交叉航路飞行间隔安全评估研究

在交叉航路上初步研究了碰撞风险模型,从冲突区域模型、概率论模型、Event模型、Reich及其改进模型等5种碰撞风险模型的角度,分析了各个模型的使用范围及建模思想,并在此基础上分析了飞行间隔安全评估未来的研究方向：基于CNS性能的飞行间隔安全评估,防撞系统如何减少碰撞风险以及人为因素对碰撞风险的影响,为今后的研究奠定了基础。     

基于回归型支持向量机的空战目标威胁评估

空战目标威胁评估是协同多目标攻击中的关键问题.针对传统空战目标威胁评估方法在确定权重系数方面的不足,提出了一种新的基于回归型支持向量机的评估方法.在分析了现有的空战目标威胁评估方法中距离威胁模型存在缺陷的基础上,提出了改进的距离威胁模型.建立了基于回归型支持向量机的空战目标威胁评估模型,利用该模型对想定的空战目标进行了威胁评估.仿真结果表明,该方法具有很好的预测能力,可以快速、准确地完成空战目标威胁评估.     

机载气象雷达发展趋势分析

作为危险气象感知的重要手段,机载气象雷达在航空安全保障中发挥着重要作用。本文通过分析机载气象雷达的发展历程和国内外产品及技术,展望了机载气象雷达的发展趋势,并对其关键技术与难点进行了梳理,分析结果可以促进国内相关技术的研究和发展。     

技术成熟度评价方法及其在交会对接任务中的应用

介绍了技术成熟度等级和评价的概念,简述了技术成熟度评价在国外航天工程中的应用情况,提出了航天工程技术成熟度评价标准,包括开展技术成熟度评价的目的、技术成熟度的详细定义及其内涵,并以技术成熟度等级五级为例,给出了具有可操作性的评价细则以及实施要点,通过交会对接任务中运载火箭评价应用实例对技术成熟度评价的应用进行了说明。     

高风险场所安全防范系统不确定性分析与评估

安全防范系统运行的有效性是保证被防护对象的关键。然而,安全防范系统本身及其运行环境存在多种不确定性因素,这些不确定性的存在将导致场所内存在很大的风险性,如果分析处理不当会产生严重的后果。在给出物理系统不确定性模型的基础上,分析了安全防范系统中存在的不确定性因素,提出了层次分析和灰色理论相结合的方法,评估不确定风险因素的权重,实现对入侵报警系统不确定性的评估。     

TIA前机载软件成熟度评估的相关研究

率先引入rFAA（美国联邦航空局）提出的软件成熟度的概念。局方正式签发TIA（型号检查核准书）前,在软件的构型和符合性均未达到最终冻结状态的情况下,通过对软件的成熟度进行有效评估,可以为验证试飞前软件的工程批准提供有力的支持与保障,在一定程度上降低局方飞行试验的风险,保障适航验证试飞活动的顺利开展。由于机载软件成熟度足一个新兴的概念,目前局方（FAA、CAAC）对于如何进行成熟度评估尚未形成正式的、通用的政策性指导文件,国内主机厂对此问题也没有相关的处理经验和具体的操作方法。基于机载软件本身的特点,参考局方在机载软件审查时的主要关注点,提出了TIA前机载软件成熟度评估的基本考虑要素与分析重点。     

On the effect of considering more realistic particle shape and mass parameters in MMOD risk assessments

