先进战斗机保障性AGA-SSI评估模型

科学、有效地进行保障性评估是提高装备综合保障能力和加快装备形成战斗力的研究重点之一。文章采用基于加速遗传算法的Shepard相似插值方法,构建了先进战斗机保障性AGA-SSI评估模型并对两型飞机保障性进行了评估,结果表明,模型是可行的、有效的。     

VS-CMA盲均衡算法在短波数据通信中的应用研究

在美军标MIL-STD-188-110B基础上,改进短波（HF）数据通信发送端数据流结构,以便接收端对信号进行盲均衡处理。基于8PSK调制信号的峰度为恒定值的统计特性,提出采用均衡输出信号的峰度与理想信号的峰度差异,以调整恒模算法（CMA）的步长因子;并针对国际电联推荐的短波信道参数,进行了算法的性能仿真。仿真分析表明该算法对慢衰落的短波信道具有较好的均衡效果,对快衰落信道的均衡能力有限;应对快速衰落信道,算法还有待进一步改进。     

无人机航迹规划技术研究及发展趋势

通过对无人机航迹规划的研究,构建了无人机航迹规划的结构框架;分析了无人机系统约束及威胁场约束,探讨了无人机航迹几何建模方法及规划算法的国内外研究概况;并着重分析了规划算法。最后,阐述了无人机航迹规划面临的关键问题及发展趋势。     

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.     

Galactic Wind: Mass Fractionation and Cosmic Ray Acceleration

The dynamical and chemical effects of the Galactic Wind are discussed. This wind is primarily driven by the pressure gradient of the Cosmic Rays. Assuming the latter to be accelerated in the Supernova Remnants of the disk which at the same time produce the Hot Interstellar Medium, it is argued that the gas removed by the wind is enriched in the nucleosynthesis products of Supernova explosions. Therefore the moderate mass loss through this wind should still be able to remove a substantial amount of metals, opening the way for stars to produce more metals than observed in the disk, by e.g. assuming a Salpeter-type stellar initial mass function beyond a few Solar masses. The wind also allows a global, physically appealing interpretation of Cosmic Ray propagation and escape from the Galaxy. In addition the spiral structure of the disk induces periodic pressure waves in the expanding wind that become a sawtooth shock wave train at large distances which can re-accelerate “knee” particles coming from the disk sources. This new Galactic Cosmic Ray component can reach energies of a few×10¹⁸ eV and may contribute to the juncture between the particles of Galactic and extragalactic origin in the observed overall Cosmic Ray spectrum.     

基于知识库的路径规划辅助系统研究

为降低飞机驾驶员在路径规划任务中的工作负荷,提出了基于知识库的路径规划辅助系统结构。采用基于网格的启发式A*搜索技术完成路径规划任务。利用知识库中的规则进行推理,调节启发函数的加权因子,提高求解最优性,并调节规划网格大小,获得最佳求解速度和精度。知识库中的知识规则根据具体条件的累积和计算,在训练及使用中不断得以补充,减少不确定因素对驾驶员的影响。通过系统仿真验证,表明了该方案和算法的有效性。     

基于遗传算法的某型涡扇发动机数字PID控制器设计

在基于DSP平台的某型航空涡扇发动机综合电子调节器的数字化研究中,提出了一种改进遗传算法,并将其应用于数字PID控制器的参数整定过程中.仿真结果表明,该改进遗传算法相比于基本遗传算法及常规PID参数整定方法,控制器动态性能更为优越,可调整性更强.     

基于Nash-Pareto策略的两种改进算法及其应用

针对多目标、多设计变量的优化问题,提出了两种优化的新算法:一种是将多目标问题转化为单目标时,对目标权重的确定提出了新的途径;另一种是直接对多目标问题进行优化,并对Pareto遗传优化技术作了改进,以得到均匀分布的Pareto最优解集.两种新算法都是建立在Nash的系统分解与Pareto遗传算法的基础上,因此称这类算法为Nash-Pareto策略.借助于这类算法,文中以跨声速压气机双圆弧类叶型的气动优化为例,给出了气动优化的全过程.数值优化的实验表明所给出的改进算法是可行的、有效的.     

巡航导弹组合导航中综合地形匹配算法研究

为了克服惯导误差随时间累积的不足,提高巡航导弹的目标命中精度,提出了基于惯导/地形匹配组合导航的巡航导弹中制导方案.其中,地形轮廓匹配技术采用MSD算法和COR算法相结合的综合地形匹配算法,通过粗配和精配两步完成地形匹配过程.组合导航仿真结果表明,采用综合地形匹配算法的地形匹配辅助导航方法可以明显提高惯导精度,因而基于惯导/地形匹配组合导航的巡航导弹中制导方案是可行的.     

基于禁忌搜索算法的机场场面联合优化模型

针对当今机场场面优化对象仅为某一独立环节的情况,梳理联合优化框架,利用已有的单一环节优化模型,建立了滑行路径规划与停机位分配联合优化模型,并设计了禁忌搜索算法流程,最终降低了航班进离场资源占用时间。将优化模型分别植入空域管理与评估系统（ ACES）的空侧容量评估系统中进行仿真分析,结果表明,联合优化模型能够在综合考虑机场运行实际的条件下大幅提升空侧容量,改善机场运行效率与资源配置情况。