基于并行禁忌遗传算法(PTGA)的预警卫星传感器调度研究

对预警卫星的传感器调度进行了研究，提出了传感器管理调度的系统组成。通过对传感器调度的分析，建立起相应的数学模型，定义了评价指标。结合并行遗传算法和禁忌搜索的特点，提出了一种新的解决预警卫星传感器调度问题的并行禁忌遗传算法(PTGA)。该算法采用多种群和禁忌搜索思想改进遗传算法的性能，从而提高整个算法的收敛速度和精度。实验结果表明该算法有效地解决了多目标情况下的传感器实时调度问题，并优于一般启发式算法。     

卫星图像采集任务调度系统的设计与实现

随着卫星遥感技术的高速发展 ,卫星图像在众多领域有了广泛的应用。文章给出了一个卫星图像采集任务调度系统的总体结构及其功能 ,讨论了该系统实现过程中的卫星资源描述、卫星图像采集任务描述、调度引擎、卫星时间窗口的仿真计算、调度结果的可视化展现等关键技术 ,归纳了系统的特点 ,并总结了今后系统的研究方向     

机载聚束式SAR天线波束指向控制分析

建立波束控制条件下的机载聚束式SAR的天线指向及成像数学模型,证实天线波束指向被控造成回波信号的幅度调制,引起成对回波,从而影响成像质量。此外,分析波束指向控制比率与测绘带方位宽度、图像动态范围的制约关系,提出设计机载聚束式SAR天线波束指向控制比率的基本原则。最后,通过计算机仿真,验证理论分析的正确性。     

稀疏孔径成像系统发展概况

介绍了稀疏孔径成像系统的发展现状。重点介绍了系统的成像原理和种类，国外的研究进展以及系统实现的关键技术和应用前景。     

基于最小成本的飞机着陆规划算法

在以往着陆规划中，较少考虑公司的成本。利用航班的成本函数，建立了满足着陆间隔、着陆时间段等约束的着陆规划模型，提出了一种使用局部搜索和线性规划的启发式算法。实例验算表明，所给模型及算法可以在合理的时间内求解大规模规划问题，有效地降低公司成本。     

遗传算法在飞机着陆调度问题上的应用

用遗传算法对飞机着陆调度问题的两个方面:队列顺序的确定和跑道指派进行了研究.队列顺序采用飞机编号的单一整数染色体编码方案,配合相应的变异、交叉算子,避免了后代非法解的问题.跑道指派则在适值函数计算中,基于对列最短的原则来加以确定,避免了对队列顺序和跑道指派进行分别编码.算例研究了单跑道与双跑道两种情况.计算结果表明,这种编码方案以及变异、交叉算子对这一问题具有很好的效果,可在普通PC机上实现雷达扫描周期内的实时计算要求.     

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.     

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.     

调频连续波SAR成像算法研究

机载遥感微波成像雷达在地球观测特别是在城市应用中起着非常重要的作用,现在人们对体积小、重量轻、成本效益高、分辨率高的成像雷达越来越关注。调频连续波(FM-CW)技术和SAR相结合的调频连续波合成孔径雷达应运而生。论文详细分析了FM-CW SAR的成像过程,提出了去除相位残余的算法,并给出仿真结果。通过仿真可以看出,调频连续波合成孔径雷达具有较好的空间分辨力。     

加工时间依赖工件位置的单机成组排序问题

排序问题是一类重要的组合优化问题,现代排序问题突破了经典排序问题的种种假设,有着越来越广阔的应用前景。对加工时间依赖于工件位置的单机成组排序问题进行了研究,讨论了成组技术中,要求同一组内工件必须连续加工,加工时间的函数变量是工件所在的加工位置,目标函数分别为极小化最大完工时间与总完工时间。分别给出其多项式时间的最优算法。