排序方式: 共有39条查询结果,搜索用时 15 毫秒
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月球探测器软着陆机构展开过程的运动学分析 总被引:1,自引:0,他引:1
软着陆机构是月球探测器实现软着陆的关键部件。针对一种四腿式软着陆机构方案,论述了该软着陆机构展开的工作原理,分析了机构的奇异性,推导了机构不发生奇异的条件,建立了展开机构的运动学方程组,采用Newton-Raphson法求解了该非线性运动学方程组,获得了主支撑杆运动参数的变化规律。 相似文献
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为分析编队卫星不同模型间的差异,分别根据动力学和运动学推导了星间相对运动的非线性、线性和相对轨道根数三种模型。以非线性相对运动模型为参考,在相同初始条件下比较各模型的位置误差。仿真结果表明:中心星在圆轨道或近圆轨道上运动时,三个模型结果相差较大。增大中心星轨道偏心率,可减小其位置误差。 相似文献
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Nonlinear dynamics of a flapping rotary wing: Modeling and optimal wing kinematic analysis 总被引:2,自引:4,他引:2
The analysis of the passive rotation feature of a micro Flapping Rotary Wing(FRW)applicable for Micro Air Vehicle(MAV) design is presented in this paper. The dynamics of the wing and its influence on aerodynamic performance of FRW is studied at low Reynolds number(~10~3).The FRW is modeled as a simplified system of three rigid bodies: a rotary base with two flapping wings. The multibody dynamic theory is employed to derive the motion equations for FRW. A quasi-steady aerodynamic model is utilized for the calculation of the aerodynamic forces and moments. The dynamic motion process and the effects of the kinematics of wings on the dynamic rotational equilibrium of FWR and the aerodynamic performances are studied. The results show that the passive rotation motion of the wings is a continuous dynamic process which converges into an equilibrium rotary velocity due to the interaction between aerodynamic thrust, drag force and wing inertia. This causes a unique dynamic time-lag phenomena of lift generation for FRW, unlike the normal flapping wing flight vehicle driven by its own motor to actively rotate its wings. The analysis also shows that in order to acquire a high positive lift generation with high power efficiency and small dynamic time-lag, a relative high mid-up stroke angle within 7–15° and low mid-down stroke angle within -40° to -35° are necessary. The results provide a quantified guidance for design option of FRW together with the optimal kinematics of motion according to flight performance requirement. 相似文献
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首先对一般运动学方法在进行近赤道卫星编队相对运动分析和轨道设计时存在的问题进行了分析 ;其次介绍了一种基于零倾角轨道变换的运动学新方法 ,用其对近赤道卫星编队中参考卫星轨道倾角对环绕卫星轨道根数的影响进行了研究 ;最后对零倾角卫星编队相对运动方程的线性化误差进行了理论分析 ,并利用数值仿真对两种运动学方法的相对运动方程线性化误差进行了比较分析。数值仿真的结果表明 :由基于零倾角轨道变换运动学方法得到的相对运动方程的线性化误差不随参考卫星轨道倾角改变 ,而由一般运动学得到的相对运动方程的线性化误差随着卫星编队接近赤道而呈非线性增大。 相似文献
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