舰载直升机任务航电系统及建模

介绍了美国海军舰载直升机的发展,着重阐述了"海鹰"直升机的发展,概述了其先进的任务航电系统,还对"海鹰"直升机的建模进行简单说明。     

快速可重组测控试验平台布线子系统的设计

在一种基于虚拟仪器的多功能快速可重组测控实验环境中,为了实现快速可重组思想,需要实现模块之间布线系统的设计。本文讨论了在Visual C＋＋开发平台下布线系统中线类的设计思想和实现过程,并对其中设计的主要函数和算法进行详细描述。     

多用途战斗机/涡扇发动机一体化循环参数优化

 针对多用途战斗机的特点,发展了基于飞/发一体化的涡扇发动机循环参数优化设计模型和相应的计算程序,优化设计模型中包括双变量控制涡扇发动机特性计算模型、进排气系统安装特性计算模型、飞机气动特性分析模型、重量组成分析模型、任务剖面分析模型、约束分析与任务分析模型和优化计算模型等。重点研究了多用途战斗机约束边界的获得方法,利用多岛遗传算法和自适应模拟退火优化算法,分别对现役多用途战斗机、不加力超声速巡航多用途战斗机以及下一代先进多用途战斗机用涡扇发动机循环参数进行了优化计算,对计算结果进行了分析,获得了对多用途战斗机用涡扇发动机循环参数选择有指导意义的结论。     

PROBA-3 mission and the Shadow Position Sensors: Metrology measurement concept and budget

PROBA-3 is a space mission of the European Space Agency that will test, and validate metrology and control systems for autonomous formation flying of two independent satellites. PROBA-3 will operate in a High Elliptic Orbit and when approaching the apogee at 6·10⁴ Km, the two spacecraft will align to realize a giant externally occulted coronagraph named ASPIICS, with the telescope on one satellite and the external occulter on the other one, at inter-satellite distance of 144.3 m. The formation will be maintained over 6 hrs across the apogee transit and during this time different validation operations will be performed to confirm the effectiveness of the formation flying metrology concept, the metrology control systems and algorithms, and the spacecraft manoeuvring. The observation of the Sun’s Corona in the field of view [1.08;3.0]R_Sun will represent the scientific tool to confirm the formation flying alignment. In this paper, we review the mission concept and we describe the Shadow Position Sensors (SPS), one of the metrological systems designed to provide high accuracy (sub-millimetre level) absolute and relative alignment measurement of the formation flying. The metrology algorithm developed to convert the SPS measurements in lateral and longitudinal movement estimation is also described and the measurement budget summarized.     

GOCE star tracker attitude quaternion calibration and combination

We analyse the inter-boresight angles (IBA) measured by the star trackers on board the GOCE satellite and find that they exhibit small offsets of 7–9″ with respect to the ones calculated from the rotation of the star tracker reference frames to the satellite reference frame. Further, we find small variations in the offsets with a peak-to-peak amplitude of up to 8″, which correlate with variations of the star trackers’ temperatures. Motivated by these findings, we present a method for combining the attitude quaternions measured by two or more star trackers that includes an estimation of relative attitude offsets between star trackers as a linear function of temperature. The method was used to correct and combine the star tracker attitude quaternions within the reprocessing of GOCE data performed in 2018. We demonstrate that the IBA calculated from the corrected star tracker attitude quaternions show no significant offsets with respect to the reference frame information. Finally, we show that neglecting the star tracker attitude offsets in the processing would result in perturbations in the gravity gradients that are visible at frequencies below 2?mHz and have a magnitude of up to 90?mE. The presented method avoids such perturbations to a large extent.     

