Study of the ionosphere during a magnetospheric storm using data on the ground and in space

For the magnetospheric storm of May 14–16, 1997 geophysical data of satellites DMSP and IMP-8 are compared with data of radio propagation on the high-latitude HF radio path of Heiss Island – St. Petersburg and data from European ionosondes. Peculiarities of variations of the operational frequencies range MOF–LOF (maximum and lowest observed frequencies) on the path were considered. The range has been determined by the method of oblique ionospheric sounding (OIS). The latter is more informative for observations during a magnetic storm compared to the vertical sounding method. Nevertheless, an analysis of variations of the critical frequency of the ionospheric F2 layer from the chain of European ionosondes was carried out. For interpretation of results, data of magnetospheric parameters, AE-indexes and riometer data were used. The variations of both frequency range on the path and critical frequencies of the F2 layer through the ionosondes chain during the disturbed period had certain regularities of behaviour. These regularities are being explained from the physical point of view. The analysis of the satellite DMSP data has showed that a magnetospheric disturbance causes displacement equatorward of precipitation and some growth of its width and energy.     

航天器飞行控制仿真与平行系统

总结并分析了目前国内外航天器飞行控制仿真与平行技术的发展现状和任务需求,针对中国当前飞控仿真与平行系统的通用化和标准化不足的情况,提出了一种可组装的飞控仿真与平行系统的定义和系统架构,阐述了仿真与验证、决策与支持两个部分的设计方案,并通过嫦娥五号的飞控工作进行了检验,验证了系统的有效性。最后展望了未来航天器飞行控制仿真与平行技术的发展方向。     

嫦娥五号探测器月面铲挖采样前后状态变化分析

为了深入研究月球演化历史以及太空环境对月球土壤的风化影响,需要定量分析月球表面物质与次表层物质的状态差异。研究提出一种依据彩色图像数据分析月壤状态差异的方法,利用嫦娥五号任务采样期间获取的月球表面铲挖前后的图像数据,分析了每次铲挖前后月球表面的图像灰度表现特性等特征,分析结果表明:月球次表层物质的平均反射率小于表面物质,全色谱段中的平均变化率为-24.71%;局部区域的月球表面次表层物质的平均反射特性基本一致,全色谱段中的平均变化率为-0.30%;月球表层颗粒形态与次表层颗粒形态可能不一致;月球表层颗粒与次表层颗粒组成和化学分子结构可能不一致。分析数据表明嫦娥五号采样位置铲挖前后的原态月壤和新鲜月壤存在明显状态差异,研究结果可为我国后续月球采样实施方案的改进提供基础数据。     

刍议军人婚姻保护

经济、社会的发展和多元化,使军人婚姻和家庭稳定面对越来越多的现实挑战,这直接关系和影响到部队日常训练和作战能力.因此,加强和完善必要的法律和措施,切实保护军人在婚姻家庭方面的合法权益对于稳定部队、提升部队作战能力有着重要的现实意义.本文主要从军婚概念的界定、军婚现状及保护军婚的意义、措施方面入手,对这一问题进行分析和探...     

四阶微分方程两点边值问题解的存在唯一性

讨论了非线性四阶常微分方程y（4）=f（x,y,y’,y”,y”’）在混合两点边值条件y’（a）=0,y”（a）＋y”（6）=0,y（b）=0,y”’（b）=0或y’（a）=0,y”＇（a）＋y＇”（b）=0,y（b）=0,y”（6）=0下,解的存在唯一性。其中f在[a,b]×R4上连续且满足Lipschitz条件。并在推广后的Lipschitz条件与Banach压缩映射原理基础上,得到一些新的存在唯一性结果。     

On the possibility of existence of an additional source of anomalous cosmic rays outside the solar system

On the basis of experimental data obtained at exposure of solid-state track detectors in the magnetosphere of the Earth during solar flares and in quiet Sun periods, an estimate of possible contribution of singly charged oxygen ions to the flare particle fluxes is made. A possibility is considered of the appearance in the vicinity of the solar system of singly ionized oxygen ions generated on stars.     

ZrO2陶瓷切向超声辅助磨削表面及亚表面损伤机制

为进一步揭示切向超声辅助磨削过程中硬脆材料的表面及亚表面损伤机理,基于应变率模型对其磨削过程中材料的动态力学性能进行分析,并在此基础上建立了硬脆材料的脆-塑转变临界切削深度模型与微裂纹损伤深度模型。研究发现,脆-塑转变临界切削深度和微裂纹损伤深度均与应变率有关,其中临界切削深度随着应变率的增加而增加,而横向裂纹损伤深度与中位裂纹损伤深度均随应变率的增加而减小。通过ZrO₂陶瓷切向超声辅助磨削试验进行验证。试验结果表明：由于切向超声振动的引入提高了材料应变率,进而提高了材料的动态断裂应力以及动态断裂韧性,从而扩大了ZrO₂陶瓷的塑性域去除范围,降低了加工表面的横向裂纹与中位裂纹损伤深度,使得ZrO₂陶瓷的表面及亚表面质量得到明显改善。试验结果与理论分析相一致,为进一步揭示切向超声辅助磨削过程中硬脆材料的表面及亚表面微观损伤机理提供了理论参考。     

Broad-search algorithms for the spacecraft trajectory design of Callisto–Ganymede–Io triple flyby sequences from 2024 to 2040, Part II: Lambert pathfinding and trajectory solutions

Triple-satellite-aided capture employs gravity-assist flybys of three of the Galilean moons of Jupiter in order to decrease the amount of ΔV$\mathrm{\Delta }V$ required to capture a spacecraft into Jupiter orbit. Similarly, triple flybys can be used within a Jupiter satellite tour to rapidly modify the orbital parameters of a Jovicentric orbit, or to increase the number of science flybys. In order to provide a nearly comprehensive search of the solution space of Callisto–Ganymede–Io triple flybys from 2024 to 2040, a third-order, Chebyshev's method variant of the p-iteration solution to Lambert's problem is paired with a second-order, Newton–Raphson method, time of flight iteration solution to the _V∞$V_{\infty }$-matching problem. The iterative solutions of these problems provide the orbital parameters of the Callisto–Ganymede transfer, the Ganymede flyby, and the Ganymede–Io transfer, but the characteristics of the Callisto and Io flybys are unconstrained, so they are permitted to vary in order to produce an even larger number of trajectory solutions. The vast amount of solution data is searched to find the best triple-satellite-aided capture window between 2024 and 2040.