会议筹备优化设计

根据代表回执的住房要求数据,通过曲线拟合估计出本届与会代表人数,定义了距离数量指标和代表满意数量指标,并对指标赋予权重,再利用线性规划,建立优化模型,得到应预定的宾馆及每个宾馆应预定的房间;对会议室的租借问题,将各分组会议分为三个级别,并根据其重要性赋予相应的权重,再结合与会代表总人数,求得各级别会议的与会代表人数,选定会议室;对租车方案,以租车总费用最少为目标函数,以租借三种类型作为约束条件,建立优化模型,利用Lingo软件编程求解。     

考虑协同航路规划的多无人机任务分配

针对多无人机任务分配与协同航路规划问题，以分布式合同网拍卖算法为基础，构建无人机集群任务拍卖架构与拍卖收益函数，结合模拟退火算法协调任务执行次序，采用A^*算法完成两任务点间航程预估，在任务分配阶段同步完成多无人机间协同航路的初规划，确定最佳任务执行次序，实现任务分配与协同航路规划的紧耦合。仿真结果表明，在考虑禁飞区、障碍威胁情况下，该算法能够有效完成多架无人机不同类型任务的分配，且目标分配、执行次序合理，总执行代价小，各机间负载均衡；在任务分配阶段考虑协同航路规划具有明显的效果，能够有效提高任务分配的合理性。     

区域防空组网雷达对跟踪目标交接班模型研究

组网雷达对跟踪目标进行交接班是对目标进行稳定跟踪的基础.在综合考虑组网雷达的作战背景的基础上,分析了接班雷达选择模型和交班时机选择模型.在接班雷达选择模型中,将定位精度和目标在接班雷达探测区域的飞行时间作为接班雷达选择的两个指标,并利用基于理想点的多属性决策方法进行决策,可保证对目标跟踪的连续性并防止频繁交接班情况的发生.最后对提出的交接班模型进行了仿真验证.     

ERP设备管理软件中数据库的跨平台研究

ERP系统的顺利实施可以实现对企业资源的合理调配,满足最大化地创造社会财富的要求。本文依据在ERP设备管理软件的实际开发过程中使用到的一些数据库技术,通过实例介绍了在ERP系统的开发设计中如何实现数据库的跨平台特性。     

空间站应用的发展及存在问题

简要介绍了国外载人空间站应用的发展和"国际空间站"应用的现状,重点总结和分析空间站应用面临的挑战性问题,包括应用人时不足,建设进度推迟,有效载荷配置不到位,运输能力不够,供电欠缺,设备和器材无序安装与存放,缺少合理建造与应用的综合规划和协调程序,以及潜在的设备故障与人为失误,同时,给出了解决这些问题的思路和途径。     

“多对多”模式下GEO卫星在轨加注任务规划

随着在轨服务技术的发展和对航天器发射运营成本的控制，航天器在轨服务模式将由“一对一”服务逐步发展为“一对多”“多对多”的服务模式。在具有多个服务目标的模式下，针对服务航天器的任务分配与规划将变得尤为关键。因此，本文研究了多服务航天器为多个地球同步轨道(GEO)卫星进行在轨加注的任务规划问题。首先，考虑服务航天器容量约束、服务路径约束等多类约束条件，以最小化燃料消耗为优化指标，以每个服务航天器的服务顺序为决策变量，建立“多对多”在轨加注任务规划模型。其次，针对遗传算法局部搜索能力差、易陷入局部最优的缺陷，设计了一种将大邻域搜索算法和遗传算法相结合的混合启发式算法(LNS-GA)，用以求解该任务规划问题。该算法利用大邻域搜索算法中的“破坏”和“修复”思想，对遗传算法每一代种群中的精英个体进行进一步的迭代搜索，从而增强算法的局部搜索能力。最后，通过设定的仿真场景与单一遗传算法进行仿真对比，验证了本文所提出算法的有效性和优越性。     

规划未来塑造自我

通过对有关大学生心理困惑方面的问卷调查分析,笔者发现目前大学生在学习生活中存在着很大的盲目性,解决问题的出路之一是把握学年特点,根据自己的实际情况,作出合理规划,并付诸实践.     

