空间在轨装配技术综述

代表国家科技实力的空间站、空间望远镜、大型通信天线、空间太阳能电站、在轨燃料补给站、深空探测中转站及地外基地等空间大型平台和基础设施的建设需求日益迫切,如何对此进行智能自主建造是当前的巨大技术挑战。鉴于大型平台与基础设施在未来空间探索中的重要性,国内外航天研究机构均提出并发展了在轨装配的系列技术方案。本文主要对在轨装配研究现状和技术发展情况进行系统地综述。首先分析了有人与无人在轨装配的国内外技术进展,总结了在轨装配技术的发展路线、装配层次与方法;然后在此基础上,详细梳理了在轨装配的技术需求和应用前景,并得出在轨装配的使能关键技术——模块化技术、机器人技术和地面模拟装配技术,预期为中国未来的空间在轨装配研究提供有益的参考。     

Composition of the Volatile Material in Halley's Coma from In Situ Measurements

The investigation of the volatile material in the coma of comets is a key to understanding the origin of cometary material, the physical and chemical conditions in the early solar system, the process of comet formation, and the changes that comets have undergone during the last 4.6 billion years. So far, in situ investigations of the volatile constituents have been confined to a single comet, namely P/Halley in 1986. Although, the Giotto mission gave only a few hours of data from the coma, it has yielded a surprising amount of new data and has advanced cometary science by a large step. In the present article the most important results of the measurements of the volatile material of Halley's comet are summarized and an overview of the identified molecules is given. Furthermore, a list of identified radicals and unstable molecules is presented for the first time. At least one of the radicals, namely CH₂, seems to be present as such in the cometary ice. As an outlook to the future we present a list of open questions concerning cometary volatiles and a short preview on the next generation of mass spectrometers that are being built for the International Rosetta Mission to explore the coma of Comet Wirtanen. This revised version was published online in June 2006 with corrections to the Cover Date.     

Rapporteur Paper on the Composition of Comets

The ISSI workshop on “Origin and evolution of comet nuclei” had the goal to put together recent scientific findings concerning the “life” of a comet from the formation of the material in a dark molecular cloud to the accretion in the early solar system, from cometesimals to comet nuclei which were shaped and altered by cosmic rays, by radioisotopic heating, to their sublimation in the inner solar system. Astronomers, space researchers, modelers and laboratory experimentalists tried to draw the coherent picture. However, it became clear that there are still a lot of open questions, findings which seem to contradict each other, missing laboratory data, and experimental biases not taken into account. The Rosetta mission will make a big step forward in cometary science, but it will almost certainly not be able to resolve all questions. The main outcome of this workshop was the fact that comets are much more diverse than commonly thought and they are not only different from comet to comet but may consist of morphologically and chemically inhomogeneous cometesimals which may even have different places of origin.     

基于深度学习的小目标检测研究进展

随着深度学习方法的快速发展,目标检测作为计算机视觉领域中最基本、最具有挑战性的任务之一,已取得了令人瞩目的进展。现有的算法大多针对于具有一定尺寸或比例的大中型目标,但由于待测目标尺寸小、特征弱等原因,对小目标的检测性能还远远不能令人满意。小目标检测（SOT）作为一种广泛应用于室外远程拍摄和航空遥感场景的技术,近年来受到了广泛的关注,各种方法层出不穷,但是目前对该问题的全面综述较少。从问题定义、算法分析、应用介绍、方向展望等方面对基于深度学习的小目标检测研究进展进行了综述。首先,给出了小目标检测问题的定义,阐述了其技术难点及在实际应用中面临的挑战;接着,从8个不同角度分析了检测器对小目标检测精度较低的主要原因及相应的改进方法,详细归纳总结了小目标检测在各技术方面的研究工作;然后介绍了几个特定场景下小目标检测算法的典型应用;最后,对小目标检测未来的发展趋势进行展望,提出可行的研究方向,期望为该领域的研究工作提供可借鉴和参考的思路。     

Cometary Materials: Progress Toward Understanding the Composition in the Outer Solar Nebula

A major objective of the workshop was to learn about the chemical composition, physical structure, and thermodynamic conditions of the outer parts of the solar nebula where comets formed. Here we sum up what we have learned from years of research about the molecular constituents of comet comae primarily from in situ measurements of Comet 1P/Halley and remote sensing of Comets 1P/Halley, Hale-Bopp (C/1995 O1), and Hyakutake (C/1996 B2). These three bright comets are presumably captured Oort cloud comets. We summarize the analyses of these data to predict the composition of comet nuclei and project them further to the composition, structure, and thermodynamic conditions in the nebula. Near-future comet missions are directed toward less active short-period Jupiter-family comets. Thus, future analyses will afford a better understanding of the diversity of these two major groups of comets and their respective regions of origin in the solar or presolar nebula. We conclude with recommendations for determining critical data needed to aid in further analyses. Results of the workshop provide new guidelines and constraints for modeling the solar nebula. This revised version was published online in June 2006 with corrections to the Cover Date.     

