S形加减速的嵌套式前瞻快速算法

前瞻处理功能是现代数控系统的标志性功能之一,前瞻算法设计直接关系到数控机床的加工效率和运动平稳性。针对目前广泛研究的S形加减速前瞻算法复杂、难以满足实时性要求的问题,从工程实现的角度设计了嵌套式自适应前瞻算法。依据S形加减速曲线的对称性建立了速度规划模型,通过对加速度等效曲线逼近提高了模型求解效率,给出了S形速度规划曲线构造和校验两主要运算阶段的解析解。以连续短直线加工为例,给出了完整的嵌套式快速前瞻算法和实例加工验证。实验结果表明,所提出的算法能获得全局最优运动效率,计算量不足传统方法的30%,结果精确,耗时稳定,能满足现代数控系统甚至是高速高精度数控系统对前瞻处理的实时性要求。给出的解析结果对S形加减速模型的求解有通用意义,可适用于连续短直线、二次曲线以及非均匀有理B样条曲线(NURBS)等参数曲线的S形加减速前瞻速度规划。     

稳态加速度模拟试验设备：离心机设计（17）

文章分3篇10章详细介绍了稳态加速度模拟试验设备——离心机的设计。上篇对稳态加速度环境及其效应、试验方法和相关标准作了阐述;中篇（上）系统介绍国内外该类离心机发展的基本历程、概貌及典型离心机结构细节,并对其适当予以小结与点评;中篇（下）对离心机运动学进行基本理论分析,研究总体设计和部件设计问题,提出离心机设计原则及相应计算方法;下篇通过一个国家＂七五＂科技攻关项目的研制报告作为实例,提供读者进行具体设计时参考。文中,作者对多年累积的技术资料与实践心得进行了系统整理与归纳,力求梳理出一条研制稳态加速度模拟用离心机的设计思路与实用程序,使其兼具资料性、技术性与实用性。该文对相关领域的研究者和技术人员将有一定启发与助益,对其他类同设备设计也有某些触类旁通作用,对该专业有兴趣的读者也可作为参考读物。文章主要探讨的对象是中型、大型、特大型航空航天离心机,土工离心机和载人离心机。在第8章中介绍了离心机主要部件的设计。     

稳态加速度模拟试验设备：离心机设计（4）

路和实用的工作程序.该文章对相关领域的研究人员和技术人员会有启发和帮助,同时对其他同类设备的设计也有触类旁通的作用.文章主要探讨的对象是中型、大型、特大型航空航天物体离心机,土工离心机和载人离心机.     

Relativistic solar protons in the ground level event of 23 February 1956: New study

In this study we applied again to the outstanding solar particle event of 23 February 1956, the largest one in the entire history of observations of solar cosmic rays. Due to significant improvement of the analysis/modeling techniques and new understanding of physical processes in the solar atmosphere and interplanetary space, a possibility arises to interpret the old data in the light of modern concept of multiple particle acceleration at/near the Sun. In our new analysis the data of available then neutron monitors and muon telescopes are used. The technique of the analysis includes: (a) calculation of asymptotic cones of ground-based detectors; (b) modeling of cosmic ray detector responses at variable parameters of the flux of solar relativistic protons; (c) determination of primary solar proton parameters outside magnetosphere by comparison of computed responses with observations. Certain evidence was obtained that the flux of relativistic solar protons consisted of two distinct components: prompt and delayed ones. The prompt component with exponential energy spectrum caused a giant impulse-like increase at a number of European cosmic ray stations. The delayed component had a power-law spectrum and was a cause of gradual increase at cosmic ray stations in the North American region. A numerical simulation of the proton acceleration in the vicinity of the magnetic reconnection region brings to the proton spectrum with exponential dependence on energy. This agrees with observational data for the prompt component. It is also shown that the huge increase in ∼5000% on neutron monitors was due to the prompt component only with the exponential proton spectrum. The power-law spectrum of comparable intensity gave considerably smaller effect.     

