基于非相干积累的微小伪距偏差RAIM方法研究

针对传统RAIM算法难以检测连续微小伪距偏差的问题,提出一种基于非相干积累的微小伪距偏差RAIM方法。该方法通过对多个历元时刻奇偶矢量的非相干积累,使得检测统计量的非中心参数增大,从而提高算法对于微小伪距偏差的故障检测概率。理论分析和仿真结果表明,该方法在历元累加数为10时,可以显著提高对微小伪距偏差的检测性能,其可检测最小伪距偏差值约为传统奇偶矢量法的1/3。同时,该方法无需判断伪距偏差符号,在伪距偏差快速变化条件下,也能有效检测出微小伪距偏差。     

高温空气传输特性对边界层稳定性及转捩预测的影响

为了研究黏度和导热系数对边界层内基本流和流动稳定性的影响，首先通过分析比较Sutherland公式和目前常用的Gupta等人的拟合关系式，建立了高温气体下黏度和导热系数的计算模型，并分别将Sutherland公式和新建立的计算模型应用于7组元化学平衡流的平板模型，在马赫数为10，16和20，飞行高度为30-5km等条件下分别对黏度和导热系数的模型进行比较.计算结果表明:在高温范围内，黏度和导热系数均影响着边界层的基本流、流动稳定性及转捩预测，且两者影响的趋势相反，黏度的增加、导热系数的减小都能使扰动的增长率变大，增长区变宽，转捩位置提前.      

PR方程推算氮气/灭火剂蒸气等熵指数

氮气(N2)/灭火剂蒸气组成的混合气体的容积等熵指数和温度等熵指数随充填压力和温度的变化关系是影响机载灭火系统灭火剂释放过程的重要因素。基于PR(Peng Robinson)方程和范德瓦尔混合规则,编制了N2/灭火剂混合气体的容积等熵指数和温度等熵指数的计算程序,计算了三组混合气体N2/HFC227ea、N2/CF3I和N2/CF3Br充填压力分别为42MPa和25MPa,初始温度为293K时等熵指数随温度的变化曲线。结果表明:它们的容积等熵指数和温度等熵指数随着温度的升高而逐渐下降,呈近似线性关系。在相同温度下,充填压力为42MPa时的三组混合物的容积等熵指数和温度等熵指数均高于充填压力25MPa时的结果。在相同的充填压力和温度下,N2/CF3I的等熵指数最大,其次为N2/HFC227ea和N2/CF3Br的最小。      

Formation flying for magnetic sails around artificial equilibrium points

This paper investigates the problem of magnetic sail-based spacecraft formation control around the artificial equilibrium points (AEPs), which can eliminate the requirement of the propellant. The thrusts are achieved by utilizing the interaction between the solar wind and the artificial magnetosphere generated by superconducting current coil onboard. The circular restricted three-body problem (CRTBP) of magnetic sail is discussed including the allowed regions and linear stability of AEPs, the locations of collinear AEPs and the possibility of existence of periodic orbits around the collinear AEPs. Next, the dynamical models of magnetic sail formation around the collinear AEPs are established. A novel fast fixed-time nonsingular terminal sliding mode controller (FFNTSM) based on fixed-time disturbance observer (FTDO) is developed to account for external disturbances. Several numerical simulations are conducted to substantiate that spacecraft formation can be precisely controlled by the proposed propellantless propulsion method in the presence of external disturbances.     

Boundary of nighttime ozone chemical equilibrium in the mesopause region: Improved criterion of determining the boundary from satellite data

A modified derivation of the criterion of nighttime ozone chemical equilibrium (NOCE) in the mesopause region is presented. According to 3D model calculations, the improved criterion reproduces the lower boundary of the equilibrium much better than its earlier version. Processing of the SABER/TIMED data of 2021 has shown that the modified criterion elevates the NOCE boundary by ～ 0.1–1.7 km, depending on latitude and season. The proposed method of determining the condition of chemical equilibrium can be used to analyse the equilibrium of many trace gases in the stratosphere and troposphere important for different practical applications.     

临近空间地面模拟装置等离子体源仿真研究

为了指导临近空间地面模拟装置中等离子体源结构设计及等离子体环境参数优化，围绕相关指标体系要求，采用数值模拟方法，分析临近空间等离子体环境地面模拟装置中的射流等离子体与下游目标模拟体相互作用。通过研究射流入口处等离子体状态与下游等离子体对钝体包覆效果的依赖关系，明确了影响包覆特性的关键等离子体参数、重要外控参量，及其对下游目标模拟体包覆特性的影响规律。仿真结果表明：相对于其他因素，射流入口的半径、气体流速、速度偏角、气体温度、钝体直径、环境背压等工况对有效实验区长度及厚度参数的影响较大。相关结果对于临近空间等离子体环境地面模拟装置中等离子体源优化设计及等离子体环境参数定向调控具有指导和借鉴意义。