小型固定翼无人机集群综述和未来发展综述

围绕小型固定翼无人机集群这一难度高、发展快、应用前景广阔、多学科交叉的新方向,从集群系统内涵、现有典型项目、关键技术3个角度综述了国内外小型固定翼无人机集群的研究现状。在系统梳理集群系统内涵和应用优势的基础上,从集群协同模式探索、分布指挥体系构建、核心关键技术突破和集群验证等4个视角总结现有典型项目,从体系架构、通信组网、决策与规划、飞机平台、集群飞行、集群安全与集群指控等7个核心点综述了技术研究现状。最后,综合小型固定翼无人机集群中亟需解决的关键技术,展望了这一领域未来的发展趋势。     

叶轮机械颤振研究进展 “两机专刊”

叶轮机械颤振是航空发动机、燃气轮机安全运行的重要威胁,一旦出现将严重影响设备的安全性并降低使用寿命。但颤振发生机理复杂,影响气弹稳定性参数多,流动结构和关键参数相互耦合,因此颤振一直是叶轮机械的研究难点。本文从颤振发生机理的角度,重点综述了近十年来关于颤振发生机理的新发现和新进展,其中包括流动结构、振动模态以及声波传播与反射等方面。在此基础上,结合工程实际简要总结了颤振抑制方法,以及不同方法的应用可行性。最后结合作者的思考,提出了叶轮机械颤振研究的重点方向。     

航空发动机失谐叶盘动态特性研究进展

航空发动机叶盘结构中不可避免存在的失谐会严重影响发动机的结构完整性和可靠性,国内外针对这一问题进行了大量深入的研究。详述了失谐叶盘建模、模型减缩、动态特性分析及评价等方面的研究现状,重点介绍多级叶盘和几何失谐叶盘的建模和动态特性分析等方面的最新研究进展,并对失谐叶盘未来研究方向进行了预测。     

Mupus – A Thermal and Mechanical Properties Probe for the Rosetta Lander Philae

MUPUS, the multi purpose sensor package onboard the Rosetta lander Philae, will measure the energy balance and the physical parameters in the near-surface layers – up to about 30 cm depth- of the nucleus of Rosetta’s target comet Churyumov-Gerasimenko. Moreover it will monitor changes in these parameters over time as the comet approaches the sun. Among the parameters studied are the density, the porosity, cohesion, the thermal diffusivity and conductivity, and temperature. The data should increase our knowledge of how comets work, and how the coma gases form. The data may also be used to constrain the microstructure of the nucleus material. Changes with time of physical properties will reveal timescales and possibly the nature of processes that modify the material close to the surface. Thereby, the data will indicate how pristine cometary matter sampled and analysed by other experiments on Philae really is.     

航空发动机控制系统的研发与展望

对国内外军用航空发动机控制系统的研制现状和今后的发展方向进行了归纳和分析,主要对主燃油控制、加力燃油控制、尾喷管控制、防喘控制、发动机状态监视和故障诊断各系统的技术特点,方案选择,研究动向进行了介绍和评述。从航空发动机控制系统近年来取得的进展,特别是全权限数字电子控制(FADEC)技术的研究和应用,可以看出航空发动机控制系统的发展潜力巨大,将会对飞机和航空发动机的研制和发展产生巨大的影响。      

系留悬浮式风力发电技术的研究进展与展望

风力发电作为清洁能源利用的重要方式,具有无污染、可再生、方便采集等特点,近年来得到快速发展。相对于传统低空风力发电,系留悬浮式风力发电具有容量系数高、发电成本低等优点,拥有更大的开发价值和发展潜力,已有多个国家开展研究并取得一定成果。本文通过对系留悬浮式风力发电技术发展的调研,归纳四种系留悬浮式风力发电技术类型,分析各技术类型的工作原理与特点,总结未来系留悬浮式风力发电需要重点突破的轻质高强系留缆绳设计与制造、高性能囊体复合材料、稳定与智能控制、高效风力发电飞行平台总体设计、便利展开部署五种关键技术,为后续研究提供参考。     

