基于STF和加权改进的群目标跟踪算法

为了进一步提高群目标交互多模型跟踪算法的估计性能,提出一种改进的群跟踪算法.首先,通过采用模型转换概率的自适应算法,优化模型与目标运动模式的实时匹配.并通过引入强跟踪滤波（STF,Strong Tracking Filter）中的渐消因子,提高机动阶段时的群质心的状态估计精度.其次,分别利用概率加权法和标量加权法完成群质心状态和扩展状态的融合估计.最后在变分贝叶斯滤波的基础上,建立完整的跟踪算法流程.仿真实验结果表明,该方法不仅能够提高群质心状态和扩展状态的估计精度,还能有效降低机动阶段时的峰值误差.     

面向数字化技术支援的数字样机逐层轻量化技术

直观的三维模型有助于提高民用飞机远程维修支援的效率和准确度,但由于计算机辅助设计系统产生的模型数据量通常比较巨大,三维数字样机的轻量化成为了很大的挑战.基于对格式转换与模型简化这两种轻量化方法的分析,提出了基于单元数据量的数字样机逐级轻量化的方法,将全机的三维模型进行不同简化程度的轻量化处理,并且提出了基于失真度判据的层级化管理方法,按照模型结构树对简化率高的失真模型与具有细节特征的无损模型进行逐级的加载与使用.实例验证表明所提出的方法有效减小了网络传输的数据量并保留了模型必要的细节特征,使在互联网中快速访问全机三维模型得以实现.     

Scientific objectives and payloads of Tianwen-1, China’s first Mars exploration mission

This paper describes the scientific objectives and payloads of Tianwen-1, China’s first exploration mission to Mars. An orbiter, carrying a lander and a rover, lifted-off in July 2020 for a journey to Mars where it should arrive in February 2021. A suite of 13 scientific payloads, for in-situ and remote sensing, autonomously commanded by integrated payload controllers and mounted on the orbiter and the rover will study the magnetosphere and ionosphere of Mars and the relation with the solar wind, the atmosphere, surface and subsurface of the planet, looking at the topography, composition and structure and in particular for subsurface ice. The mission will also investigate Mars climate history. It is expected that Tianwen-1 will contribute significantly to advance our scientific knowledge of Mars.     

零售服务质量中的人力资源管理(英文)

本文研究了人力资源管理与服务质量的关系。透过问卷调查及数据分析,确立人力资源的重点、结构与相互关系,促进服务质量。研究选择了零售服务为试点,给管理人员提供了一个更直接、更清晰的指引,发挥人力资源本身的素质。研究结果把希士杰等质量大师在美国哈佛商报中提出的“服务利润连接（Ｓｅｒｖｉｃｅｐｒｏｆｉｔｃｈａｉｎ）”具体化,使管理人员可以直接在企业内运用。     

幂律过程拟合优度检验的功效比较

幂律过程常被用于描述复杂系统的可靠性增长模型和可修系统的可靠性分析。本文考虑定数截尾场合幂律过程的７种拟合优度检验统计量,在备选假设为对数幂律过程时,比较了这７种检验法的功效。大量随机模拟计算表明,当ｒ在较宽的范围内,Ｆ检验法的功效比其余６种检验法都要高。     

平面激光诱导荧光显示火焰中OH的分布图像

用平面激光诱导荧光技术测量了平面火焰炉、原子气化炉和超声速燃烧室的单脉冲激光诱导OH荧光。由平面荧光图可得到氢氧基相对浓度分布和它的厚度。由超声速燃烧室的OH荧光测量 ,可以看出不同时间OH分布的差别。氢氧基的PLIF图像是研究火焰结构和流场的有力工具。     

基于时频图像形态学的雷达信号IF估计

针对低信噪比下雷达信号的IF估计,提出一种将时频分析和图像处理相结合的估计方法.首先通过时频变换将一维信号转化为二维时频图像;然后采用形态学方法去除时频图像上的噪声点和毛刺,并将其骨骼化;最后采用图像处理中标注连接分量的方法,区分出不同分量的雷达信号以及噪声分量,并通过统计信号分量的行索引和列索引估计出信号的IF.对SFM、LFM和FSK信号的IF估计进行了仿真分析,实验结果表明该方法能够在较低信噪比下有效地估计出信号的IF,同时也适用于多分量信号.     

