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.      

基于动态RCS的无人机航迹实时规划

传统的无人机航迹规划主要采用仅考虑无人机与雷达距离的简化雷达威胁模型,未充分考虑无人机雷达散射截面RCS(Radar Cross-Section)随自身姿态角改变而产生的动态变化.据此,提出了无人机周向动态RCS模型,并建立了综合考虑无人机动态RCS与雷达距离的探测概率模型,利用遗传算法进行了基于动态RCS的航迹实时规划,计算结果与传统航迹规划结果进行了对比.仿真结果表明该模型的可行性和有效性,能充分利用无人机自身的优势规避威胁,满足无人机的航迹实时规划的要求.      

基于离散事件方法的AFDX建模与仿真

采用了建模仿真的方法来分析航空电子全双工交换式以太网(AFDX,Avionics Full Duplex switched ethernet)协议.通过对AFDX协议的抽象,基于离散事件的建模方法,以基本的网络元素来抽象化网络中的端系统、交换机等设备,以离散事件来描述网络设备的行为,以此构建了AFDX网络模型,并依据模型实现了仿真.网络演算是一种理论计算AFDX最坏延迟界限的方法,将典型场景下仿真得到的结果与理论计算的结果进行比较,验证了模型.通过不同流量方案下仿真结果的对比,对AFDX进行了传输特性的分析.      

太阳活动与全球气候变化

太阳不断向地球辐射电磁波和粒子, 太阳辐射是地球气候系统最主要的能量来源. 地球气候系统对太阳活动的响应是一个复杂的过程, 包括辐射过程、动力学过程以及微观物理过程等. 根据太阳辐射的卫星观测结果和重建结果, 例举了古气候、温度、大气环流和云量等方面太阳影响气候的观测证据, 论述了太阳影响气候的三种可能机制, 即太阳总辐射变化可以影响地表温度, 并通过海-气耦合改变大气环流; 太阳紫外辐射通过调制平流层的温度和风场影响下面的对流层; 太阳通过行星际磁场调制银河宇宙线, 而银河宇宙线通过电离大气影响云量, 进而改变地球的能量收支.      

不等温空腔的有效发射率计算

采用Monte-Carlo法对不等温空腔的有效发射率进行计算分析,讨论了腔壁的不等温性、材料的光谱发射率和方向发射率对法向有效发射率的影响,为黑体辐射源的设计提供了理论计算依据。     

月球精确软着陆最优标称轨迹在轨制导方法

为实现在月球表面期望的着陆点进行精确软着陆（PPL）,且满足燃耗最优性要求,基于提出的LIDAR目标点在轨自主选定的月球精确软着陆方案,对月球PPL最优标称轨迹在轨快速规划制导方法进行研究。首先针对月球PPL三维球体非线性轨道动力学模型,采用Legendre Gauss Lobatto伪光谱方法将轨迹优化的最优控制问题转化为非线性规划问题（NLP）,再利用SQP优化算法求解月球PPL最优标称轨迹,最后通过遗传算法对优化结果进行验证,并提出应用遗传算法提供SQP在轨规划初值数据库的方案。仿真结果表明了最优标称轨迹在轨规划方法的快速性和有效性。     

对接口匹配的航天器双主动最优交会研究

研究了两航天器协同轨道机动（双主动）完成近距离交会任务的最优控制问题。在考虑航天器姿态变化、对接口位置及路径约束的情况下,构建了完整的6自由度、26状态的双主动最优交会数学模型。利用高斯伪谱法分别将燃料总消耗最少和交会时间最短两种最优问题离散为大型非线性规划问题,而后应用SNOPT软件包进行了求解。在此基础上通过大量数值计算分析总结了不同初始参数对最小燃料消耗和最短交会时间的影响规律,并与主被动交会形式进行了对比。结果表明,当两航天器质量接近时,双主动交会通常可明显减少燃料消耗,或缩短交会时间;而当质量差距较大时,双主动最优交会逐渐退化为主被动最优交会。     

响应面法优化牡蛎复合酶水解工艺研究

采用响应面法优化牡蛎的复合酶水解工艺.结果表明：中性蛋白酶与风味蛋白酶按照2∶1复配,在水解温度40℃,水解时间5.68h,水解pH值7.0条件下,牡蛎蛋白水解度可达到32.24%,水解效果最优.验证试验表明,实际蛋白质的水解度与模型预测值相近,因此采用响应面法优化牡蛎酶解工艺,准确可靠.     

Low-dose carbon ion irradiation effects on DNA damage and oxidative stress in the mouse testis

To investigate the effects of low-dose carbon ion irradiation on reproductive system of mice, the testes of outbred Kunming strain mice were whole-body irradiated with 0, 0.05, 0.1, 0.5 and 1 Gy, respectively. We measured DNA double-strand breaks (DNA DSBs) and oxidative stress parameters including malondialdehyde (MDA) content, superoxide dismutase (SOD) activity, and testis weight and sperm count at 12 h, 21 d and 35 d after irradiation in mouse testis. At 12 h postirradiation, a significant increase in DNA DSB level but no pronounced alterations in MDA content or SOD activity were observed in 0.5 and 1 Gy groups compared with the control group. At 21 d postirradiation, there was a significant reduction in sperm count and distinct enhancements of DSB level and MDA content in 0.5 and 1 Gy groups in comparison with control. At 35 d postirradiation, the levels of DNA DSBs and MDA, and SOD activity returned to the baseline except for the MDA content in 1 Gy (P < 0.05), while extreme falls of sperm count were still observed in 0.5 (P < 0.01) and 1 Gy (P < 0.01) groups. For the 0.05 or 0.1 Gy group, no differences were found in DNA DSB level and MDA content between control and at 12 h, 21 d and 35 d after irradiation, indicating that lower doses of carbon ion irradiation have no significant influence on spermatogenesis processes. In this study, male germ cells irradiated with over 0.5 Gy of carbon ions are difficult to repair completely marked by the sperm count. Furthermore, these data suggest that the deleterious effects may be chronic or delayed in reproductive system after whole-body exposure to acute high-dose carbon ions.     

Geostationary orbit determination using SATRE

A new strategy of precise orbit determination (POD) for GEO (Geostationary Earth Orbit) satellite using SATRE (SAtellite Time and Ranging Equipment) is presented. Two observation modes are proposed and different channels of the same instruments are used to construct different observation modes, one mode receiving time signals from their own station and the other mode receiving time signals from each other for two stations called pairs of combined observations. Using data from such a tracking network in China, the results for both modes are compared. The precise orbit determination for the Sino-1 satellite using the data from 6 June 2005 to 13 June 2005 has been carried out in this work. The RMS (Root-Mean-Square) of observing residuals for 3-day solutions with the former mode is better than 9.1 cm. The RMS of observing residuals for 3-day solutions with the latter mode is better than 4.8 cm, much better than the former mode. Orbital overlapping (3-day orbit solution with 1-day orbit overlap) tests show that the RMS of the orbit difference for the former mode is 0.16 m in the radial direction, 0.53 m in the along-track direction, 0.97 m in the cross-track direction and 1.12 m in the 3-dimension position and the RMS of the orbit difference for the latter mode is 0.36 m in the radial direction, 0.89 m in the along-track direction, 1.18 m in the cross-track direction and 1.52 m in the 3-dimension position, almost the same as the former mode. All the experiments indicate that a meter-level accuracy of orbit determination for geostationary satellite is achievable.