结构非线性对颤振特性的影响

基于描述函数法，对操纵系统的结构非线性问题，提出了用于描述函数法的耦合模态和非耦合的综合计算模型，使用跨音速非定常空气动力，对扑动间隙和旋转间隙进行研究，揭示了全动水平尾翼振动的根源主要是操纵间隙造成的，为其它同类问题提供了可行的工程分析方法。     

Numerical simulations of the radiance from the comet 46P/Wirtanen in the various configurations of the measurements during “Rosetta” mission

The work we present deals with the spectrometric measurements of VIRTIS instrument of the Comet P/Wirtanen planned for the Rosetta mission. This spectrometer can monitor (VIRTIS M channel: 0.250μm – 0.980μm; Δκ=20cm⁻¹; 0.980 – 5.0 μm; Δκ = 5cm⁻¹; VIRTIS H channel: 2.0 μm – 5.0 μm; Δκ=2cm⁻¹) the nucleus and the coma in order to provide a general picture of coma's composition, the production of gas and dust, the relationship of coma production to surface composition and the structure and variation of mineralogy of the nucleus surface. During the mission the observation conditions of the spectroscopic investigation change due to different relative positions spacecraft/comet, and to the different illumination conditions of the surface at various distances of the comet to the Sun. The nucleus surface is continuously modified by the ice sublimation accompanied by gas and dust emission. Consequently the surface also its spectrophotometric properties changes and their monitoring can give a new insight. The important role of simulations is to predict the results of measurements in various experimental condition what, in the future, can help in interpretation of the measured data.

In this paper the first results of our simulation the radiance from the comet in the 0.25–5.0μm spectral range at two distances from the Sun (1AU and 3AU) are shown. The distance between the Rosetta orbiter and the nucleus surface as well as the sun zenith angles are taken into account according to the Rosetta mission phases. In fact the surface and coma properties vary along the comet orbit, and should be taken into account in our calculations. The optical parameters of the dust on the surface (e.g. reflectance) and in the coma (e.g. Q_ext) were calculated from optical constants of possible comet analogues. The thermodynamic parameters of the comet are taken from the models of comet evolution. Through this kind of modelling it is possible to identify the surface characteristics in spectra of the radiation from the surface of nucleus transmitted through the coma loaded with dust and gases.

Even if the “Rosetta mission” is postponed, with the consequence of a target change, we think that our idea and the method used for the simulations can be useful also for the new Rosetta target - the comet 67P/Churyumov Gerasimenko.     

动目标双站RCS预估的图形电磁计算（GRECO）方法

图形电磁计算 (GRECO)技术是目前分析高频区复杂目标雷达散射截面 (RCS)最有效方法之一。通过应用 GRECO方法和单 -双站等效原理 ,计算动目标高频区的双站 RCS,给出了与实验结果符合良好的计算实例 ,具有很好的工程应用价值     

航空结构件铣削残余应力分布规律的研究

 采用三维有限元方法,模拟计算航空铝合金7050-T7451 材料在无内应力前提下数控铣削时产生的表层残余应力场。在综合考虑了现行的常规工艺方案基础上,从中选定4 种具有代表性的走刀路径分别进行分析计算,进而优选出最为合适的走刀工艺规则。走刀过程采用动态载荷步模拟,材料去除采用生死单元模拟,从而使计算结果更加精确、可信。通过本文的研究工作,可为提高该类材料数控铣削加工的尺寸稳定性确定合理的工艺策略。     

Solar flares as sources of energetic particles

In this paper a review is presented of the present status of our knowledge of solar flare phenomena with special emphasis on the production of suprathermal particles and their solar effects. Of these energetic particles electrons play an important role since they produce the X-ray and radiobursts observed during many flares. Also, during their slowing down to thermal energies they contribute to the heating of localized regions in the solar atmosphere, through energy exchange with the ambient electrons. Observable radiations of energetic protons, and other nuclei, are produced through nuclear interactions leading to the emissions of gamma-ray lines. Detectable fluxes of these gamma-ray lines are produced only in the most powerful flares. Also the nuclei that enter into deeper layers of the solar atmosphere transfer most of their kinetic energy to the ambient plasma.     

The evolution of massive stars

The evolution of stars with masses between 15 M ₀ and 100M ₀ is considered. Stars in this mass range lose a considerable fraction of their matter during their evolution.The treatment of convection, semi-convection and the influence of mass loss by stellar winds at different evolutionary phases are analysed as well as the adopted opacities.Evolutionary sequences computed by various groups are examined and compared with observations, and the advanced evolution of a 15M ₀ and a 25M ₀ star from zero-age main sequence (ZAMS) through iron collapse is discussed.The effect of centrifugal forces on stellar wind mass loss and the influence of rotation on evolutionary models is examined. As a consequence of the outflow of matter deeper layers show up and when the mass loss rates are large enough layers with changed composition, due to interior nuclear reactions, appear on the surface.The evolution of massive close binaries as well during the phase of mass loss by stellar wind as during the mass exchange and mass loss phase due to Roche lobe overflow is treated in detail, and the value of the parameters governing mass and angular momentum losses are discussed.The problem of the Wolf-Rayet stars, their origin and the possibilities of their production either as single stars or as massive binaries is examined.Finally, the origin of X-ray binaries is discussed and the scenario for the formation of these objects (starting from massive ZAMS close binaries, through Wolf-Rayet binaries leading to OB-stars with a compact companion after a supernova explosion) is reviewed and completed, including stellar wind mass loss.     

基于最优估计神经网络的惯导系统初始对准研究

本文研究了一种基于卡尔曼滤波原理权值更新的多层神经网络学习算法，对此算法进行了详细的推证，并将该算法运用到惯导系统的初始对准过程。仿真结果表明了这种神经网络结构用于惯导系统初始对准问题的有效性，既可获得与卡尔曼滤波器相同的对准精度，又提高了系统的实时性。从而得到了利用神经网络解决惯导系统初始对准问题的一种有效算法。     

考虑星-箭动力耦合作用结构瞬态响应分析

利用直接激励法，对火箭发射过程中考虑星箭动力耦合作用的卫星结构瞬态响应问题进行了求解。给出了最大动压、一二级分离前和分离后三种工况下卫星结构的加速度响应历程。该方法克服了大质量法和惯性载荷法瞬态响应计算中的载荷处理困难和数据回归困难。文中给出了大质量法、直接激励法和惯性载荷法的动力学方程，指出各种方法的应用条件。计算结果表明，直接激励法简捷实用，优于惯性载荷法和大质量法。     

遥感卫星自截断SPIHT压缩译码技术

链表式SPIHT算法是目前公认最好的压缩方案,但是由于其传输中具有极差的抗误码特性,在遥感图像数据压缩中的应用具有一定局限性。本文提出的自截断式SPIHT压缩算法使得译码器在出现“致使性”误码的情况下能够自动中止该帧数据流译码,使得误码不至于扩散到整幅图像之中。为SPIHT算法在遥感图像数据压缩中的应用提供了理论依据。