基于特征模型的全系数自适应控制系统稳定性研究

讨论了基于特征模型的黄金分割加逻辑微分自适应控制律组成闭环系统的稳定性问题。针对参数未知、线性定常或慢时变的二阶不稳定对象,本文给出了在采样周期满足一定条件下,上述闭环系统渐近稳定的充分条件,其中包含对于时变参数变化范围和非线性阻尼系数的约束条件。     

What Determines the Composition of SEPs in Gradual Events?

Gradual solar energetic particle (SEP) events are evidently accelerated by coronal/interplanetary shocks driven by coronal mass ejections. This talk addresses the different factors which determine the composition of the accelerated ions. The first factor is the set of available seed populations including the solar wind core and suprathermal tail, remnant impulsive events from preceding solar flares, and remnant gradual events. The second factor is the fractionation of the seed ions by the injection process, that is, what fraction of the ions are extracted by the shock to participate in diffusive shock acceleration. Injection is a controversial topic since it depends on the detailed electromagnetic structure of the shock transition and the transport of ions in these structured fields, both of which are not well understood or determined theoretically. The third factor is fractionation during the acceleration process, due to the dependence of ion transport in the turbulent electromagnetic fields adjacent to the shock on the mass/charge ratio. Of crucial importance in the last two factors is the magnetic obliquity of the shock. The form of the proton-excited hydromagnetic wave spectrum is also important. Finally, more subtle effects on ion composition arise from the superposition of ion contributions over the time history of the shock along the observer’s magnetic flux tube, and the sequence of flux tubes sampled by the observer.     

Galactic Wind: Mass Fractionation and Cosmic Ray Acceleration

The dynamical and chemical effects of the Galactic Wind are discussed. This wind is primarily driven by the pressure gradient of the Cosmic Rays. Assuming the latter to be accelerated in the Supernova Remnants of the disk which at the same time produce the Hot Interstellar Medium, it is argued that the gas removed by the wind is enriched in the nucleosynthesis products of Supernova explosions. Therefore the moderate mass loss through this wind should still be able to remove a substantial amount of metals, opening the way for stars to produce more metals than observed in the disk, by e.g. assuming a Salpeter-type stellar initial mass function beyond a few Solar masses. The wind also allows a global, physically appealing interpretation of Cosmic Ray propagation and escape from the Galaxy. In addition the spiral structure of the disk induces periodic pressure waves in the expanding wind that become a sawtooth shock wave train at large distances which can re-accelerate “knee” particles coming from the disk sources. This new Galactic Cosmic Ray component can reach energies of a few×10¹⁸ eV and may contribute to the juncture between the particles of Galactic and extragalactic origin in the observed overall Cosmic Ray spectrum.     

离箱扰动和折叠翼展开数学模型研究

根据箱式发射导轨与导弹，导弹与折叠翼的约束特点，应用动力学普遍定理和解除约束原理，创建了离箱扰动运动数学模型和拆卸叠翼展开过程计算数学模型，并将计算结果与飞行试验结果作了比较。     

基于有限元法的隧道荷载模型位移反分析

介绍了一种以荷载模型为求解对象的位移反分析法。它是以通用有限元软件为实验平台，利用隧道位移实测值建立荷载灵敏系数方程，根据最小二乘法原理反求隧道模型的荷载，再将正分析结果和实际值进行对比分析井重新调整隧道荷载模型，最终获得较为符合实际的隧道荷载模型。该方法的优点是既考虑了岩土松动荷载效应又能体现支护结构与周围岩土体的共同作用，且具有较好的操作性。     

掠海飞行导弹击水概率的仿真研究

本文对掠海导弹的击水概率问题进行了研究,提出了用均匀设计、Monte—Carlo法和逐步回归法建立击水概率预报公式的仿真方法,并结合某型号的反舰导弹进行计算,得到了满意的结果。本文还利用表观频率和表观频谱的概念,建立起飞航导弹的背景干扰——海浪和阵风的数学模型,并用波叠加法进行了数字仿真。     

空间实验室大面积太阳电池阵技术研究

介绍了空间实验室大面积太阳电池阵的方案构型，并进行了模态分析、热结构耦合分析和动力学仿真分析。生产出了全尺寸的集成演示样机，进行了展开试验、主展开机构的模态试验，以及半刚性太阳电池板和二自由度驱动机构的振动试验。计算和试验结果表明，技术方案是可行的。     

浅谈消费心理与购买模式的逻辑关系--兼论技术类人员营销素质的培养

本文针对目前市场上对营销人员的需求旺盛情况，主要谈了从非专业人员中培养营销人员的方法。强调了学习创新的重要性。用通俗的引例，解释了复杂的心理学有关术语及认识过程与消费者购买行为的关系。培养营销人员准确把握消费者心理活动的能力，提高营销人员自身的生存能力和企业的竞争能力。     

具有年龄结构的离散流行病模型

离散的流行病模型能够更恰地描述某些流4行病的传播过程，本文针对恢复者不具有免疫力而被再次传染成为易感者的情况，提出了具有年龄结构的离散SIS（易感者Susceptible、染病者Infective、易感者Susceptible）模型，运用线性化方法，比较法及计算机模拟等方法对模型的动力学性态进行了较全面的研究，研究中引入基本再生数，其意义为在染病期内一个典型的染病者在完全易感的人群产生的新患者平均数，基本再生数决定平衡点的稳定性，文中主要得到了无病平衡点的全局稳定性，最后，对所研究的理论结果进行了计算机模拟。