摄像机标定研究

目前,摄像机标定是计算机视觉领域中的研究热点之一,其目的是通过摄像机拍摄的单幅或多幅图像来确定摄像机的参数模型,进而获得摄像机的各项参数,在机器人导航、三维重建、生物医疗、虚拟现实、视觉监控、视觉伺服等领域均有广泛的应用前景。本文综述了传统标定方法,自标定方法和基于主动视觉的标定方法的研究现状,对其优缺点作出评价并指出发展方向。     

基于多层激励函数量子神经网络的入侵检测研究

为解决传统入侵检测模型所存在的检测效率低,对未知的入侵行为检测困难等问题,对神经网路隐层激励函数进行了研究,利用多层激励函数的量子神经网络模型进行入侵检测,该量子神经网络借鉴量子理论中量子态叠加的思想,使得隐层神经元能表示更多地状态或量级,从而很好的对入侵类型进行分类,增加隐层神经元的处理速度和检测性能法。实验表明,叠加的每个sigmoid函数较传统的sigmoid函数不仅对已知的入侵具有较好的识别能力,而且能较好的识别未知入侵行为,从而实现入侵检测的智能化。     

CFM56-5B发动机推力管理及一起故障分析

系统地阐述了CFM56-5B发动机推力管理和慢车转速控制的工作原理,并以此为基础,针对该型发动机一起常见推力控制故障的现象、原因及其排故方法进行了分析。通过此分析,进一步说明了CFM56-5B发动机慢车转速控制的基本控制逻辑,可为航空公司正确处理此类故障提供参考。     

半模机翼振动的风洞实验技术研究

飞行器机模型振动是影响其风洞实验数据可靠性的主要因素之一。为此,通过专门研制的半模振动模型,采用对称翼型NACA0012和层流翼型NACA64-210两种半模机翼进行了低速风洞振动实验。选取五种激振方式,用直接测力法得到模型在静态和不同激振方式下升力特性变化曲线,研究了振动频率、自然转捩和固定转捩、数据采集方式等参数对机翼气动特性测量结果的影响。结果表明：振动对半模机翼气动特性的影响程度因不同翼型构型、不同采集方式和翼面不同流动模式等而产生不同效果。结论对提高飞机模型风洞实验大迎角振动情况下的测量精准度有参考价值。     

含高氮化合物BTATz的CMDB推进剂特性

以新型高氮化合物3,6-双(1-氢-1,2,3,4-四唑-5-氨基)-1,2,4,5-四嗪(BTATz)取代RDX制得了BTATz-CMDB推进剂试样,获得了燃速结果,并利用TG-DTG,PDSC,单幅照相、燃烧波温度分布和熄火表面形貌及元素含量测试技术对推进剂的热分解特性及燃烧特性进行了系统研究。结果发现,BTATz的氧平衡值较低,用其取代双基推进剂中的NC和NG后,推进剂的各能量特性参量出现不同程度的降低,因此,BTATz在推进剂中的含量不宜太高。BTATz-CMDB推进剂适用于常规无溶剂成型工艺进行制造;BTATz在燃速提升方面具有突出潜力,尤其在对推进剂主放热反应催化加速的催化体系(邻苯二甲酸铅、己二酸铜和炭黑的混合物)作用下,燃速提升效果更加明显;BTATz-CMDB推进剂燃烧时的火焰符合双基系推进剂火焰的一般特征,但由于BTATz不存在类似RDX那样的熔融过程,该类推进剂燃烧产生了发散火焰束,燃烧表面由熔融状变为疏松珊瑚状,火焰强度增强;随着压强升高,燃烧表面产生发散火焰束的活性点增多,暗区迅速变薄,增加了火焰区向燃烧表面的热反馈,加速了燃烧反应;催化体系对推进剂燃烧反应的气相区影响不大,它加强了凝聚相及表面附近的放热反应,改变了推进剂燃烧表面的结构,在推进剂燃烧过程中,催化剂(新生态)在推进剂的燃烧表面富集,催化了推进剂的分解和燃烧,促进了推进剂燃速的提高。     

后缘装置LET对多段翼型气动特性的影响研究

采用求解N-S方程的方法,分别对安装后缘装置(Lift Enhancing Tabs,LET)中的传统形式Gurney襟翼(Gurney Flap,GF)和新型后缘装置(Mini-Trailing Edge Device,Mini-TED)后的多段翼型气动特性进行了分析研究。以带有30%弦长富勒襟翼的NACA632-215B两段高升力翼型为基础,分析了不同安装位置的GF对气动特性的影响。结果表明,在中等襟翼偏角下主翼尾缘安装GF对气动特性是不利的,而GF在襟翼尾缘的安装则有实际应用的可能。针对某真实飞机起飞、着陆构型多段翼型,研究了襟翼后缘不同偏角的Mini-TED对气动特性的影响。计算结果表明,通过对Mini-TED安装偏角的优化,对于不同的构型和飞行状态可以增大其改善飞机气动特性的使用范围。     

