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倾转旋翼机的不同舵面存在冗余操纵,而冗余舵面的分配策略和飞行转换路径对其控制重构具有重要的意义。对建立的小型无人倾转旋翼机全量非线性飞行动力学模型在不同飞行模式下的进行配平计算、模型线化后,求出单位操纵面位移所引起的俯仰、滚转和偏航力矩的改变量,即考察倾转旋翼机各操纵面的操纵功效,并对其结果进行详细分析,以确定倾转旋翼机的冗余舵面控制重构能力;确定各飞行模式下倾转旋翼机的操纵方式,给出舵面分配策略的权重系数矩阵;在此基础上,提出三种不同的全模式飞行转换路径方案,并分别计算三种方案下倾转旋翼机的飞行速度与前倾角、姿态角及操纵量的关系。结果表明:三种方案都能实现对飞行器的合理操纵,表明倾转旋翼机的冗余舵面控制重构是可以实现的。 相似文献
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切削过程有限元仿真研究进展 总被引:1,自引:0,他引:1
得益于高性能计算机和软件技术的发展,数值仿真为深入理解切削过程、研究刀具磨损、提高加工表面质量等提供了强大的技术支持。总结了现有几种本构模型的特点,对构建切削仿真有限元模型中的几个关键问题进行了分析和总结,综述了有限元仿真技术在金属切削过程中切屑形成研究、切削温度和切削力、刀具磨损、刀具优化和残余应力预测以及加工表面显微组织演变模拟等方面的研究成果。最后,系统地分析了切削过程有限元仿真研究中存在的问题,探讨了该研究领域未来的发展趋势和需要进一步探索的热点问题。 相似文献
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飞机静力试验中机翼的载荷分配研究 总被引:1,自引:0,他引:1
针对飞机静力试验加载的问题,为使得试验加载力反映飞机受力特性,由载荷分配前输入的典型剖面上剪力、弯矩、扭矩推导出相邻剖面之间的剪力、弯矩、扭矩,通过构造带内力约束的拉格朗日极值函数求出试验加载力,将载荷分配前输入的内力与试验载荷分配后产生的内力进行对比分析,可以得出:通过构造带内力约束的拉格拉日极值函数法分配得到的试验载荷符合载荷的传递,能够满足飞机静力试验加载的要求,可以用于飞机静力试验的加载。 相似文献
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David G. Sibeck R. Allen H. Aryan D. Bodewits P. Brandt G. Branduardi-Raymont G. Brown J. A. Carter Y. M. Collado-Vega M. R. Collier H. K. Connor T. E. Cravens Y. Ezoe M.-C. Fok M. Galeazzi O. Gutynska M. Holmström S.-Y. Hsieh K. Ishikawa D. Koutroumpa K. D. Kuntz M. Leutenegger Y. Miyoshi F. S. Porter M. E. Purucker A. M. Read J. Raeder I. P. Robertson A. A. Samsonov S. Sembay S. L. Snowden N. E. Thomas R. von Steiger B. M. Walsh S. Wing 《Space Science Reviews》2018,214(4):79
Both heliophysics and planetary physics seek to understand the complex nature of the solar wind’s interaction with solar system obstacles like Earth’s magnetosphere, the ionospheres of Venus and Mars, and comets. Studies with this objective are frequently conducted with the help of single or multipoint in situ electromagnetic field and particle observations, guided by the predictions of both local and global numerical simulations, and placed in context by observations from far and extreme ultraviolet (FUV, EUV), hard X-ray, and energetic neutral atom imagers (ENA). Each proposed interaction mechanism (e.g., steady or transient magnetic reconnection, local or global magnetic reconnection, ion pick-up, or the Kelvin-Helmholtz instability) generates diagnostic plasma density structures. The significance of each mechanism to the overall interaction (as measured in terms of atmospheric/ionospheric loss at comets, Venus, and Mars or global magnetospheric/ionospheric convection at Earth) remains to be determined but can be evaluated on the basis of how often the density signatures that it generates are observed as a function of solar wind conditions. This paper reviews efforts to image the diagnostic plasma density structures in the soft (low energy, 0.1–2.0 keV) X-rays produced when high charge state solar wind ions exchange electrons with the exospheric neutrals surrounding solar system obstacles.The introduction notes that theory, local, and global simulations predict the characteristics of plasma boundaries such the bow shock and magnetopause (including location, density gradient, and motion) and regions such as the magnetosheath (including density and width) as a function of location, solar wind conditions, and the particular mechanism operating. In situ measurements confirm the existence of time- and spatial-dependent plasma density structures like the bow shock, magnetosheath, and magnetopause/ionopause at Venus, Mars, comets, and the Earth. However, in situ measurements rarely suffice to determine the global extent of these density structures or their global variation as a function of solar wind conditions, except in the form of empirical studies based on observations from many different times and solar wind conditions. Remote sensing observations provide global information about auroral ovals (FUV and hard X-ray), the terrestrial plasmasphere (EUV), and the terrestrial ring current (ENA). ENA instruments with low energy thresholds (\(\sim1~\mbox{keV}\)) have recently been used to obtain important information concerning the magnetosheaths of Venus, Mars, and the Earth. Recent technological developments make these magnetosheaths valuable potential targets for high-cadence wide-field-of-view soft X-ray imagers.Section 2 describes proposed dayside interaction mechanisms, including reconnection, the Kelvin-Helmholtz instability, and other processes in greater detail with an emphasis on the plasma density structures that they generate. It focuses upon the questions that remain as yet unanswered, such as the significance of each proposed interaction mode, which can be determined from its occurrence pattern as a function of location and solar wind conditions. Section 3 outlines the physics underlying the charge exchange generation of soft X-rays. Section 4 lists the background sources (helium focusing cone, planetary, and cosmic) of soft X-rays from which the charge exchange emissions generated by solar wind exchange must be distinguished. With the help of simulations employing state-of-the-art magnetohydrodynamic models for the solar wind-magnetosphere interaction, models for Earth’s exosphere, and knowledge concerning these background emissions, Sect. 5 demonstrates that boundaries and regions such as the bow shock, magnetosheath, magnetopause, and cusps can readily be identified in images of charge exchange emissions. Section 6 reviews observations by (generally narrow) field of view (FOV) astrophysical telescopes that confirm the presence of these emissions at the intensities predicted by the simulations. Section 7 describes the design of a notional wide FOV “lobster-eye” telescope capable of imaging the global interactions and shows how it might be used to extract information concerning the global interaction of the solar wind with solar system obstacles. The conclusion outlines prospects for missions employing such wide FOV imagers. 相似文献
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本文建立了描述复合材料固化应力史的综合模型。在本模型中考虑了化学收缩对残余应力史的贡献,并考虑了以玻璃化转变区为应力释放区的应力松弛过程。整个模型由四部分组成:描述温度场的模型、物理力学参数的模型、描述细观纵向残余应力史的模型、描述层合固化应力史的模型。 相似文献