一种新的导航星选取算法研究

在导航星表的建立过程中，由于恒星的数量太多，往往要进行筛选，通常这种选择复杂费时，而结果往往并不是最优的。本文引入了动态星等阈值分布函数，将传统星等阈值过滤算法中的静态阈值用动态星等阈值代替，建立了一种新的动态星等阈值过滤选择模式。而基于统计学习理论的支持向量机方法为求解高维非线性动态星等阈值分布函数提供了新的途径。本文讨论了这种基于支持向量机的导航星自动选择算法——回归选取算法。实验表明，用该算法所选取的导航星表，导航星数量少、分布均匀性好。同时它还能适应多种任务的导航星选取要求，具有很强的通用性。     

高速弹载平台相参积累研究

针对高速弹载平台加速度大相参积累效果变差需进行加速度补偿的问题，研究了信号波长和积累时间与加速度之间的关系，推导了利用多普勒谱宽计算加速度的公式，提出短时间积累使用弹载惯导设备输出加速度值进行补偿、长时间积累使用惯导数据与多普勒谱宽测量加速度相结合的加速度补偿方法。仿真验证了该方法的有效性。     

飞行模拟器动力学控制的研究

针对如何获取运动平台的实时加速度和在精确跟踪加速度的同时限制位移,建立了系统动力学模型以计算加速度,使用虚拟弹簧法限制位移。在Matlab环境下,搭建了整个伺服控制系统。仿真结果表明,控制系统在保证平台位移不脱离限制区域的基础上,实现了加速度的精确跟踪。     

Diffusive shock acceleration at interplanetary perpendicular shock waves: Influence of the large scale structure of turbulence on the maximum particle energy

We calculate the maximum energy that a particle can obtain at perpendicular interplanetary shock waves by the mechanism of diffusive shock acceleration. The influence of the energy range spectral index of the two-dimensional modes of the interplanetary turbulence is explored. We show that changes in this parameter lead to energies that differ in at least one order of magnitude. Therefore, the large scale structure of the turbulence is a key input if the maximum particle energy is calculated.     

基于动态时间阈值的报警聚合方法研究

针对网络入侵检测中持续性攻击引发的多个报警事件时间间隔变化的问题,引入时间间隔变异系数描述报警的时间波动特征;通过将报警数据属性分为时间约束属性和相似度约束属性,提出了一种利用动态时间阈值约束的相似报警数据聚合方法。实验结果表明,这种方法能有效减少持续性攻击触发的冗余报警。     

冲击加速度校准中低通滤波器的应用

介绍了在冲击加速度校准中,为了抑制电、机械等干扰和噪声对冲击加速度测量结果的影响,采用二阶巴特沃斯型低通滤波器,通过时间序列翻转、二次滤波等方式,实现零相移的低通滤波效果。并比较不同截止频率下,低通滤波器对衰减程度不同的冲击加速度波形产生的峰值偏差,给出不同加速度波形下,低通滤波器截止频率选择应注意的问题。     

Thermodynamic features of aircraft diagonal gas turbines

An effect of the Coriolis forces on the process of gas expansion in the turbine stage is considered. Expressions for efficiency with regard for the radial flow passage are derived. The calculation results and statistical data on the geometric parameters of diagonal stages are presented.     

Study of the 28 October 2003 and 20 January 2005 solar flares by means of 2.223 MeV gamma-emission line

By the data on intensity-time profiles of the neutron capture line of 2.223 MeV we have studied some characteristics of two solar flares, 28 October 2003 and 20 January 2005 (INTEGRAL and CORONAS-F observations, respectively). The SINP code was applied making allowance for the main processes of neutron interactions and deceleration in the solar plasma, character of neutron source, losses of neutrons and density model of the solar atmosphere. Comparison of the computed time profiles of 2.223 MeV line with observed ones for the flare of 28 October 2003 confirms the results obtained earlier for three other flares. Namely, the effect of density enhancement (EDE) in the sub-flare region, as well as the variations (hardening) of accelerated particle spectrum in the course of the event have been confirmed. The usual modeling procedure by the SINP code, however, seems to be inapplicable to the event of 20 January 2005. Possible causes of density enhancements during some flares and peculiarities of the 20 January 2005 flare are discussed.     

静电电磁脉冲辐射场诱发针-球电极结构放电试验

针对当前国内外诱发静电放电（ESD）研究较少的实际情况，为了解自然环境下静电放电辐射场诱发放电的基本特性，进一步分析诱发放电的特征规律，建立了大气条件下诱发放电试验系统。主要采取理论分析、试验验证的方式，对静电放电辐射场诱发针-球电极结构放电的基本规律进行摸索，初步得出了诱发放电的基本规律。研究结果表明：在外界条件一定的情况下，随着辐射场强的不断增大，放电重复频率不断增大；在辐射场强一定的情况下，随着高压源电压的不断增大，诱发放电重复频率不断增大；在外界环境条件一定的情况下，能够确定该条件下的诱发放电唯一阈值。这些试验规律的取得，为真空条件下的诱发放电特性研究提供了试验方法和理论依据，对开展航天器运行环境中的诱发放电研究和防护方法设计具有重要意义。     

Optimal steering law of refractive sail

The interaction between electromagnetic waves and matter is the working principle of a photon-propelled spacecraft, which extracts momentum from the solar radiation to obtain a propulsive acceleration. An example is offered by solar sails, which use a thin membrane to reflect the impinging photons. The solar radiation momentum may actually be transferred to matter by means of various optical phenomena, such as absorption, emission, or refraction. This paper deals with the novel concept of a refractive sail, through which the Sun’s light is refracted by crossing a film made of polymeric micro-prisms. The main feature of a refractive sail is to give a large transverse component of thrust even when the sail nominal plane is orthogonal to the Sun-spacecraft line. Starting from the recent literature results, this paper proposes a semi-analytical thrust model that estimates the characteristics of the propulsive acceleration vector as a function of the sail attitude angles. Such a mathematical model is then used to analyze a simplified Earth-Mars and Earth-Venus interplanetary transfer within an optimal framework.