基于时间最短的SGKW共面打击轨道优化设计

天基对地打击动能武器(SGKW)用于从太空对地面高价值战略目标进行快速、准确的打击。针对最短打击时间要求,研究了SGKW共面打击轨道的优化设计方法。首先建立了SGKW的无量纲化平面运动模型,然后利用庞特里亚金极大值原理将时间最短共面打击轨道的最优控制问题转化为两点边值问题。由于约束条件中存在优化参数,一种基于"遗传算法 序列二次规划"的组合优化算法被用于求解未知参数。仿真结果验证了上述方法的有效性。     

一种基于HMM的多用户检测算法

针对以概率统计为基础信道估计收敛速度慢、状态估计存在非合理性的问题进行研究,提出了一种新的多用户检测方法.该算法以隐马尔可夫模型为基础,为了避免由于相邻状态序列后向概率相差很大而造成的信道估计发散,采用固定延迟的方法,利用锯齿延时的办法计算后向序列概率以减少计算复杂度.根据前后序列之间的相关性和最陡下降法,提出了解相关最小均方(DLMS)多用户上行复合信道的盲估计. 考虑到由于发射序列状态之间可能存在时序非继承性,而搜索与前向序列对应的具有最大转移概率的后续序列,给出了最大后验(MAP)多用户检测方法.计算机仿真实验表明,该算法提高了信道响应估计速度,具有全局收敛性和系统的稳定性.      

一种确定燃气涡轮轴发动机起动最小所需扭矩的工程方法

依据某型涡轴发动机冷运转试验数据,给出了发动机阻力矩和净力矩的计算方法。按照发动机在此温度条件下的最大允许起动时间,提出了确定发动机在该大气温度条件下起动时最小所需扭矩的方法,并通过试验表明用这种方法得到的计算结果和试验结果较吻合。      

返回舱弹道重建与黑障区弹道再现研究

对于飞船返回舱，黑障区弹道再现是再人飞行试验气动分析工作的重要环节。利用舱上测量数据和有限的雷达测量数据重构飞行弹道，是黑障区弹道再现的有效方法。本文建立了返回舱弹道重建的数学模型，包括运动学模型、观测模型、测量误差模型，从而将返回舱弹道重建问题转化为一个非线性动态系统的参数辨识问题。给出了基于极大似然判据和Newton-Raphson迭代的弹道重建算法。对某飞船返回舱的飞行试验数据进行了计算和分析，结果证实了弹道重建数学模型的正确性和算法的可行性。通过弹道重建，不仅再现了黑障区的弹道，而且提供了可靠的、完整的弹道数据。     

具有通信约束的分布式SOR多智能体轨迹估计算法

针对传统多智能体轨迹估计算法信息交换量大，计算量随群规模指数增长，可扩展性差等诸多不足，提出了一种基于超松弛迭代（SOR）的分布式多智能体轨迹估计算法，通过将最大似然（ML）准则下的轨迹估计转化为两级线性优化问题，并综合利用分布式超松弛迭代（Distributed SOR）和标记初始化方法，加快求解速度并简化信息交换流程，最终实现了多智能体位姿轨迹优化和协作定位。实验表明，所提的分布式方法能达到集中式算法的精度水平，在49个智能体规模条件下，位置估计误差小于0.15 m，姿态估计误差小于0.03°，且数据交换量仅到现有主流分布式方法DDF-SAM的0.06%，能很好用于大规模集群的场景。     

H6飞机最大起飞质量数学模型的研究

正确确定最大起飞质量，对于轰炸机和大型运输机的起飞安全有着非常重要的意义。确定最大起飞质量，以往多采用作图的方法，由于影响最大起飞质量的因素比较复杂，所以比较准确的数学模型未曾建立。近几年来对这个问题进行了多方面的探讨，得出一个计算Ｈ６最大起飞质量比较准确的数学模型。此数学模型的建立为其它轰炸机、运输机最大起飞质量的计算开辟了一条新路，对工程应用具有一定的参考价值。     

Primary mass discrimination of high energy cosmic rays using PNN and k-NN methods

