Autonomous attitude coordinated control for spacecraft formation with input constraint,model uncertainties,and external disturbances

To synchronize the attitude of a spacecraft formation flying system, three novel autonomous control schemes are proposed to deal with the issue in this paper. The first one is an ideal autonomous attitude coordinated controller, which is applied to address the case with certain models and no disturbance. The second one is a robust adaptive attitude coordinated controller, which aims to tackle the case with external disturbances and model uncertainties. The last one is a filtered robust adaptive attitude coordinated controller, which is used to overcome the case with input con- straint, model uncertainties, and external disturbances. The above three controllers do not need any external tracking signal and only require angular velocity and relative orientation between a spacecraft and its neighbors. Besides, the relative information is represented in the body frame of each spacecraft. The controllers are proved to be able to result in asymptotical stability almost everywhere. Numerical simulation results show that the proposed three approaches are effective for attitude coordination in a spacecraft formation flying system.     

航空直喷发动机缸内混合气形成的试验

基于航空活塞式基础样机的结构特点,自主研制了单缸低压直喷全透明光学发动机,并利用高速摄影对缸内混合气形成进行试验研究.分析了不同燃烧室形状、燃油启喷时刻以及发动机转速等条件下低压直喷发动机缸内的混合气形成规律.研究结果表明:新设计的偏心碗型活塞顶面能够有效地引导燃油喷雾形成向燃烧室顶部卷吸的运动,从而使得燃油液滴聚集在双侧火花塞附近;燃油喷射时刻对混合气形成影响很大,当进气门开度较小且活塞与上止点距离较为适中时喷射燃油,混合气形成质量最好;进气运动较强烈时,发动机转速提高会加速燃油液滴的蒸发,但同时活塞顶面对喷雾的引导作用被削弱,混合气形成质量变差;当进气运动变弱时,发动机转速提高会增强活塞顶面对油束的作用,即引导作用变强.      

高速列车模型编组长度和风挡结构对气动阻力的影响

采用风洞试验的方法,分别对高速列车试验模型2～6车编组状态下的各节车厢气动阻力的分布规律,以及2种不同结构外形的风挡对3车编组列车模型各节车厢气动阻力的影响进行了研究。结果表明：当编组长度大于3车,头车、尾车的阻力系数随编组长度的增加变化较小,中间车的阻力系数约为0．1。1节头车＋N节中间车＋1节尾车的全车气动阻力系数,可用3车编组模型试验的头车阻力系数＋0．1×N＋尾车阻力系数之和进行估算。高速列车风洞试验模型分别采用风挡1和风挡2两种风挡,只是使得气动阻力在各节车厢之间形成不同的分配,对由各节车厢相加形成的全车气动阻力的试验结果影响很小。     

Decentralized attitude synchronization tracking control for multiple spacecraft under directed communication topology

This paper studies the attitude synchronization tracking control of spacecraft formation flying with a directed communication topology and presents three different controllers. By introducing a novel error variable associated with rotation matrix, a decentralized attitude synchronization controller, which could obtain almost global asymptotical stability of the closed-loop system, is developed. Then, considering model uncertainties and unknown external disturbances, we propose a robust adaptive attitude synchronization controller by designing adaptive laws to estimate the unknown parameters. After that, the third controller is proposed by extending this method to the case of time-varying communication delays via Lyapunov–Krasovskii analysis. The distinctive feature of this work is to address attitude coordinated control with model uncertainties, unknown disturbances and time-varying delays in a decentralized framework, with a strongly connected directed information flow. It is shown that tracking and synchronization of an arbitrary desired attitude can be achieved when the stability condition is satisfied. Simulation results are provided to demonstrate the effectiveness of the proposed control schemes.     

基于LAS码的星群多目标测控技术研究

针对星群多目标同时测控问题,基于星群轨道根数的时延特性和多普勒频移特性分析可得,星群多目标测控的上行链路遥控与测距信号可实现S CDMA（Synchronous Code Division Multiple Access,同步码分多址）,由于星间距离较小,下行链路遥测与测距信号满足QS CDMA（Quasi synchronous code division multiple access,准同步码分多址）.上行链路遥控和测距信号形式设计为PCM BPSK CDMA（Pulse Code Modulation Binary Phase Shift Keying Code Division Multiple Access,脉冲编码调制二进制相移键控码分多址）,上行链路信号采用Gold序列扩频;下行链路遥测和测距信号形式设计为PCM BPSK CDMA,根据总的时延差,提出下行链路采用基于等长脉冲间隔法构造的LAS（Large Area Synchronous,大区域同步）码扩频.结果表明：比特信噪比Eb/N0为10.5 dB时,遥控误码率为1＆#215;10 6;Eb/N0为9.6 dB时,遥测误码率为1×10^5——与达到相同误码性能的Gold序列相比有1 dB改善,因此,LAS码相比于Gold码能够获得更好的误码性能.     