GPS共视比对数据处理软件设计

为了满足对大量GPS共视比对数据处理和分析的要求,在共视比对规范和TEC-map电离层模型的基础上,设计了GPS共视比对数据处理软件。该软件具有进一步消除单频接收机电离层时延的影响及对单通道、多通道、双频数据的单站和双站比对功能,直接平滑、内插作曲线图,并生成文件,给出平滑以后的均方差。     

广义回归神经网络在MC-CDMA多用户检测中的应用

在简要介绍了反传(BP)神经网络,径向基神经网络(RBFN),广义回归神经网络(GRNN)的基础上,可知GRNN与传统的基于反传(BP)算法的神经网络相比,有收敛速度快,鲁棒性强等优点,本文将广义回归神经网络(GRNN)技术援引到MC-CDMA多用户检测中,进行了误码率和收敛性的仿真计算,表明了GRNN在多用户检测应用中的优越性和有效性。     

Sq(H) field variations at Sonmiani geomagnetic observatory,Pakistan for solar cycle 24

In this study, Sq(H) field results for Sonmiani geomagnetic observatory (SON), Pakistan are presented first time for solar cycle i.e., Solar Cycle 24. Sonmiani observatory was established in 2008 and was included in the list of INTERMAGNET Magnetic Observatory (IMO) in 2012. The analysis of Sq(H) field is performed to examine diurnal, annual and seasonal behaviour of Sq(H) field at Sonmiani along with Honolulu which is used as reference observatory. Both the observatories lie at the Equatorial Ionisation Anomaly (EIA) crest. In general strong dependency of Sq(H) field on solar cycle has been observed. First peak of SC24 was visible in Sq(H) field at both observatories. However, at HON maximum Sq(H) was observed in 2015 instead of 2014, a year later than the year of solar maximum. Prominent longitudinal difference has been noted between both observatories. At HON, maximum Sq(H) was observed during equinox while at SON it was noted during equinox and summer as a consequence of shift in latitude of Sq focus. Phase shift of Sq(H) at SON followed a general trend, that is maximum Sq(H) shifted to later hours in solar maximum as compared to solar minimum. Whereas, an opposite trend was noted at HON which might be due to coastal effect. In case of seasonal phase shift, at both observatories maximum Sq(H) occurred at later hours in summer than in winter which is opposite to the results obtained by many workers. These points need further investigation and geomagnetic as well as wind, and electric field data of other observatories situated at the EIA crest region is required to interpret the Sq(H) phase shift extensively.     

Encounter trajectories for deep space mission ASTER to the triple near Earth asteroid 2001-SN263. The laser altimeter (ALR) point of view

In cooperation with Russia, the Brazilian deep space mission ASTER plans to send a small spacecraft to investigate the triple asteroid 2001-SN263. The nearest launch opportunities for this project include June 2022 and June 2025. One main exploration campaign is being planned with focus on the largest asteroid (Alpha). Among the instruments under development, a laser altimeter (named ALR) was preliminarily designed and presented in 2010–2011. Many studies to define mission and instruments requirements were performed aiming at the characterization of important issues for the successful realization of the mission. Among them, the identification of a suitable trajectory that could be followed by the ASTER spacecraft in the encounter phase, when the main campaign will take place. This paper describes the effort undertaken with focus on the laser altimeter operation. Possible encounter trajectories were modelled and simulated to identify suitable approach parameters and conditions allowing the accomplishment of the intended investigation. The simulation also involves the instrument operation, considering approach geometry, attitude, relative motion, time/date, and the dynamics of the main asteroid. From the laser altimeter point of view, keeping in mind the desired coverage results (50% minimum surface coverage of asteroid Alpha, complying with horizontal and vertical resolution requirements), results point out crucial features for the encounter trajectory, like the need for a small inclination (10^-6 degrees; with respect to the asteroid's orbit), the most favourable spacecraft positioning (between the Sun and the asteroid) and pointing condition (back to the Sun), the minimum amount of achievable surface coverage (58%, focused on central areas), and the most proper time to conduct the main campaign (January 2025). Concerning the instrument, results offer refined values for divergence angle (500 to 650 μrad, half-cone), pulse repetition frequencies (from 1/20 to 1 Hz), and consequent data generation rates. A simulation tool that can use any 3D generated trajectories as input data was created for the analyses presented here. Although created for the ALR in this mission, this simple analysis tool can be adapted to other instruments in this or other missions.