悬臂空心梁式加速度计的设计

分析证明:悬臂梁式加速度计的灵敏度与它的谐振频率的平方成反比。因此,欲展宽频带而保持灵敏度不变就很困难。利用应力集中的方法可以有效地解决这一问题。采用空心梁结构不仅能产生应力集中而且能减少梁的自身质量带来的影响,可以有效地展宽频带。文中给出了几种梁的刚度计算。     

波形环式弹性支座刚度的测试与数值模拟

进行了波形环式弹性支座刚度数值模拟研究,推导了波形环支承刚度与其离散弧段刚度之间的关联式,建立了环弧段刚度分析模型,用有限元分析程序“APOLANS”计算了环弧段的载荷-位移场静力问题。与原有分析方法相比,精度有显着的提高,相当接近测试刚度,起到了理论分析与测试数据相互校验的作用,并为波形环式弹性支座刚度设计提供了可靠的理论依据。      

柔性接头角刚度及弹性件剪切应变的精确计算

角刚度（又称弹性比力矩）及弹性件在最大摆角下的剪切应变是固体发动机柔性接头设计的重要指标。在考虑固体火箭发动机柔性接头层弹性件几何尺寸的差异的基础上,推导了角刚度及弹性件剪切应变的精确计算公式。算例表明,该方法计算精度更高。     

Rigidity spectrum of the 27-day variation of the galactic cosmic ray intensity in different epochs of solar activity

We study the temporal evolution of the power rigidity spectrum of the first (27 days) and the second (14 days) harmonics of the 27-day variation of the galactic cosmic ray intensity measured by neutron monitors in the period of 1965–2002. The rigidity spectrum of these variations can be approximated by a power law. We show the rigidity spectra of the first and the second harmonics of the 27-day variation of the galactic cosmic ray intensity have similar time profiles. These spectra are hard (γ ≈ 0.5 ± 0.1) and soft (γ ≈ 1.1 ± 0.2) during solar maximum and minimum activity, respectively. We ascribe this to the alternation of the sizes of the modulation regions responsible for the 27-day variation of the galactic cosmic ray intensity in different epochs of solar activity. Especially, the average radial sizes of the modulation regions of the 27-day variation and the heliolatitudinal extension of the heliolongitudinal asymmetry are smaller during solar minimum than during solar maximum. We show also, that the temporal changes of the power rigidity spectra of the first and the second harmonics of the 27-day variation of the galactic cosmic ray intensity are in a negative correlation with the changes of the rigidity spectrum of the corresponding 11-year variation.     

制造公差是影响螺旋弹簧刚度和弹力的主要因素

分析了弹簧的几何尺寸制造公差对其刚度和弹力的影响。     

薄壁结构强刚度可靠性分析

本文提出了一种可模拟飞行器翼面等溥壁结构的强刚度可靠性分析方法。给出了在Mises屈服条件下平面应力元件强、刚度安全裕量方程。讨论了强度失效模式和刚度失效模式的相关性。     

转子动力学优化设计

优化设计可以使转子支承系统具有先天优良的转子动力学特性, 优化支承的刚度与阻尼系数是使转子支承系统获得优良动力学特性的有效途径。本文采用传递矩阵-拟模态综合法分析转子支承系统的动力特性-临界转速、不平衡响应以及对支承动力参数灵敏度分析, 进而对支承动力参数作优化设计。本文所提出的方法已经过算例、模型试验及工程应用的证实。      

New index of long-term variations of galactic cosmic ray intensity

We find that the soft rigidity spectrum of the Galactic Cosmic Ray (GCR) intensity variations for the maximum epoch and the hard rigidity spectrum for the minimum epoch calculated based on the neutron monitors experimental data (1960–2002) are related with the various dependence of the diffusion coefficient on the GCR particle’s rigidity for different epoch of solar activity. This dependence is stronger in the maximum epoch than in the minimum epoch of solar activity, and is provided by the essential temporal rearrangements of the structure of the Interplanetary Magnetic Field (IMF) turbulence from the maxima to minima epoch of solar activity. We also show that the rigidity spectrum of GCR intensity variations is harder for the effective rigidities ∼(10–15) GV (by neutron monitors data), than for the effective rigidities ∼(25–30) GV (by neutron monitors and muon telescopes data). A general scenario of GCR modulation versus solar activity is settled on the essential temporal rearrangements of the structure of the IMF turbulence. Therefore, the temporal changes of the power law rigidity spectrum exponent can be considered as a vital (new) index to explain the 11-year variations of the GCR intensity. We assume that ∼(70–80)% of the changes of the amplitudes of the 11-year variations of GCR intensity is related with the changes of the IMF turbulence versus solar activity.     

叠层球面橡胶-金属弹性轴承等刚度设计研究

从理论上推导了叠层球面橡胶-金属弹性轴承各胶层的压缩刚度和扭转刚度计算公式,探讨了胶层压缩刚度、扭转刚度的等刚度设计方法,并将等压缩刚度和等扭转刚度设计方案的理论计算结果、有限元仿真结果分别与未进行等刚度设计方案的结果分别进行了计算和对比,结果表明,等刚度设计可以很大程度上消除不同胶层之间的刚度差异,各胶层压缩刚度和扭转刚度的理论计算结果与仿真结果基本吻合。