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An improved numerical method that can construct Halo/Lissajous orbits in the vicinity of collinear libration points in a full solar system model is investigated. A full solar system gravitational model in the geocentric rotating coordinate system with a clear presentation of the angular velocity relative to the inertial coordinate system is proposed. An alternative way to determine patch points in the multiple shooting method is provided based on a dynamical analysis with Poincare′sections. By employing the new patch points and sequential quadratic programming, Halo orbits for L_1, L_2, and L_3 points as well as Lissajous orbits for L_1 and L_2 points in the EarthMoon system are generated with the proposed full solar system gravitational model to verify the effectiveness of the proposed method. 相似文献
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Yue Wang Shijie Xu Mengping Zhu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The full dynamics of spacecraft around an asteroid, in which the spacecraft is considered as a rigid body and the gravitational orbit–attitude coupling is taken into account, is of great value and interest in the precise theories of the motion. The spectral stability of the classical relative equilibria of the full spacecraft dynamics around an asteroid is studied with the method of geometric mechanics. The stability conditions are given explicitly based on the characteristic equation of the linear system matrix. It is found that the linearized system decouples into two entirely independent subsystems, which correspond to the motions within and outside the equatorial plane of the asteroid respectively. The system parameters are divided into three groups that describe the traditional stationary orbit stability, the significance of the orbit–attitude coupling and the mass distribution of the spacecraft respectively. The spectral stability of the relative equilibria is investigated numerically with respect to the three groups of system parameters. The relations between the full spacecraft dynamics and the traditional spacecraft dynamics, as well as the effect of the orbit–attitude coupling, are assessed. We find that when the orbit–attitude coupling is strong, the mass distribution of the spacecraft dominates the stability of the relative equilibria; whereas when the orbit–attitude coupling is weak, both the mass distribution and the traditional stationary orbit stability have significant effects on the stability. We also give a criterion to determine whether the orbit–attitude coupling needs to be considered. 相似文献
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To meet the requirements of fast and automatic computation of subsonic and transonic aerodynamics in aircraft conceptual design,a novel finite volume solver for full potential flows on adaptive Cartesian grids is developed in this paper.Cartesian grids with geometric adaptation are firstly generated automatically with boundary cells processed by cell-cutting and cell-merging algo rithms.The nonlinear full potential equation is discretized by a finite volume scheme on these Cartesian grids and iteratively solved in an implicit fashion with a generalized minimum residual (GMRES) algorithm.During computation,solution-based mesh adaptation is also applied so as to capture flow features more accurately.An improved ghost-cell method is proposed to implement the non-penetration wall boundary condition where the velocity-potential of a ghost cell is modified by an analytic method instead.According to the characteristics of the Cartesian grids,the Kutta condition is applied by specially computing the gradients on Kutta-faces without directly assigning the potential jump to cells adjacent wake faces,which can significantly improve the solution con verging speed.The feasibility and accuracy of the proposed method are validated by several typical cases of sub/transonic flows around an ONERA M6 wing,a DLR-F4 wing-body,and an unconventional figuration of a blended wing body (BWB).The validation cases demonstrate a fast convergence with fully automatic grid treatment and computation,and the results suggest its capacity in application for aircraft conceptual design. 相似文献
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获取舰载直升机实用风限图,仅依靠实装飞行试验或建模仿真都是非常困难的。通过起降飞行模拟试验获取理论风限图,结合少量的海上实装飞行验证试验是一种综合较优的方法。起降飞行模拟试验需要真实飞行员和高等级飞行模拟器参与,飞行模拟器中的母舰气流场数据、母舰运动可由建模仿真或试验测试得到,且必须考虑母舰气流场的非定场特性;只有当飞行员视景或视觉反馈受限时(如能见度降低时),飞行模拟器基座的六自由度运动才是必需的;用DIPES或Bedford方法量化飞行员主观操纵负担,结合记录的客观操纵数据,评判起降难度;典型的飞行模拟试验程序包含了不同风况下的进近和甲板着舰,通常每隔15°和5kn一个风况。通过起降飞行模拟试验得到的理论风限图,可以更加有效和安全地指导海上实装飞行验证试验,最终获得实用风限图。 相似文献
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为了获得全流量补燃循环发动机的富燃预燃室可靠点火、稳定燃烧和均匀的出口燃气,对富燃预燃室头部喷注器排布方案展开了研究。对设计的中心燃烧区和环形燃烧区两种不同头部方案进行了试验,得到了富燃预燃室的压力曲线和预燃室出口的温度分布。试验结果表明:相比中心燃烧区结构方案,环形燃烧区结构方案更容易获得可靠的点火和稳定的燃烧,有更好的燃气均匀度。相比常规的富燃预燃室,全流量补燃循环发动机的富燃预燃室工作温度更低、混合比更小。相比使用液氧的方案,使用气氧的富燃预燃室在启动、关机过程更迅速、平稳。 相似文献
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文章通过讨论n沟道CCD的物理结构以及两种CCD饱和弥散(弥散型饱和状态和表面型饱和状态)的差异,介绍了面阵CCD抗弥散技术,它通过改变垂直转移时序使普通CCD具有抗弥散功能。对采用该技术前后相机抗弥散的实际效果进行了对比,进一步研究了面阵CCD时序抗弥散所必需的表面型饱和高电平偏置电压测定方法、低电平电压偏置测定方法以及时序工作频率标定方法,给出了工程实现的具体途径。总结了时序抗弥散技术的优缺点,列出了该技术的使用范围和限制条件。 相似文献
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