基于能量管理的横向机动弹道优化设计

为实现小射程能量的有效利用,增强导弹的突防能力和禁飞区规避能力,提出了一种基于能量管理的横向机动弹道设计与优化方法.该方法通过初始离面角使弹道一级偏离传统射面,后面级再修正射面以命中目标.在建立能量管理方程、初始离面角及横向转弯角的解析计算模型的基础上,迭代解析计算机动角的初值;采用遗传算法对机动角及弹道程序进行优化,得到了最优解.仿真结果表明,该方法在满足导弹能量管理的条件下实现了导弹的横向机动,可有效提高弹道导弹的突防能力,优化算法简单可行,收敛效果好.     

基于Netlogo的终端区进场交通流建模与仿真

终端区进场交通流特性参数研究对于解决复杂空域结构下航空器拥堵、航班延误具有重要的实际意义。基于元胞传输模型将进场航线划分元胞,并且在数理推导的基础上,基于Netlogo仿真建模平台搭建进场交通流元胞传输模型仿真环境,对进场交通流的宏观涌现行为进行仿真模拟,得到交通流基本参数速度、流量、密度之间演变趋势。研究结果表明,终端区进场交通流三大基本参数之间存在明显的数量关系,关系曲线相对应分为自由流、拥挤流和阻塞流三种状态,并且受到管制间隔、飞行程序、管制策略的影响。利用相关研究成果,可通过改变管制策略、调整管制间隔、优化飞行程序的方法使得交通流特性向着可预知的方向演变,因此对终端区交通态势的判断具有应用价值。     

基于PDM的TC取证信息管理系统开发

为改变发动机型号合格取证信息化管理水平落后的现状,加快适航取证工作进程,在对航空发动机型号取证工作进行深入研究的基础上,以PDM(产品数据管理)系统为平台,使用Java语言和Eclipse工具,对Teamcenter进行定制和二次开发,设计开发了发动机型号合格取证信息管理系统。通过系统可以对发动机型号合格取证工作总体进度进行监控,并且实现了对取证文档、审定流程和取证人员及其权限控制的一体化管理。提高了航空发动机型号取证工作效率,推动了发动机适航取证工作的信息化进程。     

航空发动机PC取证信息管理系统模型研究

针对航空发动机制造企业生产许可取证组织混乱、业务繁杂、信息庞大复杂且联系弱、取证流程不清晰等问题,在深入研究生产许可(PC)取证工作和适航法规的基础上,以航空发动机生产许可审定为对象,结合丰田企业精益生产管理理念,并参照基于产品全生命周期管理PLM、企业资源管理ERP、生产管控等系统,实现了生产许可审定组织模型、业务模型、流程模型和系统模型的集成构建,研究和开发了具有实用价值的航空发动机生产许可审定信息管理系统模型,极大方便了企业构建适航取证系统,加快适航取证步伐,提高工作效率.     

Modelling of galactic Carbon in an asymmetrical heliosphere: Effects of asymmetrical modulation conditions

Observations of galactic cosmic rays (GCRs) from the two Voyager spacecraft inside the heliosheath indicate significant differences between them, suggesting that in addition to a possible global asymmetry in the north–south dimensions (meridional plane) of the heliosphere, it is also possible that different modulation (turbulence) conditions could exist between the two hemispheres of the heliosphere. We focus on illustrating the effects on GCR Carbon of asymmetrical modulation conditions combined with a heliosheath thickness that has a significant dependence on heliolatitude. To reflect different modulation conditions between the two heliospheric hemispheres in our numerical model, the enhancement of both polar and radial perpendicular diffusion off the ecliptic plane is assumed to differ from heliographic pole to pole. The computed radial GCR intensities at polar angles of 55° (approximating the Voyager 1 direction) and 125° (approximating the Voyager 2 direction) are compared at different energies and for both particle drift cycles. This is done in the context of illustrating how different values of the enhancement of both polar and radial perpendicular diffusion between the two hemispheres contribute to causing differences in radial intensities during solar minimum and moderate maximum conditions. We find that in the A > 0 cycle these differences between 55° and 125° change both quantitatively and qualitatively for the assumed asymmetrical modulation condition as reflected by polar diffusion, while in the A < 0 cycle, minute quantitative differences are obtained. However, when both polar and radial perpendicular diffusion have significant latitude dependences, major differences in radial intensities between the two polar angles are obtained in both polarity cycles. Furthermore, significant differences in radial intensity gradients obtained in the heliosheath at lower energies may suggest that the solar wind turbulence at and beyond the solar wind termination shock must have a larger latitudinal dependence.     

