渐扩通道内湍流流动与混合的数值模拟

应用标准形式的ｋ－ε湍流模型,对具有逆向压力梯度的渐扩通道内两股等温或不等温射流的湍流流动与混合进行了数值模拟。结果表明,时均速度场与温度场的计算结果与实验测量数据相符合。     

Real-time total system error estimation:Modeling and application in required navigation performance

In required navigation performance（RNP）, total system error（TSE） is estimated to provide a timely warning in the presence of an excessive error. In this paper, by analyzing the underlying formation mechanism, the TSE estimation is modeled as the estimation fusion of a fixed bias and a Gaussian random variable. To address the challenge of high computational load induced by the accurate numerical method, two efficient methods are proposed for real-time application, which are called the circle tangent ellipse method（CTEM） and the line tangent ellipse method（LTEM）,respectively. Compared with the accurate numerical method and the traditional scalar quantity summation method（SQSM）, the computational load and accuracy of these four methods are extensively analyzed. The theoretical and experimental results both show that the computing time of the LTEM is approximately equal to that of the SQSM, while it is only about 1/30 and 1/6 of that of the numerical method and the CTEM. Moreover, the estimation result of the LTEM is parallel with that of the numerical method, but is more accurate than those of the SQSM and the CTEM. It is illustrated that the LTEM is quite appropriate for real-time TSE estimation in RNP application.     

Correlation between sunspots and interplanetary shocks measured by ACE during 1998–2014 and some estimations for the 22nd solar cycle and the years between 2015 and 2018 with artificial neural network using the Cavus 2013 model

The Advanced Composition Explorer (ACE) spacecraft has measured 235 solar-based interplanetary (IP) shock waves between the years of 1998–2014. These were composed of 203 fast forward (FF), 6 slow forward (SF), 21 fast reverse (FR) and 5 slow reverse (SR) type shocks. These data can be obtained from the Interplanetary Shock Database of Harvard-Smithsonian Centre for Astrophysics. The Solar Section of American Association of Variable Star Observers (AAVSO) is an organization that counts the number of the sunspots. The effects of interplanetary shock waves on some physical parameters can be computed using a hydrodynamical model. There should be some correlations between these effects and the sunspot variations. The major objective of this paper is twofold. The first one is to search these correlations with sunspots given in the database of AAVSO. As expected, high correlations between physical parameters and sunspots have been obtained and these are presented in tables below. The second objective is to make an estimation of these parameters for the 22nd solar cycle and the years between 2015 and 2018 using an artificial neural network. Predictions have been made for these years where no shock data is present using artificial intelligence. The correlations were observed to increase further when these prediction results were included.     

谈扩频与信道编码——与郑志彬等三同志商榷

分析了扩频调制与信道编码的本质区别，讨论指出文［２］是扩频体制，而不是如文［１］所说的信道编码。     

USB数传I支路的信道测试

分析遥测解调分系统中 I支路数据传输的特点 ,制定了相应的测试方案。方案弥补了原有测试方法的不足 ,给出了具体的测试结果。实践证明该方法合理可行 ,具有较高的实用价值。     

基于视觉的惯性导航误差在线修正

陀螺零偏和加速度计零偏是影响惯性测量单元(IMU)积分精度的重要因素。提供一组精确的实时的零偏估计可以提高IMU的积分精度,为视觉导航提供良好的位姿预测,提高整个系统的动态性能。通过合理地建立IMU的噪声模型以及IMU和视觉的组合方程,利用一种基于李群和李代数知识的IMU预积分方法将零偏进行合理的线性化,运用Kalman滤波进行IMU零偏的在线估计。实验结果表明,通过本文的修正方法,惯性导航的平均积累误差由0.034m/s提高到0.0037m/s,精度明显提高。     

燃气源开槽导管出口烧蚀特性分析

针对某火箭弹控制系统燃气源在点火试验过程中出现的导管出口烧蚀现象,利用数值计算模拟气流流动参数分布, 考虑到导管管壁的非稳态传热过程, 计算出不同时刻在导管开槽出口附近管壁的温度分布, 得出与试验一致的结论     

燃气源开槽导管三维流场的数值模拟

为了解某火箭弹控制系统燃气源开槽导管内的气流流动特性,通过ＳＩＭＰＬＥ方法对其复杂流场进行了数值模拟。采用隐式时间分裂格式、幂函数方案及交错网格修正压力等方法,获得了燃烧室后部和导管内气流的速度、压力、密度和温度的三维分布,计算结果与实验现象的规律一致     

简论飞机生存力的设计

生存力是指飞机在人为敌对环境中躲避、承受敌方武器威胁的能力。它是衡量飞机作战效能的最重要的指标。本文从生存力的构成、生存力提高的方法、生存力提高的设计原则．以及生存力设计的实施和评估几个方面对飞机生存力设计作了简要的论述。     

自旋稳定卫星姿态参数递推容错LS估计

准确计算自旋稳定卫星姿态参数是正确实施姿态控制的前提。本文基于最小二乘（LS）理论，建立了在线计算卫星姿态参数的一组具有容错功能的递推LS算法，简要论证了该算法具备良好的统计最优性质。