Concepts for the curation,primary examination,and allocation of comet nucleus samples by a comet sample receiving laboratory

The Comet Nucleus Sample Return Mission ROSETTA, a cornerstone mission of ESA jointly planned with NASA, requires the implementation of a highly sophisticated curatorial facility for the returned samples. A concept for the instrumentation and the mode of operation of a Comet Sample Receiving Laboratory (CSRL) is proposed. The main elements of the facility are: (1) cryogenic evacuated cabinets with robotic manipulators, (2) devices for sample dissection, aliquotisation, phase separation, and thin section preparation, and (3) instrumentation for non-destructive chemical and physical analyses and facilities for destructive mineralogical, textural, and (micro)chemical analyses. It is recommended that a very detailed Primary Sample Examination and Analysis be performed on a small representative fraction of the samples at the P-T-conditions of the parent comet nucleus before sample aliquots are released to Principal Investigators. The CSRL should be staffed with top rank personnel and supervised by an international peer review panel which may also be responsible for the selection of investigators and the allocation of samples.     

GEMS at the Galactic Cosmic-Ray Source

Galactic cosmic rays probably predominantly originate from shock-accelerated gas and dust in superbubbles. It is usually assumed that the shock-accelerated dust is quickly destroyed by sputtering. However, it may be that some of the dust can survive bombardment by the high-metallicity gas in the superbubble interior, and that some of that dust has been incorporated into solar system materials. Interplanetary dust particles (IDPs) contain enigmatic submicron components called GEMS (Glass with Embedded Metal and Sulfides). These GEMS have properties that closely match those expected of a population of surviving shock-accelerated dust at the GCR source (Westphal and Bradley in Astrophys. J. 617:1131, 2004). In order to test the hypothesis that GEMS are synthesized from shock-accelerated dust in superbubbles, we plan to measure the relative abundances of Fe, Zr, and Mo isotopes in GEMS using the new Resonance Ionization Mass Spectrometer at Argonne National Laboratory. If GEMS are synthesized from shock-accelerated dust in superbubbles, they should exhibit isotopic anomalies in Fe, Zr and Mo: specificially, enhancements in the r-only isotopes ⁹⁶Zr and ¹⁰⁰Mo, and separately in ⁵⁸Fe, should be observed. We review also recent developments in observations of GEMS, laboratory synthesis of GEMS-like materials, and implications of observations of GEMS-like materials in Stardust samples.     

The Deep Impact Earth-Based Campaign

Prior to the selection of the comet 9P/Tempel 1 as the Deep Impact mission target, the comet was not well observed. From 1999 through the present there has been an intensive world-wide observing campaign designed to obtain mission critical information about the target nucleus, including the nucleus size, albedo, rotation rate, rotation state, phase function, and the development of the dust and gas coma. The specific observing schemes used to obtain this information and the resources needed are presented here. The Deep Impact mission is unique in that part of the mission observations will rely on an Earth-based (ground and orbital) suite of complementary observations of the comet just prior to impact and in the weeks following. While the impact should result in new cometary activity, the actual physical outcome is uncertain, and the Earth-based observations must allow for a wide range of post-impact phenomena. A world-wide coordinated effort for these observations is described.     

燃料浓度分布激光诊断方法与应用

航空发动机内部燃料浓度分布情况影响其性能,诸如点火性能、燃烧效率、污染物生成和出口温度场等,因此,燃料浓度分布研究十分重要。近年来,基于激光的非接触测量与诊断技术快速发展,平面激光诱导荧光（PLIF）、Raman散射、Rayleigh散射、Mie散射、激光诱导击穿光谱（LIBS）、可调二极管激光吸收光谱（TDLAS）等非接触测量手段已成功应用于燃料浓度分布的诊断研究中。介绍了上述基于激光来诊断燃料浓度分布技术的基本工作原理及研究进展,分析对比了各种测量手段的优缺点,提出了基于单台高能量激光器同时测量多组PLIF组分、基于体激光诱导荧光（VLIF）发展V-Rayleigh散射和V-Mie散射技术等新的测量思路,展望了这几种激光诊断技术在燃料浓度分布研究方面的发展趋势,未来航空发动机内部的燃料浓度测量将会朝着高速瞬时演化过程的3D成像方向发展。     

