑系统相似准则,得到了模型与原型各物理量相似比.通过求解不同相似比下Jeffcott转子系统临界转速的解析解,和利用有限元软件ANSYS对某转子系统临界转速和振型相似性进行了数值模拟,验证了所推导的考虑陀螺力矩转子系统相似准则的正确性.研究表明:考虑陀螺力矩、简单支撑和Rayleigh比例阻尼的转子系统,在相似转速下缩尺模型与原型的固有频率具有相似性,并且临界转速相似. 相似文献
56.
M.D. Ngobeni M.S. Potgieter 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
Observations of galactic cosmic rays (GCRs) from the two Voyager spacecraft inside the heliosheath indicate significant differences between them, suggesting that in addition to a possible global asymmetry in the north–south dimensions (meridional plane) of the heliosphere, it is also possible that different modulation (turbulence) conditions could exist between the two hemispheres of the heliosphere. We focus on illustrating the effects on GCR Carbon of asymmetrical modulation conditions combined with a heliosheath thickness that has a significant dependence on heliolatitude. To reflect different modulation conditions between the two heliospheric hemispheres in our numerical model, the enhancement of both polar and radial perpendicular diffusion off the ecliptic plane is assumed to differ from heliographic pole to pole. The computed radial GCR intensities at polar angles of 55° (approximating the Voyager 1 direction) and 125° (approximating the Voyager 2 direction) are compared at different energies and for both particle drift cycles. This is done in the context of illustrating how different values of the enhancement of both polar and radial perpendicular diffusion between the two hemispheres contribute to causing differences in radial intensities during solar minimum and moderate maximum conditions. We find that in the A > 0 cycle these differences between 55° and 125° change both quantitatively and qualitatively for the assumed asymmetrical modulation condition as reflected by polar diffusion, while in the A < 0 cycle, minute quantitative differences are obtained. However, when both polar and radial perpendicular diffusion have significant latitude dependences, major differences in radial intensities between the two polar angles are obtained in both polarity cycles. Furthermore, significant differences in radial intensity gradients obtained in the heliosheath at lower energies may suggest that the solar wind turbulence at and beyond the solar wind termination shock must have a larger latitudinal dependence. 相似文献
57.
针对气动发动机的工作过程,利用能量方程、气体状态方程、连续性方程及运动过程方程建立气动发动机的非线性微分方程组.选取合适的基准量,对所建立的微分方程组进行无因次化,得到无因次化的数学模型.利用MATLAB/Simulink仿真工具,对无因次数学模型进行研究,得到各无因次量对气动发动机输出扭矩的影响.从仿真结果可以看出,气动发动机的无因次转速、进气门面积比例因子、排气门面积比例因子以及进气持续角度对气动发动机的无因次输出扭矩影响较大.当发动机转速升高扭矩急剧下降时,可以通过调整进气门面积比例因子、排气门面积比例因子以及进气持续角度使输出扭矩恒定. 相似文献
58.
59.
S.I. Oronsaye L.A. McKinnell J.B. Habarulema 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
A new version of global empirical model for the ionospheric propagation factor, M(3000)F2 prediction is presented. Artificial neural network (ANN) technique was employed by considering the relevant geophysical input parameters which are known to influence the M(3000)F2 parameter. This new version is an update to the previous neural network based M(3000)F2 global model developed by Oyeyemi et al. (2007), and aims to address the inadequacy of the International Reference Ionosphere (IRI) M(3000)F2 model (the International Radio Consultative Committee (CCIR) M(3000)F2 model). The M(3000)F2 has been found to be relatively inaccurate in representing the diurnal structure of the low latitude region and the equatorial ionosphere. In particular, the existing hmF2 IRI model is unable to reproduce the sharp post-sunset drop in M(3000)F2 values, which correspond to a sharp post-sunset peak in the peak height of the F2 layer, hmF2. Data from 80 ionospheric stations globally, including a good number of stations in the low latitude region were considered for this work. M(3000)F2 hourly values from 1987 to 2008, spanning all periods of low and high solar activity were used for model development and verification process. The ability of the new model to predict the M(3000)F2 parameter especially in the low latitude and equatorial regions, which is known to be problematic for the existing IRI model is demonstrated. 相似文献
60.