爆轰法处理有害气体技术的研究

本项研究是根据化学反应爆轰理论，寻求一种有害气体无害化处理技术的新方法－爆轰法。本法采用乙炔与氧气或窑混合气体的爆轰反应机理，理论计算出反应可能达到的高温、高压，经过实验证明，该方法对于象含氯氟烃类热稳定性高，化学性质安定的有害物质，进行无害化处理是可行的，是一种处理效率可达到９９．９％以上的最新方法。     

The Effects of Transverse Magnetic Field and Density Variations on the Particle Energy Spectra in a Reconnecting 3D Current Sheet

Electron and proton acceleration by a super-Dreicer electric field is further investigated in a non-neutral reconnecting current sheet (RCS) with a variable plasma density. The tangential B _z and transverse magnetic field components B _x are assumed to vary with the distances x and z from the X nullpoint linearly and exponentially, respectively; the longitudinal component (a ‘guiding field’) is accepted constant. Particles are found to gain a bulk of their energy in a thin region close to the X nullpoint where the RCS density increases with z exponentially with the index λ and the tangential magnetic field B _x also increases with z exponentially with the index α. For the RCS with a constant density (λ = 0), the variations of the tangential magnetic field lead to particle power-law energy spectra with the spectral indices γ₁ being dependent on the exponent α as: for protons and for electrons in a strong guiding field (β > 10⁻²) and for electrons in a moderate or weak guiding field (β > 10⁻⁴). For the RCS with an exponential density increase in the vicinity of the X nullpoint (λ≥ 0) there is a further increase of the resulting spectral indices γ that depends on the density exponent index λ as for protons and for electrons in weaker guiding fields and as for electrons in stronger guiding fields. These dependencies can explain a wide variety (1.5–10) of particle spectral indices observed in solar flares by the variations of a magnetic field topology and physical conditions in a reconnecting region. This can be used as a diagnostic tool for the investigation of the RCS dynamics from the accelerated particle spectra found from hard X-ray and microwave emission.     

基于Weibull分布的疲劳加速腐蚀因子分析

考虑预腐蚀对飞机结构疲劳寿命的影响,建立了疲劳寿命服从Weibull分布的 加速腐蚀因子确定方法.假设预腐蚀疲劳寿命服从Weibull分布,特征寿命随时间呈指数规 律变化,推导得到了以疲劳寿命为腐蚀量的加速腐蚀因子表达式,以及在工程常用的时间范 围内加速腐蚀因子与腐蚀时间无关的结论;进行了相关参数估计,建立了加速腐蚀 因子的估计方法,得到了加速腐蚀因子估计量的近似分布,对其进行了统计分析.      

基于角加速度的陀螺框架伺服系统干扰观测器

磁悬浮控制力矩陀螺(MSCMG,Magnetically Suspended Control Moment Gyro)是大型航天器姿态控制的关键执行机构,影响MSCMG输出力矩准确度的一个关键因素是其框架伺服系统的控制精度.为提高MSCMG框架伺服系统的抗干扰能力和控制精度,提出了一种基于角加速度的干扰观测器.其设计思想是:卡尔曼滤波器利用角位置估计出角速度并送往状态观测器以获取准确的角加速度,角加速度和电流作为干扰观测器的输入以获得补偿电流,补偿电流加到电流环的输入端以补偿各种干扰.干扰观测器结构简单,抗干扰能力强.实验表明:该方法有效地提高了MSCMG框架伺服系统的角速度精度与稳定度.     

过载约束下的大机动目标协同拦截

研究了非线性拦截几何下具有过载约束的多枚弱机动能力的导弹拦截强机动能力的目标的协同拦截问题。首先，在建立导弹的可达域、导弹的可行域以及目标的逃逸域这3个概念的基础上提出了非线性拦截几何下的基于逃逸域覆盖的协同拦截策略，并提出了基于标准弹道的设计方法。然后，给出了协同拦截制导律的形式，研究了导弹的末制导初始阵位、制导律参数以及导弹对目标机动的覆盖区域这三者间的关系，并设计了数值求解算法来实现对多弹的覆盖区域的分配、协同制导律的设计以及多弹初始拦截阵位的配置。最后，对理论结果进行仿真。结果显示，多枚机动性较小的导弹，通过初始拦截阵位的合理配置和协同拦截制导律的合理设计，可以实现对机动性能较强的目标的协同拦截。     

用微元法建立单刚体动力学的虚加速度原理和虚力原理

本文首先从刚体动力学方程出发,利用变积法推得其虚加速度原理和虚力原理,然后用微元法思想由质点系动力学的虚加速度原理、虚力原理推得刚体动力学的虚加速度原理与虚力原理,并对两种方法本身进行了比较。由于本文的推导方法是从连续介质力学的观点进行的,故这种方法对进一步建立单柔体、多柔体动力学的虚加速度原理和虚力原理具有重要应用价值,进而对现在热点之一的柔性飞行器动力学的研究有潜在的意义。