飞行高度对固体火箭两相喷焰流动与辐射的影响

固体火箭发动机喷焰的辐射特性对火箭目标探测与跟踪识别具有重要工程意义。本文针对某模型固体火箭发动机,基于欧拉离散相模型描述气-固两相相互作用,采用详细化学反应机理计算喷焰复燃效应,基于逐线积分法+米散射理论求解气体及粒子辐射物性参数,通过视在光线法计算辐射传输,并利用测量数据验证了本文模型的适用性,仿真分析了不同飞行高度对气固两相喷焰流动及辐射特性的影响。研究结果表明：随着飞行高度增加,喷焰中燃气与固体颗粒间相互作用减弱,且粒径越大的粒子与燃气间差异越大;两相喷焰受不同飞行高度上掺混与复燃效应程度差异的影响,致其温度分布和不同组分浓度分布存在显著差异;各高度下两相喷焰光谱辐射呈现气体选择性发射谱结构,其中高温Al2O3对辐射贡献主要集中在短波,且高度越高,影响越小;不同谱带间辐射特性受不同组分发射带影响而存在差异,且2.7μm和4.3μm两个主要发射带的辐射峰值出现在不同飞行高度。     

介质阻挡体放电对甲烷扩散火焰CH*自发辐射影响实验研究

为分析非平衡等离子体对空气/甲烷扩散火焰的助燃效果,实验以发射中心谱线430nm的激发态自由基CH*表征火焰燃烧状态,采用同轴圆柱构型激励器在高频交流模式下激发等离子体,分析了火焰CH*自发辐射图像、火焰高度、CH*径向分布和燃烧释热速率等火焰特性在不同空气流量和当量比下随放电电压的变化规律。结果表明：等离子体激励在空气流量较低时,会显著增强火焰上游甲烷燃烧,从而降低CH*空间分布高度和火焰高度;空气流量增大后,有利于促进甲烷充分燃烧,增大火焰下游CH*辐射强度和分布范围。在火焰上游区域,等离子体气动效应可有效扩展甲烷径向分布,实现剪切层更宽范围燃烧,其活化效应会明显提高剪切层燃烧强度,并随电压增大作用效果逐渐增强。此外,等离子体激励会使燃烧器喷嘴出口附近火焰释热速率显著增大,该现象在空气-甲烷动量比较大时更容易发生。     

电动力绳系离轨系统电流与拉力混合展开控制

电动力绳系离轨系统是一种典型的空间碎片主动消除技术,本文针对电动力绳离轨系统在初始阶段展开的控制问题,仅通过调节有限的系绳张力与电流,不依赖其他推进器,将导电系绳释放至期望长度并抑制系绳的摆动。首先,采用倾斜偶极子地磁场模型,建立考虑系绳质量的近地轨道二体电动力绳系卫星系统动力学模型;其次,在系绳张力与电流存在约束的条件下,采用反步法结合抗饱和辅助函数解决控制输入受限问题,并引入动态尺度广义逆实现了欠驱动电动力绳系统展开稳定控制问题;然后,应用Lyapunov稳定性定理证明了其闭环系统的稳定性;最后,在MATLAB/SIMULINK平台上进行了仿真验证。结果表明：通过调节系绳张力与电流,可以将系绳释放到指定位置,同时控制输入满足约束条件。     

无线电高度表近地测高异常分析及改进

对于轮式起降无人机而言,起降阶段相对高度的准确性对无人机的飞行安全至关重要。针对高速无人机无线电高度表近地测高出现高度拾升和饱和现象,从无线电高度表测高机理出发,深入分析高度跳变的原因,针对问题现象,在不改变安装高度的前提下,提出一种低高度变增益的方法,降低高度饱和噪声的优化措施,有效提高了无线电高度表近地测高的稳定性。通过吊高试验及地面滑行试验表明,优化措施能合理有效解决高度表近地高度测量异常的问题。     

Robust attitude coordinated control for spacecraft formation with communication delays

In this paper,attitude coordinated tracking control algorithms for multiple spacecraft formation are investigated with consideration of parametric uncertainties,external disturbances,communication delays and actuator saturation.Initially,a sliding mode delay-dependent attitude coordinated controller is proposed under bounded external disturbances.However,neither inertia uncertainty nor actuator constraint has been taken into account.Then,a robust saturated delay dependent attitude coordinated control law is further derived,where uncertainties and external disturbances are handled by Chebyshev neural networks (CNN).In addition,command filter technique is introduced to facilitate the backstepping design procedure,through which actuator saturation problem is solved.Thus the spacecraft in the formation are able to track the reference attitude trajectory even in the presence of time-varying communication delays.Rigorous analysis is presented by using Lyapunov-Krasovskii approach to demonstrate the stability of the closed-loop system under both control algorithms.Finally,the numerical examples are carried out to illustrate the efficiency of the theoretical results.     

