火箭发动机随机推力调节控制驱动器的研制

为满足某型号液体火箭发动机定混合比随机无极变推力工作要求,研制了基于DSP处理器的随机推力调节控制驱动器。该控制驱动器实时接收随机变推力指令,在定混合比条件下,协调控制发动机系统上的燃料及氧化剂路调节阀,从而控制燃料及氧化剂流量,完成发动机的随机变推力控制。其参加多次发动机系统冷调试验及地面全程热试车,工作稳定可靠,实现了变推力双组元推进剂流量同步控制,精确控制发动机混合比,快速响应随机变推力控制要求。     

嫦娥一号干涉成像光谱仪2C级图像数据质量评价

嫦娥一号干涉成像光谱仪(IIM)获取的多波段图像数据对于月表矿物成分反演具有重要意义. 从目视质量、客观参数、几何配准精度、图像质量随时间的变化情况等方面对IIM 2C级的多波段图像数据质量进行了评价. 结果显示, 其两端波段范围的图像质量较差, 不能有效识别月表单元, 中间波段图像质量较好; 自然色图像显示IIM数据存在明显的横向色调不均一性. 利用图像的客观评价指标(辐射精度、清晰度、信息量)将干涉成像光谱仪图像数据与美国Clementine UV-VIS多光谱图像数据进行对比分析, 结果表明, IIM数据清晰度好于Clementine UV-VIS, 而在方差和信息量上弱于Clementine UV-VIS. 将IIM图像数据与Clementine多光谱数据统一到相同的空间分辨率, 进行配准精度评价, 其最大控制点配准误差为0.63pixel. 此外, 还对时间跨度两个月覆盖月表同一区域的IIM图像数据从辐射精度、信息量和清晰度方面进行了评价.      

燃烧供热热光伏系统实验研究

针对未来深空探测供电需求,设计了一套热光伏发电系统,采用丙烷燃烧器模拟同位素热源,并利用低禁带GaSb电池实现了系统的热电转换。研究了气体流量、过量空气系数、回热器性能、滤波器等对辐射器温度及电池输出功率、系统转换效率的影响。结果表明：电池输出功率随燃气量单调增加,而在一定燃气量下,存在一最优过量空气系数使其达到最大值;同时,回热器和滤波器对辐射器温度和电池输出特性有很大影响;本实验系统可以实现最大输出功率密度0.45W/cm 2,系统转换效率2.8%。     

光滑粒子流体动力学的一种并行数值计算方案

在三维超高速碰撞数值计算方面,针对三维光滑粒子动力学（SPH）方法计算量大和耗时长的缺点,文章提出了一种简单直接、易于编程实现的SPH并行计算方案,并简述了该方案的基本思想、任务划分、变量存储、信息传递以及主要计算步骤。最后利用自编并行程序计算了两个超高速碰撞实例,结果表明:针对几百万个粒子,在运算速度为每秒5万亿次的“银河”计算机上申请23个核并行计算,每步约需要8 s,加速比约为10,并行效率约为50%,计算时间显著减少。     

一种改进的直方图概率多假设多目标跟踪方法

直方图概率多假设跟踪（H-PMHT）方法及其变形泊松分布直方图概率多假设跟踪（P-HPMHT）方法的一个主要缺点是其量测模型仅考虑了背景杂波而没有考虑传感器噪声,从而导致在低信噪比条件下检测概率较低。针对这一问题,提出了一种带传感器噪声模型的H-PMHT方法,通过将传感器噪声引入量测模型,从而明显提高了对低信噪比目标的跟踪检测能力。该方法的计算量与目标数保持线性关系,仍然适用于目标数目较多的情况。仿真实验表明：该方法在误跟踪比率为1‰,信噪比为6 dB时,检测比率可提升近20%,信噪比为3 dB时,可提升近10%。     

带中介轴承的双转子系统振动耦合作用评估

为了评估中介轴承对双转子系统的振动耦合作用,从临界转速位置振型变化、临界转速变化、模态振型与稳态不平衡响应的应变能分布变化、中介轴承受力变化等多角度,阐释双转子耦合振动的表现形式和关联关系,提出了相应的评价指标或评估方法,并以典型燃气涡轮发动机双转子系统为对象,进行了分析评估。结果表明,单转子的模态振型可能在双转子模态振型中表现为3种形式,一一对应出现、重复出现或耦合出现,对应的临界转速及应变能分布也会随之产生相应的变化;中介轴承受力在临界转速位置出现峰值,而应变能分布变化最大的转速位置与系统临界转速位置不一致,同时还受不平衡激励位置影响;各单元应变能占比变化量随转速变化曲线可详细分析特定不平衡激励下系统应变能分布变化情况。所提方法可为双转子-中介轴承系统的设计、故障诊断提供参考。     

