分布式航天器相对位置测量平台设计

分布式航天器间相对位置的实时高精度测量是分布式航天器实现空间队形保持的关键技术之一。为了对相对位置测量方法进行研究、分析和论证,建立了分布式航天器相对位置测量地面实验平台。介绍了分布式航天器相对位置测量和解算的基本原理;论述了仿真平台的组成和功能;基于仿真平台对相对位置测量精度进行了仿真试验,试验结果显示该平台具有良好的性能指标;最后介绍了相对位置解算仿真评估软件的设计方法。     

新型单元的频率选择表面

在传统十字单元基础上,提出一种新型单元的频率选择表面(FSS)。分析传统十字单元FSS和新型单元FSS在大角度入射时的极化稳定性,并研究TM波入射角度变化时,中心频率的漂移及传输系数的变化。结果表明,传统十字单元FSS在45°入射时中心频率的极化稳定性很差,漂移量为406MHz,TM波由0°到45°入射时,中心频率漂移为448MHz;而新型单元FSS具有中心频率的角度稳定性,TM波入射角度由0°变到45°时,中心频率漂移量仅为28MHz,并且在大角度入射时具有中心频率极化稳定性。     

单平台多任务电子载荷的射频与信号处理管理

介绍了侦察、对抗和打击一体化系统在现代战争中的地位与作用,分析了单个平台内多任务使命电子载荷发展的趋势在于射频和信号处理综合管理,并对综合管理面临的挑战、可行性和实现途径等进行了研究,在此基础上得出几点启示。     

冷却速度对TG6钛合金均温区组织性能的影响

通过焊接热模拟试验研究冷却速度对TG6钛合金焊接热模拟均温区组织性能的影响。结果表明:在空冷状态下均温区达到最佳的性能,随着冷却速度的增大,均温区的抗拉强度稍有提高,拉伸延伸率及断面收缩率没有明显变化;冲击韧性空冷达到最大值,水冷稍有下降;显微硬度随冷却速度增大而增加。     

抑制恒压变量柱塞泵压力低频振荡方法的研究

为解决恒压变量柱塞泵出口压力出现低频振动的问题,阐述了恒压变量机构的原理,从理论上分析了影响出口压力的因素,并指出产生振荡的原因,提出在泵装配过程中,采用工艺关键要点控制的方法可抑制压力低频振荡。试验表明,该方法有效地减小了泵出口压力的低频振荡,使产品装调合格率大大提高。     

基于特征模型的火箭发动机伺服控制系统设计

以新型大推力火箭发动机为研究对象,提出了基于特征模型的伺服系统控制器设计方法。首先,介绍了特征建模理论并讨论了特征模型参数范围;其次,采用人工蜂群算法实时估计火箭发动机伺服系统特征模型参数,使其满足特征模型输出与实际系统输出特性等价条件;最后,使用黄金分割自适应控制律保证系统在参数估计过程中的闭环稳定性,同时引入前馈跟踪控制律,逻辑积分控制律和逻辑微分控制律使伺服控制系统快速、精确跟踪线位移指令并改善动态性能。仿真结果表明,设计的火箭发动机伺服控制系统指令跟踪精度高,动态特性良好,鲁棒性强。     

异构无人系统协同作战关键技术综述

针对异构无人系统的规模、异构性强弱,对异构无人系统进行了分类,引入了异构无人系统协同作战班组的概念以及应用设想,并通过城市环境中异构无人系统协同作战问题为牵引,提出了异构无人系统协同作战面临的挑战与解决思路,在此基础之上,从异构无人系统协同控制架构、协同任务规划、智能交互、目标感知、环境感知等主要方面对异构无人系统协同作战的关键技术进行了分析,最后对异构无人系统协同作战目前的研究进展与挑战进行了总结。     

Comparison of ionospheric F2 peak parameters foF2 and hmF2 with IRI2001 at Hainan

Monthly median values of foF2, hmF2 and M(3000)F2 parameters, with quarter-hourly time interval resolution for the diurnal variation, obtained with DPS4 digisonde at Hainan (19.5°N, 109.1°E; Geomagnetic coordinates: 178.95°E, 8.1°N) are used to investigate the low-latitude ionospheric variations and comparisons with the International Reference Ionosphere (IRI) model predictions. The data used for the present study covers the period from February 2002 to April 2007, which is characterized by a wide range of solar activity, ranging from high solar activity (2002) to low solar activity (2007). The results show that (1) Generally, IRI predictions follow well the diurnal and seasonal variation patterns of the experimental values of foF2, especially in the summer of 2002. However, there are systematic deviation between experimental values and IRI predictions with either CCIR or URSI coefficients. Generally IRI model greatly underestimate the values of foF2 from about noon to sunrise of next day, especially in the afternoon, and slightly overestimate them from sunrise to about noon. It seems that there are bigger deviations between IRI Model predictions and the experimental observations for the moderate solar activity. (2) Generally the IRI-predicted hmF2 values using CCIR M(3000)F2 option shows a poor agreement with the experimental results, but there is a relatively good agreement in summer at low solar activity. The deviation between the IRI-predicted hmF2 using CCIR M(3000)F2 and observed hmF2 is bigger from noon to sunset and around sunrise especially at high solar activity. The occurrence time of hmF2 peak (about 1200 LT) of the IRI model predictions is earlier than that of observations (around 1500 LT). The agreement between the IRI hmF2 obtained with the measured M(3000)F2 and the observed hmF2 is very good except that IRI overestimates slightly hmF2 in the daytime in summer at high solar activity and underestimates it in the nighttime with lower values near sunrise at low solar activity.     

Using the radial basis function neural network to predict ionospheric critical frequency of F2 layer over Wuhan

Neural networks (NNs) have been applied to ionospheric predictions recently. This paper uses radial basis function neural network (RBF-NN) to forecast hourly values of the ionospheric F₂ layer critical frequency(f_oF₂), over Wuhan (30.5N, 114.3E), China. The false nearest neighbor method is used to determine the embedding dimension, and the principal component analysis (PCA) is used to reduce noise and dimension. The whole study is based on a sample of about 26,000 observations of f_oF₂ with 1-h time resolution, derived during the period from January 1981 to December 1983. The performance of RBF-NN is estimated by calculating the normalized root-mean-squared (NRMSE) error, and its results show that short-term predictions of f_oF₂ are improved.     

A high-performance ground-based prototype of horn-type sequential vegetable production facility for life support system in space

Vegetable cultivation plays a crucial role in dietary supplements and psychosocial benefits of the crew during manned space flight. Here we developed a ground-based prototype of horn-type sequential vegetable production facility, named Horn-type Producer (HTP), which was capable of simulating the microgravity effect and the continuous cultivation of leaf–vegetables on root modules. The growth chamber of the facility had a volume of 0.12 m³, characterized by a three-stage space expansion with plant growth. The planting surface of 0.154 m² was comprised of six ring-shaped root modules with a fibrous ion-exchange resin substrate. Root modules were fastened to a central porous tube supplying water, and moved forward with plant growth. The total illuminated crop area of 0.567 m² was provided by a combination of red and white light emitting diodes on the internal surfaces. In tests with a 24-h photoperiod, the productivity of the HTP at 0.3 kW for lettuce achieved 254.3 g eatable biomass per week. Long-term operation of the HTP did not alter vegetable nutrition composition to any great extent. Furthermore, the efficiency of the HTP, based on the Q-criterion, was 7 × 10⁻⁴ g² m⁻³ J⁻¹. These results show that the HTP exhibited high productivity, stable quality, and good efficiency in the process of planting lettuce, indicative of an interesting design for space vegetable production.