“忠诚僚机”式有人/ 无人机协同作战概念 与任务管理技术研究

“忠诚僚机”式作战概念定义了有人机与无人机协同作战的新理念，颠覆了传统作战模式。在有人/ 无人机协同作战过程中，有人机以指挥者的角色，对作战任务进行分解、分配与管理。实现有人/ 无人机编队 之间在时间、空间上的协同与配合，而无人机在有人机的指挥下完成侦察与打击等任务。     

面向全月球探测的天基中继测控系统设计

中继测控是月球探测任务中必须解决的关键问题，特别是月球背面和两极地区的着陆和巡视探测任务以及载人登月任务。本文首先对国内外月球中继测控卫星的研究和发展情况进行了调研，分析了未来全月球探测对中继测控的需求。在此基础上，重点给出了面向全月球探测任务的天基中继测控系统设计方案，并仿真分析了该方案的中继测控性能。最后给出了简要的卫星设计方案。     

METHIS: Mercury thermal infrared spectrometer

The BepiColombo mission to Mercury is devoted to the thorough exploration of Mercury and its environment, with the aim to understand the processes of planetary formation and evolution in the hottest part of the protoplanetary nebula. This mission represents an unique opportunity for the European community to extend the understanding of the Solar Nebula evolution from its outer edge – ideally represented by comets – to its inner and warmer edge. Obviously this exploration asks for a detailed knowledge of the main constituents of the matter present in the different Solar System areas. Spectroscopy is a powerful tool to acquire this knowledge. We have participated with a large consortium of European researchers to the development of the Rosetta imaging spectrometer. We propose here to use our experience to develop a newly designed spectrometer to investigate the mineralogical composition of the Mercurial surface. Given the particular thermodynamical situation of the Mercurial surface, we have developed a concept that combines a medium IR low spectral resolution imager with a moderate spectral resolution NIR point spectrometer. The main goal of METHIS is to provide the mineralogical characterisation of the surface with sufficient spectral resolution in a scientifically diagnostic spectral range.     

基层服务型党组织建设的现实依据与根本路径

加强基层服务型党组织建设,有利于更好地履行党的根本宗旨和根本执政理念,是密切党群关系的根本保证;有利于提高基层社会的治理水平,其关键是要准确把握基层服务型党组织的理论和实践内涵、本质属性,以及找准基层服务型党组织建设的着力点。未来一段时期的基层服务型党组织建设,应重点围绕增强服务意识、做强服务队伍、创新服务载体、加大基层投入、提高治理能力五个方面来推进。     

A multiple-rendezvous,sample-return mission to two near-Earth asteroids

We propose a dual-rendezvous mission, targeting near-Earth asteroids, including sample-return. The mission, Asteroid Sampling Mission (ASM), consists of two parts: (i) flyby and remote sensing of a Q-type asteroid, and (ii) sampling of a V-type asteroid. The targeted undifferentiated Q-type are found mainly in the near-Earth space, and to this date have not been the target of a space mission. We have chosen, for our sampling target, an asteroid from the basaltic class (V-type), as asteroids in this class exhibit spectral signatures that resemble those of the well-studied Howardite–Eucrite–Diogenite (HED) meteorite suite. With this mission, we expect to answer specific questions about the links between differentiated meteorites and asteroids, as well as gain further insight into the broader issues of early Solar System (SS) evolution and the formation of terrestrial planets. To achieve the mission, we designed a spacecraft with a dry mass of less than 3 tonnes that uses electric propulsion with a solar-electric power supply of 15 kW at 1 Astronomical Unit (AU). The mission includes a series of remote sensing instruments, envisages landing of the whole spacecraft on the sampling target, and employs an innovative sampling mechanism. Launch is foreseen to occur in 2018, as the designed timetable, and the mission would last about 10 years, bringing back a 150 g subsurface sample within a small re-entry capsule. This paper is a work presented at the 2008 Summer School Alpbach,“Sample return from the Moon, asteroids and comets” organized by the Aeronautics and Space Agency of the Austrian Research Promotion Agency. It is co-sponsored by ESA and the national space authorities of its Member and Co-operating States, with the support of the International Space Science Institute and Austrospace.