非晶态铁镍铬磷硼合金磁致伸缩的研究

本文分别以张力冲击法和应变电阻法对非晶态(Fe_(50)Ni_(50))_(80-z)Cr_xP_(14)B_6合金(x=0,1,2,3,4,6,10)薄带的室温饱和磁致伸缩系数进行了测量;测量结果表明,Cr元素的加入,使样品的λ_(?)有所减少;并对结果进行了讨论。     

基于迭代LMI的航天器的姿态静态输出反馈

研究了挠性航天器的姿态控制器设计问题。结合Lyapunov矩阵成形的不变椭圆,使用多目标综合技术集成干扰抑制,鲁棒稳定和控制输入约束问题。基于迭代的线性矩阵不等式(ILMI)给出了静态输出反馈控制器。仿真结果表明,该方法虽然具有一定的保守性,但可以较好的满足系统的鲁棒性能要求,对工程实现具有一定的参考价值。     

Bright band height assignment with precipitation radar data based on multi-resolution analysis (MRA) of wavelet analysis

A method for reconstruction of cross-section of rainfall situations with precipitation radar data based on wavelet analysis of multi-resolution analysis (MRA) which allows extract a peak of the radar reflectivity is proposed in order to detect bright band height. It is found that the bright band height can be estimated by using the MRA with the basis of Daubechies wavelet family. It is also found that the boundaries in rainfall structure can be clearly extracted with MRA.     

Event-triggered adaptive fuzzy attitude takeover control of spacecraft

The problem of attitude takeover control of spacecraft by using cellular satellites with limited communication, actuator faults and input saturation is investigated. In order to lighten the communication burden of cellular satellites, an event-triggered control strategy is adopted. The filtered attitude information needs to be transmitted only when the defined measurement error reaches the event-triggered threshold in this strategy. Then, to deal with the unknown inertia matrix, actuator faults, external disturbances and the errors caused by event-triggered scheme, fuzzy logic systems is introduced to estimate the uncertainties directly. Combining fuzzy logic control strategy and the event-triggered method, the first event-triggered adaptive fuzzy control law is developed. Then, torque saturation of cellular satellites is further considered in the second control law, where the upper bound of the uncertainties is estimated by fuzzy logic systems. The resulting closed-loop systems under the two control laws are guaranteed to be bounded. Finally, the effectiveness of two proposed control laws is verified by the numerical simulations.     

An update global model of hmF2 from values estimated from ionosonde and COSMIC/FORMOSAT-3 radio occultation

In this paper, we present our recent work on developing an updated global model of the ionospheric F2 peak height hmF2 parameter by combining data from the Constellation Observing System for Meteorology, Ionosphere and Climate (COSMIC/FORMOSAT-3) radio occultation (RO) measurements and from the extended global ionosonde stations. In particular, 10 Chinese ionosonde stations’ data are newly introduced into this study. The modeling technique used is based on a two-layer empirical orthogonal function (EOF) expansion. Global distributions of hmF2 maps calculated using the newly constructed global model and the one provided by the International Reference Ionosphere model (IRI-ITU-R) are compared with the global distributions of hmF2 obtained by the COSMIC RO measurements and quantitative statistical analysis of the differences between the model results and those of the COSMIC RO measurements is made for the low (2008) and high (2012) solar activity years. The obtained average root-mean-square differences (RMSEs) for our model are 27.7 km (11.1%) and 31.0 km (9.8%), respectively for the years 2008 and 2012, whereas those for the IRI-ITU-R model are 39.9 km (16.9%) and 35.0 km (11.6%), respectively. Comparison of the results calculated both by our model and the IRI-ITU-R model with the digisonde observation is also made. The comparisons show that the newly constructed global hmF2 model can reproduce reasonably well the observations and perform better than IRI-ITU-R model.