无人机近距离编队飞行模型建立及控制器设计

针对无人机编队飞行问题，提出了无人机近距离编队飞行的建模方法。采用全状态量反馈．同时将气动干扰作为非线性反馈，设计出一套适用于无人机近距离编队飞行的自动驾驶仪。通过仿真验证，表明此控制器能较好地稳定优化后的编队飞行结构，并具有良好的鲁棒性。     

STUDIES ON AIRCRAFT TOTAL ENERGY FLIGHT CONTROL SYSTEM：NONLINEAR SYSTEM INTEGRATION AND SIMULATION

ＳＴＵＤＩＥＳＯＮＡＩＲＣＲＡＦＴＴＯＴＡＬＥＮＥＲＧＹＦＬＩＧＨＴＣＯＮＴＲＯＬＳＹＳＴＥＭ：ＮＯＮＬＩＮＥＡＲＳＹＳＴＥＭＩＮＴＥＧＲＡＴＩＯＮＡＮＤＳＩＭＵＬＡＴＩＯＮＷｕＳｈｕｆａｎ；ＳｈｅｎＹｏｎｇｚｈａｎｇ；ＧｕｏＳｕｏｆｅｎｇ（Ｄｅｐｔ...     

多通道飞控计算机软件的调试支持

通常多通道飞控计算机的程序存储和执行均在EPROM中完成 ,程序的前期开发和调试则通过将其加载到RAM中进行。但是 ,由于目前通用的调试系统都是单通道的源程序级调试系统 ,若采用它们的简单组合 ,其性能无法满足多通道程序的调试需求 ;另外由于RAM和EPROM访问时序的不同 ,在RAM中调试正确的程序不能证明在EPROM中执行也正确。本文介绍了一种支持多通道飞控计算机软件调试功能的软硬件设计。     

关于《航班延误经济补偿指导意见》的几个问题

在民用航空运输中,由于多种原因,航班延误难以避免,因航班延误引起的纠纷时有发生。为了提高航班正常率,减少因航班延误引起的矛盾,中国民用航空总局2004年发布了《中国民用航空总局对国内航空公司因自身原因造成航班延误给予旅客经济补偿的指导意见(试行)》,就航班延误经济补偿的条件、标准、方式提出了原则性的建议。但具体补偿标准由航空公司自行制定。航班延误经济补偿不同于延误赔偿,二者有着质的区别。     

鲁棒颤振裕度法的应用

介绍了一种新的确定颤振边界的方法——鲁棒颤振裕度法。利用结构奇异值理论将颤振理论模型和试飞数据有机结合起来,进行了颤振边界预测。仿真结果表明,该方法是可行的。     

基于8098单片机的飞行指引系统综合测试装置

介绍一种基于8098单片机的飞行指引系统综合测试装置，给出了飞行指引系统综合测试装置的用途。主要硬件组成和软件设计方法。     

基于干扰观测器的新一代歼击机鲁棒飞行逆控制器设计

基于干扰观测器设计了新一代歼击机的鲁棒飞行逆控制器。根据时标分离的原则，将机动飞机分为快慢不同的回路。采用动态逆方法设计了快回路和慢回路控制器，并在慢回路用干扰观测器估计飞机所受的扰动，同时，用于在线补偿动态逆误差。仿真结果表明，该设计合理。     