基于匹配渐进展开的跳跃式再入解析预测-校正制导律设计

为了适应低升阻比飞行器再入返回的大航程要求,针对大气跳跃再入飞行环境复杂并难以直接获得解析解的特点,基于匹配渐进展开法设计了一种跳跃式再入解析预测-校正制导方法。首先分析了低升阻比飞行器大气跳跃再入轨迹的飞行剖面和制导分段方法;然后分别推导了其运动方程以重力作用为主导的外解和以气动力作用为主导的内解的渐进展开形式,并通过匹配获得了统一的封闭解析表达式;接着基于此解析解实时预测飞行器的剩余航程,并通过不断迭代升阻比垂向分量以满足最后的落点精度;最后针对跳跃再入飞行的不同阶段设计了不同的制导策略以获得最终的倾侧角指令。仿真结果表明采用跳跃式再入返回技术,阿波罗指令舱的航程能够达到8 348 km,而解析预测-校正制导律的落点精度为0.338 km,证明了此方法的有效性。     

O2 evolution and cyclic electron flow around photosystem I in long-term ground batch culture of Euglena gracilis

Based on the purpose of better exploring the function of green producers in the closed aquatic biological life support system, the condition of dynamic O₂ evolution and performance of cyclic electron flow around photosystem I (CEF-PSI) in long-term ground batch culture of Euglena gracilis were studied, the relationship between linear electron flow (LEF) and CEF-PSI was revealed, the function of CEF-PSI was investigated. Excellent consistency in O₂ evolution pattern was observed in cultures grown in both closed and open containers, O₂ evolution was strictly suppressed in phase 1, but the rate of it increased significantly in phase 2. CEF-PSI was proposed to be active during the whole course of cultivation, even in the declining phase 3, it still operated at the extent of 47–55%. It is suggested that the relationship between LEF and CEF-PSI is not only competition but also reciprocity. CEF-PSI was proposed to contribute to the considerable growth in phase 1; it was also suggested to play an important protective role against photosystem II (PSII) photoinhibition at the greatly enhanced level (approximately 80–95%) on the 2nd day. Our results in this research suggest that E. gracilis had very particular photosynthetic characteristics, the strict O₂ evolution suppression in the initial culture phase might be a special light acclimation behavior, and CEF-PSI could be an important mechanism involved in this kind of adaptation to the changeable light environment.     

Orbit determination by genetic algorithm and application to GEO observation

This paper demonstrates an initial orbit determination method that solves the problem by a genetic algorithm using two well-known solutions for the Lambert’s problem: universal variable method and Battin method. This paper also suggests an intuitive error evaluation method in terms of rotational angle and orbit shape by separating orbit elements into two groups. As reference orbit, mean orbit elements (original two-lines elements) and osculating orbit elements considering the J2 effect are adopted and compared. Our proposed orbit determination method has been tested with actual optical observations of a geosynchronous spacecraft. It should be noted that this demonstration of the orbit determination is limited to one test case. This observation was conducted during approximately 70 min on 2013/05/15 UT. Our method was compared with the orbit elements propagated by SGP4 using the TLE of the spacecraft. The result indicates that our proposed method had a slightly better performance on estimating orbit shape than Gauss’s methods and Escobal’s method by 120 km. In addition, the result of the rotational angle is closer to the osculating orbit elements than the mean orbit elements by 0.02°, which supports that the estimated orbit is valid.     

The classical Laplace plane as a stable disposal orbit for geostationary satellites

The classical Laplace plane is a frozen orbit, or equilibrium solution for the averaged dynamics arising from Earth oblateness and lunisolar gravitational perturbations. The pole of the orbital plane of uncontrolled GEO satellites regress around the pole of the Laplace plane at nearly constant inclination and rate. In accordance with Friesen et al. (1993), we show how this stable plane can be used as a robust long-term disposal orbit. The current graveyard regions for end-of-life retirement of GEO payloads, which is several hundred kilometers above GEO depending on the spacecraft characteristics, cannot contain the newly discovered high area-to-mass ratio debris population. Such objects are highly susceptible to the effects of solar radiation pressure exhibiting dramatic variations in eccentricity and inclination over short periods of time. The Laplace plane graveyard, on the contrary, would trap this debris and would not allow these objects to rain down through GEO. Since placing a satellite in this inclined orbit can be expensive, we discuss some alternative disposal schemes that have acceptable cost-to-benefit ratios.