“嫦娥二号”卫星L2点角动量管理

对“嫦娥二号”(CE-2)卫星进入环绕日地拉格朗日L2点的李萨如轨道后卫星喷气卸载所产生的影响进行了研究.提出了一种利用光压力矩辅助卫星太阳电池翼角度调整进行角动量管理的方法.在轨试验表明,太阳光压强度足够对飞行在L2点环绕轨道上的CE-2卫星进行角动量管理,可以大幅度减少动量轮在轨喷气卸载的次数,有利于CE-2卫星的轨道维持.     

Comparison of ionosphere characteristic parameters obtained by ionosonde with IRI-2007 model over Southeast Asia

In this work, the foF2 and hmF2 parameters at the conjugate points near the magnetic equator of Southeast Asia are studied and compared with the International Reference Ionosphere (IRI) model. Three ionosondes are installed nearly along the magnetic meridian of 100°E; one at the magnetic equator, namely Chumphon (10.72°N, 99.37°E, dip angle 3.0°N), and the other two at the magnetic conjugate points, namely Chiang Mai (18.76°N, 98.93°E, dip angle 12.7°N) and Kototabang (0.2°S, 100.30°E, dip angle 10.1°S). The monthly hourly medians of the foF2 and hmF2 parameters are calculated and compared with the predictions obtained from the IRI-2007 model from January 2004 to February 2007. Our results show that: the variations of foF2 and hmF2 predicted by the IRI-2007 model generally show the similar feature to the observed data. Both parameters generally show better agreement with the IRI predictions during daytime than during nighttime. For foF2, most of the results show that the IRI model overestimates the observed foF2 at the magnetic equator (Chumphon), underestimates at the northern crest (Chiang Mai) and is close to the measured ones at the southern crest of the EIA (Kototabang). For hmF2, the predicted hmF2 values are close to the hmF2(M3000F2_OBS) during daytime. During nighttime, the IRI model gives the underestimation at the magnetic equator and the overestimation at both EIA crests. The results are important for the future improvements of the IRI model for foF2 and hmF2 over Southeast Asia region.     

基于AFDX网络的飞行管理仿真系统

系统建模与数字仿真是大型客机飞行管理系统研发的重要阶段.初步建立了基于航空电子全双工交换式以太网(AFDX,Avionics Full-Duplex Switched Ethernet)的飞行管理系统分布式实时仿真系统模型.对飞行计划、飞行导引、轨迹预测、性能计算、综合导航、导航数据库、综合显示等核心功能进行了分析建模和算法开发.并在此基础上对飞行管理计算机、综合导航系统、自动飞行系统等仿真子系统进行了设计,在满足实时性要求的前提下,基于AFDX网络与分布式仿真结构实现了对以飞行管理计算机系统为核心的航空电子仿真系统的集成,给出了一种通用的、基于AFDX网络的飞行管理系统分布式仿真框架.仿真系统的运行结果证明:基于AFDX网络的分布式仿真结构能够有效满足实时性要求,提高网络通信性能.      

满足多约束的主动段能量管理制导方法

高超音速飞行器运载任务需要满足多项约束条件,针对耗尽关机型固体运载火箭需要在主动段进行能量管理.基于控制推力和速度之间夹角来实现主动段能量管理的思路,综合交变姿态控制能量管理(AEM,Alternate Attitude Control Energy Management)和一般能量管理(GEM,General Energy Management),提出了样条能量管理(SEM,Spline Energy Management)制导方法,并针对分离前定轴飞行约束条件进行了修正.以三级运载火箭为例,通过AEM,GEM和SEM对比,验证了样条能量管理制导方法的可行性.     

“天巡一号”微小卫星星务故障管理设计

对“天巡一号”微小卫星的总体情况进行了简单介绍,并针对星务管理系统的功能给出了设计方案.从硬件和软件上提出了基于局部冷冗余备份的多项故障预防及故障处理设计,并设计了电源安全管理及软件容错等多项可靠性措施,提高了星务管理系统的可靠性及安全性,符合“天巡一号”微小卫星星务系统采用单一中央数据处理系统,集成星务管理及姿态控制能力的设计方案.