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.     

空间能量粒子探测方法研究

阐述了空间能量粒子探测的原理和方法。介绍了国外在能量粒子探测方面所采用的半导体望远镜测量法、电场加速法、磁偏转法等方法，分析了它们各自的优缺点。就制约能量粒子探测技术发展的关键因素进行了讨论。并以此为基础，结合我国实际情况提出了一种新的探测方法。     

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.     

煤粉粒径分布在气固两相流场中的测试技术研究

针对输送管道内煤粉颗粒的粒径分布宽的特点，用侧向接收散射光的Mie散射方法和Fraunhofer衍射方法作了理论分析和实际测试。利用分子筛和显微镜对被测粒子进行了静态测量，其结果可以作为相对准确的测量标准。研究结果表明，针对细粉分离器内煤粉颗粒的形状、浓度和粒径的分布规律，用衍射测试方法可以达到较高的测试精度，取得较好的测试效果。     

磁粉检验标准环形试块的机理分析

为了分析控制磁粉检验系统综合性能的标准环形试块的机理，首先建立一个计算漏磁场的简化数学模型，然后解标量磁位的=维拉普拉斯方程，求出被磁化的环形试块上圆孔产生的漏磁场，计算环形试块表面的磁粉受力，分析其特点并得出相应的结论。     

压电驱动自耦合射流流动特性实验

为了研究压电驱动狭缝喷口自耦合射流的流动特性,采用PIV、热线风速仪测试手段,对自耦合射流激发器在不同激励因素下的流场和速度场分布进行了实验和分析.结果显示,自耦合射流在狭缝出口处产生了反向涡对,随着自耦合射流的发展,射流呈现出在喷口短轴方向急剧向两侧扩展、而在喷口长轴方向先收缩后缓慢扩展的流动特征;自耦合射流的速度分布在法线方向呈现先上升后下降的趋势,在z/b=10左右速度达到最大值;在射流展向上,短轴方向速度呈规律的对称分布和速度自模的特征,而长轴方向速度近喷口区域呈现马鞍状分布,随着法向距离增加这种趋势消失.研究中发现,激发器存在两个谐振频率,在谐振频率激发下自耦合射流的速度和涡量比较大.与常规射流相比,自耦合射流显示出了独特的流动特性.     

改进的粒子群算法求解背包问题

本文提出了改进的粒子群算法求解背包问题,阐明了该算法求解背包问题的具体实现过程。通过与其他文献中实例的计算结果比较,表明该算法切实可行,有较高的搜索效率。     

协同多目标攻击空战决策的启发式粒子群优化算法

利用协同多目标攻击战术的特定知识，并结合粒子群算法，提出了一种用于空战决策的启发式粒子群算法。该算法利用粒子群算法对解空间探索能力强，容易跳出局部最优陷井及启发式算法局部搜索能力强的优点，快速、高效地对全局最优值进行搜索。该算法通过求解友机导弹对目标的最优分配来确定空战决策方案。仿真实验结果表明。本文算法对最优空战决策方案的搜索性能明显优于普通粒子群算法及其他两种遗传算法。     

一种用于导弹末制导的线性化控制方法

针对包含未知参数的导弹运动非线性模型,提出了一种用于末制导的线性化反馈简化控制方法。在模型中引入附加加速度输出,通过消除内反馈和零极点以输入-输出的近似线性控制导弹的非线性运动。给出了控制模型及其构成。仿真结果表明,该方法的反应速度快、稳定性好,控制精度满足要求,可用于导弹跟踪飞行控制。     

液体火箭发动机初始雾化液滴分布预测

在简要描述使用最大熵原理预测初始雾化液滴分布的基础上,发展了较传统方法具有更大收敛域的数值计算方法,建立了离心式喷嘴雾化特性研究实验台,使用激光相位粒子分析仪进行了雾化粒径分布研究,结果显示实验数据同使用最大熵原理预测的分布吻合性较好,在此基础上最后提出了在液体火箭发动机雾化粒径分布预测应用中的策略。