Generalized Kutta–Joukowski theorem for multi-vortex and multi-airfoil flow with vortex production——A general model

By using a special momentum approach and with the help of interchange between singularity velocity and induced flow velocity, we derive in a physical way explicit force formulas for twodimensional inviscid flow involving multiple bound and free vortices, multiple airfoils, and vortex production. These force formulas hold individually for each airfoil thus allowing for force decomposition, and the contributions to forces from singularities(such as bound and image vortices,sources, and doublets) and bodies out of an airfoil are related to their induced velocities at the locations of singularities inside this airfoil. The force contribution due to vortex production is related to the vortex production rate and the distance between each pair of vortices in production, thus frameindependent. The formulas are validated against a number of standard problems. These force formulas, which generalize the classic Kutta–Joukowski theorem(for a single bound vortex) and the recent generalized Lagally theorem(for problems without a bound vortex and vortex production) to more general cases, can be used to identify or understand the roles of outside vortices and bodies on the forces of the actual body, optimize arrangement of outside vortices and bodies for force enhancement or reduction, and derive analytical force formulas once the flow field is given or known.     

Comparison of ionospheric F2 peak parameters foF2 and hmF2 with IRI2001 at Hainan

Monthly median values of foF2, hmF2 and M(3000)F2 parameters, with quarter-hourly time interval resolution for the diurnal variation, obtained with DPS4 digisonde at Hainan (19.5°N, 109.1°E; Geomagnetic coordinates: 178.95°E, 8.1°N) are used to investigate the low-latitude ionospheric variations and comparisons with the International Reference Ionosphere (IRI) model predictions. The data used for the present study covers the period from February 2002 to April 2007, which is characterized by a wide range of solar activity, ranging from high solar activity (2002) to low solar activity (2007). The results show that (1) Generally, IRI predictions follow well the diurnal and seasonal variation patterns of the experimental values of foF2, especially in the summer of 2002. However, there are systematic deviation between experimental values and IRI predictions with either CCIR or URSI coefficients. Generally IRI model greatly underestimate the values of foF2 from about noon to sunrise of next day, especially in the afternoon, and slightly overestimate them from sunrise to about noon. It seems that there are bigger deviations between IRI Model predictions and the experimental observations for the moderate solar activity. (2) Generally the IRI-predicted hmF2 values using CCIR M(3000)F2 option shows a poor agreement with the experimental results, but there is a relatively good agreement in summer at low solar activity. The deviation between the IRI-predicted hmF2 using CCIR M(3000)F2 and observed hmF2 is bigger from noon to sunset and around sunrise especially at high solar activity. The occurrence time of hmF2 peak (about 1200 LT) of the IRI model predictions is earlier than that of observations (around 1500 LT). The agreement between the IRI hmF2 obtained with the measured M(3000)F2 and the observed hmF2 is very good except that IRI overestimates slightly hmF2 in the daytime in summer at high solar activity and underestimates it in the nighttime with lower values near sunrise at low solar activity.     

Cluster observations showing the indication of the formation of a modified-two-stream instability in the geomagnetic tail

This study presents several observations of the Cluster spacecraft on September 24, 2003 around 15:10 UT, which show necessary prerequisites and consequences for the formation of the so-called modified-two-stream instability (MTSI). Theoretical studies suggest that the plasma is MTSI unstable if (1) a relative drift of electrons and ions is present, which exceeds the Alfvèn speed, and (2) this relative drift or current is in the cross-field direction. As consequences of the formation of a MTSI one expects to observe (1) a field-aligned electron beam, (2) heating of the plasma, and (3) an enhancement in the B-wave spectrum at frequencies in the range of the lower-hybrid-frequency (LHF). In this study we use prime parameter data of the CIS and PEACE instruments onboard the Cluster spacecraft to verify the drift velocities of ions and electrons, FGM data to calculate the expected LHF and Alfvèn velocity, and the direction of the current. The B-wave spectrum is recorded by the STAFF instrument of Cluster. Finally, a field aligned beam of electrons is observed by 3D measurements of the IES instrument of the RAPID unit. Observations are verified using a theoretical model showing the build-up of a MTSI under the given circumstances.