小波去除噪音算法研究

介绍了小波变换滤除噪音的机理和与傅立叶变换相比的优越性,其中包括确定性噪音和随机噪音。讨论了增强去噪效果的几种改进方案并提出一种试验估计去噪方法,对工程应用有一定的实用价值。     

位相物体的三维非对称温度场的重建

采用卷积背抽影公式实现了位相物体的三维非对称温度场的重建,为光线偏／折测量三维非对称温度场提供了高精度分析和处理实验数据的方法。     

Design of Interplanetary Transfers with Passive Gravity Assists and Deep Space Maneuvers

In the paper, the problem of designing interplanetary trajectories with several swing-bys and deep-space maneuvers is solved using the method of virtual trajectories developed by the authors. The algorithms for the calculation of both heliocentric and planetocentric trajectory arcs are presented, including the case of resonant trajectories. The results of applying the method of virtual trajectories to the problem of designing an interplanetary transfer to Jupiter are given and compared with the baseline trajectories for the Juno, Europa Clipper, and Laplace missions.     

客机总体方案的综合评价方法

从民用飞机的经济性、环保性、舒适性和适应性出发,运用层次分析法建立多级层次结构,形成民机总体方案的综合竞争力评价模型。给出了民机方案各性能指标的量化方法,将设计准则转化为具体的民机性能指标。引入多人评价机制,提高评价模型各层级权重分布的合理性。应用本文方法对两种大型客机总体方案进行了综合评价,结果表明该方法能明确地识别出竞争力较高的设计方案,且评价结果具有合理性。算例表明该综合评价模型可用于民机总体方案的优选。     

猎鹰9火箭Block5构型首次飞行任务解析

美国太空探索技术公司于2018年5月完成猎鹰9Block5构型火箭的首次飞行任务,研究猎鹰9Block5构型火箭的总体方案,以及为更好地实现重复使用所采取的动力系统升级、箭体结构优化和其他改进措施,回顾了猎鹰9火箭3次主要构型升级的改进方案和衍化路线,分析了此构型火箭首飞对世界航天发展的影响,提出了未来商业航天运输系统的发展建议。     

Modes of uncontrolled rotational motion of the <Emphasis Type="Italic">Progress M-29M</Emphasis> spacecraft

We have reconstructed the uncontrolled rotational motion of the Progress M-29M transport cargo spacecraft in the single-axis solar orientation mode (the so-called sunward spin) and in the mode of the gravitational orientation of a rotating satellite. The modes were implemented on April 3–7, 2016 as a part of preparation for experiments with the DAKON convection sensor onboard the Progress spacecraft. The reconstruction was performed by integral statistical techniques using the measurements of the spacecraft’s angular velocity and electric current from its solar arrays. The measurement data obtained in a certain time interval have been jointly processed using the least-squares method by integrating the equations of the spacecraft’s motion relative to the center of mass. As a result of processing, the initial conditions of motion and parameters of the mathematical model have been estimated. The motion in the sunward spin mode is the rotation of the spacecraft with an angular velocity of 2.2 deg/s about the normal to the plane of solar arrays; the normal is oriented toward the Sun or forms a small angle with this direction. The duration of the mode is several orbit passes. The reconstruction has been performed over time intervals of up to 1 h. As a result, the actual rotational motion of the spacecraft relative to the Earth–Sun direction was obtained. In the gravitational orientation mode, the spacecraft was rotated about its longitudinal axis with an angular velocity of 0.1–0.2 deg/s; the longitudinal axis executed small oscillated relative to the local vertical. The reconstruction of motion relative to the orbital coordinate system was performed in time intervals of up to 7 h using only the angularvelocity measurements. The measurements of the electric current from solar arrays were used for verification.     

A Study of the Reflection of Radio Waves from the Plasma Region on the Track behind an Axisymmetric Body Moving in the Earth’s Atmosphere

The results of numerical calculation of the dependences of the electron density, the eigenfrequency and the dielectric plasma permeability on the geometric parameters and the altitude of body motion in the near and far wake behind a thin conical body with a spherical nose blunting have been presented. The electron density maximum has been shown to be located in the region of the neck of the near wake behind the body, which determines the type of this region (supercritical or subcritical). This in turn affects the propagation of radio waves through this plasma region. A comparative analysis was performed for two different bodies with the same ballistic coefficient values. No characteristic distinctions were revealed in the values of electron density or the plasma eigenfrequency in the near and far wake behind these bodies. However, it has been shown that there are differences in the values of the distance from the bottom cross section to the neck of the near wake behind these bodies.     

Time Sequence Change-Point Model of Electrostatic State Parameters of Aircraft Engine

Electrostatic monitoring technology of particle charging information can facilitate online monitoring of aero-engine,which effectively enhances engine fault diagnosis and health managements.Unlike traditional engine state monitoring technologies,aircraft engine monitoring by gas path electrostatic monitoring not only covers the predicted information source itself,but also detects the information that can provide an early warnings for initial fault states through gas path charging levels.This paper establishes a non-stationary time sequence change-point model for anomaly recognition of electrostatic signals based on change-point theory combined with difference method of non-stationary time series.Finally,electrostatic induction data were utilized by the engine life test for a particular aircraft to validate the proposed algorithm.The results indicate that the activity level and the event rate were0.5—0.8(nc)and 50%,respectively,which were far greater than 4—12(pc)and 0—4% under normal working conditions of the engine.     

基于图和子图同构算法的制造特征识别方法

针对传统制造特征难以快速识别的难题,提出了基于图和子图同构算法的制造特征识别方法。通过提取零件模型中的几何信息与拓扑信息,构造出加权属性邻接图,对零件模型进行精准描述,为建立制造特征库,定义了文件数据的存储结构,结合子图同构算法以及相关判定规则实现对常见制造特征的识别与匹配。以Creo软件中生成的零件模型为例,在VS2010平台中进行二次开发,最后以界面窗口形式展示识别结果,验证了该方法的有效性。