基于DSPN的航天测控系统任务可靠性仿真建模

提出了基于确定与随机Petri网（deterministic and stochastic Petri nets,DSPN）的航天测控系统（tracking,telemetry and command,TT&C）任务可靠性定量分析方法,旨在对相关航天测控方案进行可靠性预计.通过对TT&C系统任务剖面进行时序弧段划分,考虑实际系统中测控单元阶段依赖、单元故障可修以及各单元参与任务起止时间不同等其他建模方法难以处理的复杂因素,建立了“单元层-系统逻辑层-阶段层”3层相互关联的TT&C系统任务可靠性DSPN模型.通过对模型仿真运行,实现了对给定测控方案下TT&C系统任务可靠性定量化评估.分析表明:仿真结果随着仿真次数增加逐渐收敛,与Markov解析方法求得的精确值对比误差控制在1%以内.      

美国加速任务试车技术在军用航空发动机上的应用

加速任务试车(AMT)是目前国外研究军用航空发动机耐久性的标准试验,是发动机寿命管理的重要方法。本文以美国F404-GE-402发动机、F110-GE-100发动机为例,介绍了AMT技术在发动机设计验证、部件改进、寿命管理、维修计划等方面的具体做法,对有效提高我国发动机型号研制的风险管理与控制能力和实现发动机的高可靠性具有重要的研究与借鉴价值。     

A Comparative Study of the Influence of the Active Young Sun on the Early Atmospheres of Earth, Venus, and Mars

Because the solar radiation and particle environment plays a major role in all atmospheric processes such as ionization, dissociation, heating of the upper atmospheres, and thermal and non-thermal atmospheric loss processes, the long-time evolution of planetary atmospheres and their water inventories can only be understood within the context of the evolving Sun. We compare the effect of solar induced X-ray and EUV (XUV) heating on the upper atmospheres of Earth, Venus and Mars since the time when the Sun arrived at the Zero-Age-Main-Sequence (ZAMS) about 4.6 Gyr ago. We apply a diffusive-gravitational equilibrium and thermal balance model for studying heating of the early thermospheres by photodissociation and ionization processes, due to exothermic chemical reactions and cooling by IR-radiating molecules like CO₂, NO, OH, etc. Our model simulations result in extended thermospheres for early Earth, Venus and Mars. The exospheric temperatures obtained for all the three planets during this time period lead to diffusion-limited hydrodynamic escape of atomic hydrogen and high Jeans’ escape rates for heavier species like H₂, He, C, N, O, etc. The duration of this blow-off phase for atomic hydrogen depends essentially on the mixing ratios of CO₂, N₂ and H₂O in the atmospheres and could last from ∼100 to several hundred million years. Furthermore, we study the efficiency of various non-thermal atmospheric loss processes on Venus and Mars and investigate the possible protecting effect of the early martian magnetosphere against solar wind induced ion pick up erosion. We find that the early martian magnetic field could decrease the ion-related non-thermal escape rates by a great amount. It is possible that non-magnetized early Mars could have lost its whole atmosphere due to the combined effect of its extended upper atmosphere and a dense solar wind plasma flow of the young Sun during about 200 Myr after the Sun arrived at the ZAMS. Depending on the solar wind parameters, our model simulations for early Venus show that ion pick up by strong solar wind from a non-magnetized planet could erode up to an equivalent amount of ∼250 bar of O⁺ ions during the first several hundred million years. This accumulated loss corresponds to an equivalent mass of ∼1 terrestrial ocean (TO (1 TO ∼1.39×10²⁴ g or expressed as partial pressure, about 265 bar, which corresponds to ∼2900 m average depth)). Finally, we discuss and compare our findings with the results of preceding studies.     

The Grain Impact Analyser and Dust Accumulator (GIADA) Experiment for the Rosetta Mission: Design, Performances and First Results

The Grain Impact Analyser and Dust Accumulator (GIADA) onboard the ROSETTA mission to comet 67P/Churyumov–Gerasimenko is devoted to study the cometary dust environment. Thanks to the rendezvous configuration of the mission, GIADA will be plunged in the dust environment of the coma and will be able to explore dust flux evolution and grain dynamic properties with position and time. This will represent a unique opportunity to perform measurements on key parameters that no ground-based observation or fly-by mission is able to obtain and that no tail or coma model elaborated so far has been able to properly simulate. The coma and nucleus properties shall be, then, clarified with consequent improvement of models describing inner and outer coma evolution, but also of models about nucleus emission during different phases of its evolution. GIADA shall be capable to measure mass/size of single particles larger than about 15 μm together with momentum in the range 6.5 × 10⁻¹⁰ ÷ 4.0 × 10⁻⁴ kg m s⁻¹ for velocities up to about 300 m s⁻¹. For micron/submicron particles the cumulative mass shall be detected with sensitivity 10⁻¹⁰ g. These performances are suitable to provide a statistically relevant set of data about dust physical and dynamic properties in the dust environment expected for the target comet 67P/Churyumov–Gerasimenko. Pre-flight measurements and post-launch checkouts demonstrate that GIADA is behaving as expected according to the design specifications. The International GIADA Consortium (I, E, UK, F, D, USA).     