Probabilistic neural network (PNN) and k-Nearest Neighbors (k-NN) methods are widely used data classification techniques. In this paper, these two methods have been used to classify the Extensive Air Shower (EAS) data sets which were simulated using the CORSIKA code for three primary cosmic rays. The primaries are proton, oxygen and iron nuclei at energies of 100?TeV–10?PeV. This study is performed in the following of the investigations into the primary cosmic ray mass sensitive observables. We propose a new approach for measuring the mass sensitive observables of EAS in order to improve the primary mass separation. In this work, the EAS observables measurement has performed locally instead of total measurements. Also the relationships between the included number of observables in the classification methods and the prediction accuracy have been investigated. We have shown that the local measurements and inclusion of more mass sensitive observables in the classification processes can improve the classifying quality and also we have shown that muons and electrons energy density can be considered as primary mass sensitive observables in primary mass classification. Also it must be noted that this study is performed for Tehran observation level without considering the details of any certain EAS detection array.     

Drag and energy accommodation coefficients during sunspot maximum

Conditions appropriate to gas-surface interactions on satellite surfaces in orbit have not been successfully duplicated in the laboratory. However, measurements by pressure gauges and mass spectrometers in orbit have revealed enough of the basic physical chemistry that realistic theoretical models of the gas-surface interaction can now be used to calculate physical drag coefficients. The dependence of these drag coefficients on conditions in space can be inferred by comparing the physical drag coefficient of a satellite with a drag coefficient fitted to its observed orbital decay. This study takes advantage of recent data on spheres and attitude stabilized satellites to compare physical drag coefficients with the histories of the orbital decay of several satellites during the recent sunspot maximum. The orbital decay was obtained by fitting, in a least squares sense, the semi-major axis decay inferred from the historical two-line elements acquired by the US Space Surveillance Network. All the principal orbital perturbations were included, namely geopotential harmonics up to the 16th degree and order, third body attraction of the Moon and the Sun, direct solar radiation pressure (with eclipses), and aerodynamic drag, using the Jacchia-Bowman 2006 (JB2006) model to describe the atmospheric density. After adjusting for density model bias, a comparison of the fitted drag coefficient with the physical drag coefficient has yielded values for the energy accommodation coefficient as well as for the physical drag coefficient as a function of altitude during solar maximum conditions. The results are consistent with the altitude and solar cycle variation of atomic oxygen, which is known to be adsorbed on satellite surfaces, affecting both the energy accommodation and angular distribution of the reemitted molecules.     

Investigation on Mechanism of Altitude Characteristic for Air-breathing Pulsed Laser Thruster

Altitude characteristic is of great importance for studying when an air-breathing pulsed laser thruster works in the dense atmosphere condition of 0-30 km altitude. The experimental findings all over the world show that the similar relationship between impulse coupling coefficient and altitude. According to strong explosion theory and an ideal gas model, a dimensionless factor indicating energy law of similitude is introduced, and formula of impulse coupling coefficient is deducted. Then theoretical study of altitude characteristic is carried out and mechanism of altitude characteristic is further explained. The results indicate that there is a maximum value of impulse coupling coefficient if the dimensionless factor equals to 0. 41 in theory, and whether the phenomena of maximum appear or not depends on the range of the dimensionless factor related to altitude. As to a conical nozzle with the fixed length of 120 mm, the relationship between the sonic velocity and the dimensionless factor causes the maximum phenomenon at the altitude of about 12. 5 km, and maximum theoretical impulse coupling coefficient is also found in the experimental investigations. The mechanism of altitude characteristic for air-breathing pulsed laser thruster is discovered in this article, which will provide reference for further research on altitude characteristic.     

民航运输机最大起飞重量和起飞速度的确定

重点论述了限制最大起飞重量的因素和起飞速度的选择方法,并以Citation Jet 1(CJ-1)飞机为例,分析了飞机在昆明/巫家坝机场起飞时限制最大起飞重量的主要因素,给出了CJ-1飞机确定最大起飞重量和起飞速度的分析方法和起飞性能分析表,为部分支线客机和公务机进行起飞分析并确定起飞分析表的内容、结构和形式提供了参考。