Magnetosphere Imaging Instrument (MIMI) on the Cassini Mission to Saturn/Titan

The magnetospheric imaging instrument (MIMI) is a neutral and charged particle detection system on the Cassini orbiter spacecraft designed to perform both global imaging and in-situ measurements to study the overall configuration and dynamics of Saturn’s magnetosphere and its interactions with the solar wind, Saturn’s atmosphere, Titan, and the icy satellites. The processes responsible for Saturn’s aurora will be investigated; a search will be performed for substorms at Saturn; and the origins of magnetospheric hot plasmas will be determined. Further, the Jovian magnetosphere and Io torus will be imaged during Jupiter flyby. The investigative approach is twofold. (1) Perform remote sensing of the magnetospheric energetic (E > 7 keV) ion plasmas by detecting and imaging charge-exchange neutrals, created when magnetospheric ions capture electrons from ambient neutral gas. Such escaping neutrals were detected by the Voyager l spacecraft outside Saturn’s magnetosphere and can be used like photons to form images of the emitting regions, as has been demonstrated at Earth. (2) Determine through in-situ measurements the 3-D particle distribution functions including ion composition and charge states (E > 3 keV/e). The combination of in-situ measurements with global images, together with analysis and interpretation techniques that include direct “forward modeling’’ and deconvolution by tomography, is expected to yield a global assessment of magnetospheric structure and dynamics, including (a) magnetospheric ring currents and hot plasma populations, (b) magnetic field distortions, (c) electric field configuration, (d) particle injection boundaries associated with magnetic storms and substorms, and (e) the connection of the magnetosphere to ionospheric altitudes. Titan and its torus will stand out in energetic neutral images throughout the Cassini orbit, and thus serve as a continuous remote probe of ion flux variations near 20R _S (e.g., magnetopause crossings and substorm plasma injections). The Titan exosphere and its cometary interaction with magnetospheric plasmas will be imaged in detail on each flyby. The three principal sensors of MIMI consists of an ion and neutral camera (INCA), a charge–energy–mass-spectrometer (CHEMS) essentially identical to our instrument flown on the ISTP/Geotail spacecraft, and the low energy magnetospheric measurements system (LEMMS), an advanced design of one of our sensors flown on the Galileo spacecraft. The INCA head is a large geometry factor (G ∼ 2.4 cm² sr) foil time-of-flight (TOF) camera that separately registers the incident direction of either energetic neutral atoms (ENA) or ion species (≥5^∘ full width half maximum) over the range 7 keV/nuc < E < 3 MeV/nuc. CHEMS uses electrostatic deflection, TOF, and energy measurement to determine ion energy, charge state, mass, and 3-D anisotropy in the range 3 ≤ E ≤ 220 keV/e with good (∼0.05 cm² sr) sensitivity. LEMMS is a two-ended telescope that measures ions in the range 0.03 ≤ E ≤ 18 MeV and electrons 0.015 ≤ E≤ 0.884 MeV in the forward direction (G ∼ 0.02 cm² sr), while high energy electrons (0.1–5 MeV) and ions (1.6–160 MeV) are measured from the back direction (G ∼ 0.4 cm² sr). The latter are relevant to inner magnetosphere studies of diffusion processes and satellite microsignatures as well as cosmic ray albedo neutron decay (CRAND). Our analyses of Voyager energetic neutral particle and Lyman-α measurements show that INCA will provide statistically significant global magnetospheric images from a distance of ∼60 R _S every 2–3 h (every ∼10 min from ∼20 R _S). Moreover, during Titan flybys, INCA will provide images of the interaction of the Titan exosphere with the Saturn magnetosphere every 1.5 min. Time resolution for charged particle measurements can be < 0.1 s, which is more than adequate for microsignature studies. Data obtained during Venus-2 flyby and Earth swingby in June and August 1999, respectively, and Jupiter flyby in December 2000 to January 2001 show that the instrument is performing well, has made important and heretofore unobtainable measurements in interplanetary space at Jupiter, and will likely obtain high-quality data throughout each orbit of the Cassini mission at Saturn. Sample data from each of the three sensors during the August 18 Earth swingby are shown, including the first ENA image of part of the ring current obtained by an instrument specifically designed for this purpose. Similarily, measurements in cis-Jovian space include the first detailed charge state determination of Iogenic ions and several ENA images of that planet’s magnetosphere.This revised version was published online in July 2005 with a corrected cover date.     

可重复使用运载器磁悬浮助推发射参数研究

针对磁悬浮助推水平起飞运载器这种新型发射概念,采用概念性分析方法,研究地面发射参数对可重复使用运载器性能的影响规律。结果表明,助推发射水平起飞运载器在降低初始推重比、推进剂和结构质量等方面具有优势,最后得出地面发射参数的一组优化值。     

航班调度应急管理研究

航班调度应急管理是针对频发、突发事件的管理方法,它以提高顾客利益与航空公司利益的综合效应为目标,涵盖了制定航班计划到执行计划的整个过程.本文就航班调度应急管理的两种方法：鲁棒调度与受扰恢复策略,论述了两者的研究重点、数学模型和算法.