FeAlCrBSiNb非晶涂层形成机理和摩擦磨损行为

研发了一种FeAlCrBSiNb粉芯丝材,采用高速电弧喷涂技术在45钢基体上制备相应涂层.通过SEM,TEM和XRD表征涂层微观组织和相成分,阐述FeAlCrBSiNb非晶涂层的形成机理,利用显微硬度计,万能拉伸试验机和环-块式摩擦磨损试验机,分析涂层力学性能和摩擦磨损行为.结果表明:涂层主要由非晶相和弥散分布其中的α-(Fe),(Fe,Cr),CrB和Fe3Al微晶纳米晶相组成,非晶相体积含量大于91.3％;涂层呈层状结构,结构致密,总体孔隙率约为2％;平均显微硬度值为850 HV0.1,是基体45钢的4倍;优良的磨损抗力使其相对耐磨性是45钢的5倍,其磨损机制主要为剥落引起的剥落磨损.     

无人机编队飞行技术的研究现状与展望

无人机编队飞行是无人机及其应用技术发展研究的新热点.在分析无人机编队飞行特点的基础上,阐述了无人机编队飞行原理与方法的研究现状,并展望了其今后的主要应用前景.     

Formation and Composition of Planetesimals

The composition of planetesimals depends upon the epoch and the location of their formation in the solar nebula. Meteorites produced in the hot inner nebula contain refractory compounds. Volatiles were present in icy planetesimals and cometesimals produced in the cold outer nebula. However, the mechanism responsible for their trapping is still controversial. We argue for a general scenario valid in all regions of the turbulent nebula where water condensed as a crystalline ice (Hersant et al., 2004). Volatiles were trapped in the form of clathrate hydrates in the continuously cooling nebula. The epoch of clathration of a given species depends upon the temperature and the pressure required for the stability of the clathrate hydrate. The efficiency of the mechanism depends upon the local amount of ice available. This scenario is the only one so far which proposes a quantitative interpretation of the non detection of N₂ in several comets of the Oort cloud (Iro et al., 2003). It may explain the large variation of the CO abundance observed in comets and predicts an Ar/O ratio much less than the upper limit of 0.1 times the solar ratio estimated on C/2001 A2 (Weaver et al., 2002). Under the assumption that the amount of water ice present at 5 AU was higher than the value corresponding to the solar O/H ratio by a factor 2.2 at least, the clathration scenario reproduces the quasi uniform enrichment with respect to solar of the Ar, Kr, Xe, C, N and S elements measured in Jupiter by the Galileo probe. The interpretation of the non-uniform enrichment in C, N and S in Saturn requires that ice was less abundant at 10 AU than at 5 AU so that CO and N₂ were not clathrated in the feeding zone of the planet while CH₄, NH₃ and H₂S were. As a result, the 14N/15N ratio in Saturn should be intermediate between that in Jupiter and the terrestrial ratio. Ar and Kr should be solar while Xe should be enriched by a factor 17. The enrichments in C, N and S in Uranus and Neptune suggest that available ice was able to form clathrates of CH₄, CO and the NH₃ hydrate, but not the clathrate of N₂. The enrichment of oxygen by a factor 440 in Neptune inferred by Lodders and Fegley (1994) from the detection of CO in the troposphere of the planet is higher by at least a factor 2.5 than the lower limit of O/H required for the clathration of CO and CH4 and for the hydration of NH₃. If CO detected by Encrenaz et al. (2004) in Uranus originates from the interior of the planet, the O/H ratio in the envelope must be around of order of 260 times the solar ratio, then also consistent with the trapping of detected volatiles by clathration. It is predicted that Ar and Kr are solar in the two planets while Xe would be enriched by a factor 30 to 70. Observational tests of the validity of the clathration scenario are proposed.     

原位钛基复合材料中TiB的生成热力学及动力学

采用自蔓延高温合成（SHS）、感应熔炼和熔模精铸相结合的方法，利用Ti—B—Al体系制备出了原位自生TiB增强的钛基复合材料。借助XRD、SEM和TEM分析了复合材料的物相和增强体的形态。结果表明：在复合材料中只存在TiB增强体和Ti，无TiAl3杂质相形成，TiB增强体呈柱状短纤维，这与其B27晶体结构有关，且增强体／基体界面清洁无杂质污染，并从热力学和动力学两方面论述了在Ti—B—Al体系中制备TiB增强体的生成机制：在Ti-B—Al体系中，Al首先受热熔化使得Ti和B相继溶解于Al液中；Ti与Al之间先行发生化学反应形成Ti—Al金属间化合物，放出的热量进一步引发了溶解于液相中的B和Ti产生高温自蔓延形成Ti—B化合物。以热力学理论分析，应最终形成TiB2，但实际上由于动力学影响，最终形成了TiB。     

L10-TiAl金属间化合物Mn,Nb合金化电子结构的计算

采用第一原理赝势平面波方法计算了L10型TiAl金属间化合物中掺入Mn,Nb后的电子结构和价键结构.通过合金原子形成热得出Mn优先占据Al点阵位置,Nb优先占据Ti点阵位置.Mulliken聚居数分析发现Mn或Nb合金化后,分别降低了(001)和(002)面内的原子间键合强度,掺入Nb还降低了层间的原子间键合强度,而掺入Mn,则使层间原子间键合强度增加.整体上来讲,掺入Mn有利于改善TiAl的室温脆性,而掺入Nb,不利于改善TiAl的室温脆性.