On the Prediction of CO Outgassing from Comets Hale-Bopp and Wirtanen

The gas flux from a volatile icy-dust mixture is computed using a comet nucleus thermal model in order to study the evolution of CO outgassing during several apparitions from long-period Comet Hale-Bopp and short-period Comet Wirtanen. The comet model assumes a spherical, porous body containing a dust component, one major ice component (H₂O), and one minor ice component of higher volatility (CO). The initial chemical composition is assumed to be homogeneous. The following processes are taken into account: heat and gas diffusion inside the rotating nucleus; release of outward diffusing gas from the comet nucleus; chemical differentiation by sublimation of volatile ices in the surface layers and recondensation of gas in deeper, cooler layers. A 2-D time dependent solution is obtained through the dependence of the boundary conditions on the local solar illumination as the nucleus rotates. The model for Comet Hale-Bopp was compared with observational measurements (Biver et al., 1999). The best agreement was obtained for a model with amorphous water ice and CO, assuming that a part of the latter is trapped by the water ice, another part is condensed as an independent ice phase. The model confirms that sublimation of CO ice at large heliocentric distance produces a gradual increase in the comet's activity as it approaches the Sun. Crystallization of amorphous water ice begins at 7 AU from the Sun, but no outbursts were found. Seasonal effects and thermal inertia of the nucleus material lead to larger CO outgassing rates as the comet recedes from the Sun. In the second part of this work the model was run with the orbital parameters of Comet Wirtanen. Unlike Comet Hale-Bopp, the predicted CO outgassing from Comet Wirtanen is almost constant throughout its orbit. Such behavior can be explained by a thermally evolved and chemically differentiated comet nucleus. This revised version was published online in June 2006 with corrections to the Cover Date.     

The Earth’s Magnetopause: Reconstruction of Motion and Structure

The Earth’s magnetosphere is an accessible region for improving our knowledge of the dynamics of collisionless plasmas. We focus here on the magnetopause a typical plasma discontinuity. We discuss recent developments in describing the structure of the magnetopause by means of reconstruction techniques, which translate in situ data into spatial information. We review short- and long-duration reconstruction methods and discuss the ideas behind them. The emphasis is on long-duration reconstruction methods in a multi-spacecraft context.     

The magnetosheath and magnetotail of Venus

We describe the observational history and assess the current understanding of the magnetosheath and magnetotail of Venus, stressing recent developments. We make recommendations for research that can be done using existing observations, as well as desirable trajectory and instrumentation characteristics for future spacecraft missions.     

Structural evolution of cometary surfaces

Comets with a high content of organics and light molecules are expected under cosmic radiation to gain a relatively unreactive crust and less volatile material to some ten metres deep. Interstellar dust impacts act to loosen and turn over 1 cm of the surface. We discuss how far this accords with observations of cometary dust halos and new versus old comets. Two key material properties have emerged from recent studies. Firstly, the source of cometary volatiles is not ice in the sense of material with a single sublimation energy. Secondly, the particulates are not simply mineral dust but include much organic material, some of which undergoes chemical processing and exchanges with the gaseous environment. Consistent with these properties, a coherent crust rather than a mantle of loose grains would build up to cover much of the nucleus of periodic comets. It would consolidate by cooking in the solar radiation, especially at peak temperatures around perihelion. There are two disjoint surface phases: one of volatile material, the other the refractory crust, the former deepening into crater-like hollows over successive apparitions. The transition to non-volatile crust is unstable, subject to competing consolidation and disruption processes, and sensitive to seasonal changes. A comet dims and becomes asteroidal as the inert crust extends over the erosion craters, and may only be rejuvenated via collision with a boulder-sized impactor or perturbation of the orbit to smaller perihelion distance.     

A review on fault-tolerant cooperative control of multiple unmanned aerial vehicles

This paper presents the recent developments in Fault-Tolerant Cooperative Control(FTCC) of multiple unmanned aerial vehicles(multi-UAVs). To facilitate the analyses of FTCC methods for multi-UAVs, the formation control strategies under fault-free flight conditions of multi-UAVs are first summarized and analyzed, including the leader-following, behavior-based, virtual structure, collision avoidance, algebraic graph-based, and close formation control methods,which are viewed as the cooperative con...