The Genesis Solar Wind Concentrator Target: Mass Fractionation Characterised by Neon Isotopes

The concentrator on Genesis provided samples of increased fluences of solar wind ions for precise determination of the oxygen isotopic composition. The concentration process caused mass fractionation as a function of the radial target position. This fractionation was measured using Ne released by UV laser ablation and compared with modelled Ne data, obtained from ion-trajectory simulations. Measured data show that the concentrator performed as expected and indicate a radially symmetric concentration process. Measured concentration factors are up to ∼30 at the target centre. The total range of isotopic fractionation along the target radius is 3.8%/amu, with monotonically decreasing ²⁰Ne/²²Ne towards the centre, which differs from model predictions. We discuss potential reasons and propose future attempts to overcome these disagreements.     

载人登月人货分运与人货合运模式对比分析

由于载人航天任务所具有的确保航天员安全的特殊属性,载人登月任务模式往往因此必须考虑救生等多种环节和因素,变得十分复杂。针对目前载人登月人货分运及人货合运两种任务模式,通过比较分析表明,从安全性、任务风险、飞船设计约束、发射窗口、测控支持复杂度方面来看,人货合运模式要优于人货分运模式,但是人货合运模式中的重型火箭如果被要求按照载人火箭标准进行设计和考核,其研制周期、经费方面的投入将会增加。     

蓄热式太阳能热光伏-热推进双模系统换热特性数值模拟研究

本文通过三维数值模拟研究蓄热式太阳能热光伏-热推进双模系统的蓄/释热特性和推进性能。在蓄热式太阳能热推进系统工程模型的基础上,通过射线光学的光路分析验证了聚光器设计的合理性,并获得吸热腔壁面能量分布情况,进一步研究了相变蓄热过程的影响因素。基于场协同原理对热光伏再生冷却结构进行了优化设计,使热光伏具有较好的散热特性,提高发电功率;通过整机流动换热仿真,分析了工质流体在推进器内部的换热情况,计算结果表明,蓄热式热推进器具有达到734s比冲和0.9N推力的推进性能,以及能够满足日蚀区微小卫星的供电和推力需求。     

基于地外天体起飞的真空羽流导流技术仿真与试验研究

针对着航天器发动机羽流导流问题,基于工程经验提出了四种典型导流装置型面(包含内凹槽形式和导流锥形式等),利用计算流体动力学/直接模拟蒙特卡罗(CFD/DSMC)耦合方法,对起飞过程中羽流导流带来的气动力和气动热效应进行了数值模拟,并对不同导流装置情况下羽流场激波、航天器表面压强和热流密度分布规律进行了分析,给出了四种导流装置的导流效果评价。最后以导流锥形式开展试验,对仿真算法进行了验证。结果表明：羽流导流并没有导致发动机燃烧不稳定;综合考虑航天器羽流和发动机安全性,大导流锥导流的方案最优;在导流锥附近的激波位置及形态和仿真一致,仿真与试验的变化趋势一致,仿真算法可信,数据规律可以作为工程参考。     

面向军用飞机任务能力的健康评估方法

军用飞机健康评估在工程实际中存在应用困难的问题。以军用飞机为研究对象,开展包括面向任务 的能力分析、基于故障劣化的功能分析以及参数化的健康评估等研究,得到基于任务分析的“飞机-任务功 能-影响参数暠两级映射作为健康评估的对象;综合利用劣化度、严酷度及极大熵改进区间层次分析法等多种 方法,得到飞机健康状态评估结果。结合具体实例及参数分析结果,表明该评估方法可信度高,具有较高的工 程实用价值。     

运输机空投货物建模与任务性能影响因素研究

针对当前运输机空投货物模型可拓展性不强的问题,提出了分离体的建模方法。在无需分析货物与飞机整体质心变化的情况下,分别以货物和飞机为对象进行受力分析,推导了货物与飞机之间的相互作用力,建立了更加贴近实际的运输机单件货物空投和连续空投的动力学模型。最后,通过数值仿真,分析了飞行速度和牵引伞牵引比对空投任务性能的影响。结果表明,飞行速度和牵引比越大,飞机在货物干扰作用下的状态变化量越小。