作战任务对防空导弹武器系统威胁判断结果的影响分析

梳理了判断涉及的目标参数结合武器系统的作战任务需求。提出了一种根据作战任务建立威胁判断数学模型的指导方案，给出了如何应用该方案对已有模型进行改进的措施。仿真分析中对一种基于层次分析法和模糊综合决策法的空袭目标威胁评估模型进行改进，在多目标的空袭环境中演示了不同作战任务对目标威胁判断结果的影响，验证了模型的工程参考价值。     

A Portrait of the Nucleus of Comet 67P/Churyumov-Gerasimenko

In 2003, comet 67P/Churyumov–Gerasimenko was selected as the new target of the Rosetta mission as the most suitable alternative to the original target, comet 46P/Wirtanen, on the basis of orbital considerations even though very little was known about the physical properties of its nucleus. In a matter of a few years and based on highly focused observational campaigns as well as thorough theoretical investigations, a detailed portrait of this nucleus has been established that will serve as a baseline for planning the Rosetta operations and observations. In this review article, we present a novel method to determine the size and shape of a cometary nucleus: several visible light curves were inverted to produce a size–scale free three–dimensional shape, the size scaling being imposed by a thermal light curve. The procedure converges to two solutions which are only marginally different. The nucleus of comet 67P/Churyumov–Gerasimenko emerges as an irregular body with an effective radius (that of the sphere having the same volume) = 1.72 km and moderate axial ratios a/b = 1.26 and a/c = 1.5 to 1.6. The overall dimensions measured along the principal axis for the two solutions are 4.49–4.75 km, 3.54–3.77 km and 2.94–2.92 km. The nucleus is found to be in principal axis rotation with a period = 12.4–12.7 h. Merging all observational constraints allow us to specify two regions for the direction of the rotational axis of the nucleus: RA = 220°^+50° _−30° and Dec = −70^° ± 10^° (retrograde rotation) or RA = 40°^+50° _-30° and Dec = +70^°± 10^° (prograde), the better convergence of the various determinations presently favoring the first solution. The phase function, although constrained by only two data points, exhibits a strong opposition effect rather similar to that of comet 9P/Tempel 1. The definition of the disk–integrated albedo of an irregular body having a strong opposition effect raises problems, and the various alternatives led to a R-band geometric albedo in the range 0.045–0.060, consistent with our present knowledge of cometary nuclei. The active fraction is low, not exceeding ~ 7% at perihelion, and is probably limited to one or two active regions subjected to a strong seasonal effect, a picture coherent with the asymmetric behaviour of the coma. Our slightly downward revision of the size of the nucleus of comet 67P/Churyumov-Gerasimenko resulting from the present analysis (with the correlative increase of the albedo compared to the originally assumed value of 0.04), and our best estimate of the bulk density of 370 kg m⁻³, lead to a mass of ~ 8 × 10¹² kg which should ease the landing of Philae and insure the overall success of the Rosetta mission.     

Thin film surface treatments for lowering dust adhesion on Mars Rover calibration targets

The current generation of calibration targets on Mars Rover serve as a color and radiometric reference for the panoramic camera. They consist of a transparent silicon-based polymer tinted with either color or grey-scale pigments and cast with a microscopically rough Lambertian surface for a diffuse reflectance pattern. This material has successfully withstood the harsh conditions existent on Mars. However, the inherent roughness of the Lambertian surface (relative to the particle size of the Martian airborne dust) and the tackiness of the polymer in the calibration targets has led to a serious dust accumulation problem. In this work, non-invasive thin film technology was successfully implemented in the design of future generation calibration targets leading to significant reduction of dust adhesion and capture. The new design consists of a μm-thick interfacial layer capped with a nm-thick optically transparent layer of pure metal. The combination of these two additional layers is effective in burying the relatively rough Lambertian surface while maintaining diffuse properties of the samples which is central to the correct operation as calibration targets. A set of these targets are scheduled for flight on the Mars Phoenix mission.