One of the primary mission risks tracked in the development of all spacecraft is that due to micro-meteoroids and orbital debris (MMOD). Both types of particles, especially those larger than 0.1 mm in diameter, contain sufficient kinetic energy due to their combined mass and velocities to cause serious damage to crew members and spacecraft. The process used to assess MMOD risk consists of three elements: environment, damage prediction, and damage tolerance. Orbital debris risk assessments for the Orion vehicle, as well as the Shuttle, Space Station and other satellites use ballistic limit equations (BLEs) that have been developed using high speed impact test data and results from numerical simulations that have used spherical projectiles. However, spheres are not expected to be a common shape for orbital debris; rather, orbital debris fragments might be better represented by other regular or irregular solids. In this paper we examine the general construction of NASA’s current orbital debris (OD) model, explore the potential variations in orbital debris mass and shape that are possible when using particle characteristic length to define particle size (instead of assuming spherical particles), and, considering specifically the Orion vehicle, perform an orbital debris risk sensitivity study taking into account variations in particle mass and shape as noted above. While the results of the work performed for this study are preliminary, they do show that continuing to use aluminum spheres in spacecraft risk assessments could result in an over-design of its MMOD protection systems. In such a case, the spacecraft could be heavier than needed, could cost more than needed, and could cost more to put into orbit than needed. The results obtained in this study also show the need to incorporate effects of mass and shape in mission risk assessment prior to first flight of any spacecraft as well as the need to continue to develop/refine BLEs so that they more accurately reflect the shape and material density variations inherent to the actual debris environment.     

基于并行蚁群优化的多UCAV任务分配仿真平台

多无人作战飞机(UCAV)协同作战是UCAV参与战斗的主要模式,而多UCAV任务分配是多UCAV协同作战研究的关键问题。针对现有多UCAV任务分配方法中所存在的计算量大、运行时间长等问题,提出了一种基于并行蚁群优化(ACO)的多UCAV任务分配方法。在构建多UCAV空战优势矩阵的基础上,给出了综合态势评估函数;随后阐述了基本ACO算法的基本原理和数学模型,提出了一种用并行ACO算法解决多UCAV任务分配问题的实现方法;最后基于MATLAB图形用户界面(GUI)开发了一种基于并行蚁群优化的多UCAV任务分配仿真平台。实践证明该仿真平台具有良好、开放的可扩展性,且使用方便。     

系统可靠性增长评估模型研究

根据系统在研制期间故障强度变化规律,考虑故障间隔时间影响的情况下,提出了广义可靠性增长评估模型,分析了其参数特性,并给出了拟合优度检验方法;然后,给出了定时截尾和定数截尾情况下,模型参数的极大似然估计公式,采用Simpson方法将积分函数化为求和函数,使得参数估计计算方便,给出了趋势检验方法给出了可靠性增长评估公式;最后,结合发动机故障数据进行了的实例分析,结果表明,模型对试验数据拟合较好,评估结果符合工程实际,模型具有实际应用价值.      

Using high-energy proton fluence to improve risk prediction for consequences of solar particle events

The potential for exposure to large solar particle events (SPEs) with high energy levels is a major concern during interplanetary transfer and extra-vehicular activities (EVAs) on the lunar and Mars surface. Previously, we have used data from the last 5 solar cycles to estimate percentiles of dose to a typical blood-forming organ (BFO) for a hypothetical astronaut in a nominally shielded spacecraft during a 120-d lunar mission. As part of this process, we made use of complete energy spectra for 34 large historical SPEs to calculate what the BFO mGy-Eq dose would have been in the above lunar scenario for each SPE. From these calculated doses, we then developed a prediction model for BFO dose based solely on an assumed value of integrated fluence above 30 MeV (Φ₃₀) for an otherwise unspecified future SPE. In this study, we reasoned that since BFO dose is determined more by protons with higher energies than by those with lower energies, more accurate BFO dose prediction models could be developed using integrated fluence above 60 (Φ₆₀) and above 100 MeV (Φ₁₀₀) as predictors instead of Φ₃₀. However to calculate the unconditional probability of a BFO dose exceeding a pre-specified limit (“BFO dose risk”), one must also take into account the distribution of the predictor (Φ_30,Φ₆₀, or Φ₁₀₀), as estimated from historical SPEs. But Φ₆₀ and Φ₁₀₀ have more variability, and less available historical information on which to estimate their distributions over many SPE occurrences, than does Φ₃₀. Therefore, when estimating BFO dose risk there is a tradeoff between increased BFO dose prediction at a given energy threshold and decreased accuracy of models for describing the distribution of that threshold over future SPEs as the threshold increases. Even when taking the second of these two factors into account, we still arrived at the conclusion that overall prediction improves as the energy level threshold increases from 30 to 60 to 100 MeV. These results can be applied to the development of approaches to improve radiation protection of astronauts and the optimization of mission planning for future space missions.