带执行装置的压气机系统建模及仿真

针对压气机主动稳定控制对模型的要求,以Moore-Greitzer模型为基础,首先将模型进行空间离散化,用平均分布在压气机周向环面的离散位置点来描述流量扰动,建立了反映压气机周向动态特性的多维状态空间模型;其次以喷气装置作为主动稳定控制系统的执行装置,通过分析加入喷气装置后对流动区域产生的质量和动量影响,同时考虑气流从喷气装置出口到压气机起始平面存在的时间滞后,建立了带执行装置的压气机系统动态模型.以某压气机为例,对压气机失速行为及喷气状态下对失速的抑制作用进行仿真,结果表明:所建立的模型可以反映压气机旋转失速动态过程,通过控制喷气流量能拓展压气机的稳定工作范围,有效抑制压气机失速,模型可用于压气机主动稳定控制系统分析与设计.      

压气机叶片型面精密数控铣加工技术应用研究

为了提高压气机叶片型面和进、排气边转接圆角的数控铣加工质量,在工艺、夹具、数控加工模型与程序以及检测方法等方面采取了攻关措施,减小了叶片型面精铣加工的变形,实现了叶身型面的精密铣削加工,对型面采用毡轮修光去除铣削痕迹后,经过3坐标、小半径投影仪等设备的测量,进、排气边转接圆角的形状和型面轮廓度、位置度各项要求的加工质量得到了质的提升,其合格率由20％提高到75％以上,加工效率和刀具耐用度提高1倍以上,使叶身型面精密铣削技术具备了精品叶片批量生产的工程化应用技术基础.     

Relativistic MHD Simulations of Jets with Toroidal Magnetic Fields

This paper presents an application of the recent relativistic HLLC approximate Riemann solver by Mignone & Bodo to magnetized flows with vanishing normal component of the magnetic field. The numerical scheme is validated in two dimensions by investigating the propagation of axisymmetric jets with toroidal magnetic fields. The selected jet models show that the HLLC solver yields sharper resolution of contact and shear waves and better convergence properties over the traditional HLL approach.     

Obscured Activity: AGN, Quasars, Starbursts and ULIGs Observed by the Infrared Space Observatory

Some of the most ‘active’ galaxies in the Universe are obscured by large quantities of dust and emit a substantial fraction of their bolometric luminosity in the infrared. Observations of these infrared luminous galaxies with the Infrared Space Observatory (ISO) have provided a relatively unabsorbed view to the sources fuelling this active emission. The improved sensitivity, spatial resolution and spectroscopic capability of ISO over its predecessor Infrared Astronomical Satellite (IRAS) of enabled significant advances in the understanding of the infrared properties of active galaxies. ISO surveyed a wide range of active galaxies which, in the context of this review, includes those powered by intense bursts of star formation as well as those containing a dominant active galactic nucleus (AGN). Mid-infrared imaging resolved for the first time the dust enshrouded nuclei in many nearby galaxies, while a new era in infrared spectroscopy was opened by probing a wealth of atomic, ionic and molecular lines as well as broad band features in the mid- and far-infrared. This was particularly useful, since it resulted in the understanding of the power production, excitation and fuelling mechanisms in the nuclei of active galaxies including the intriguing but so far elusive ultraluminous infrared galaxies. Detailed studies of various classes of AGN and quasars greatly improved our understanding of the unification scenario. Far-infrared imaging and photometry revealed the presence of a new very cold dust component in galaxies and furthered our knowledge of the far-infrared properties of faint starbursts, ULIGs and quasars. We summarise almost nine years of key results based on ISO data spanning the full range of luminosity and type of active galaxies.     

Pro／Engineer中的圆角特征处理

本文从设计原理的角度结合作者的使用经验，分析了Pro／E中圆角特征的作用、构造方法及注意事项，以利于该特征在众多菜单中理清思路并正确构造圆角特征。     

Balloon altitude studies of southern hemisphere hard X-ray sources by the Imperial College-University of Tasmania-INPE collaboration

Hard X-ray balloon altitude measurements with a 1600 cm² phoswich array are described. Data from observations on Sco X-1, GX1+4, GX5−1, Nova Oph. 1977, SMC X-1, SS433, IC 4329A and MR 2251-178 are presented. The role of Comptonisation in X-ray production for Sco X-1 and GX1+4 is discussed.     

Effect of wall suction on leading edge contamination

This paper is devoted to an experimental study of swept wing leading edge contamination by the turbulence emanating from the wing-wall junction. The main objective is to delay the contamination onset by applying surface suction along the attachment line. Two series of experiments are described; the first one was performed in a small wind tunnel at CERT ONERA, the second one was carried out in the F2 wind tunnel at Le Fauga Mauzac centre. Hot film measurements showed that leading edge contamination could be delayed up to very large Reynolds numbers. We also studied the behaviour of the relaminarized boundary layer downstream of the sucked region, along the span as well as in the chordwise direction.     

The relation between the Black hole mass and the Bulge mass for low redshift AGNs. Part I: Ground-based observations

Using the bulge data from AGN image decomposition with ground-based observations, we calculate the ratios of the central supermassive black hole mass(SMBH) to the Bulge mass (_Mbh/_Mbulge$M_{\text{bh}}/M_{\text{bulge}}$) in a sample of X-ray selected AGNs, including 15 Narrow-line Seyfert 1 galaxies (NLS1s) and 18 broad-line Seyfert 1 galaxies (BLS1s). We found that the mean value of log(_Mbh/_Mbulge)$\log (M_{\text{bh}}/M_{\text{bulge}})$ is -3.81±0.11$-3.81\pm 0.11$ for 15 NLS1s, and -2.91±0.13$-2.91\pm 0.13$ for 18 BLS1s, showing the lower _Mbh/_Mbulge$M_{\text{bh}}/M_{\text{bulge}}$ in NLS1s relative to BLS1s. The calculation shows that the Bulge mass from the host image decomposition in NLS1s is statistically smaller than that from Hubble-type correction method, and a linear mass relation is suggested for NLS1s and a nonlinear mass relation for BLS1s. The studying of host galaxies with ground-based observations strongly limited by the atmospheric seeing. We need to do the decomposition of host images for NLS1s with Hubble Space Telescope observation in the future.     

雷达有源诱偏与反辐射导弹对抗仿真技术

简要分析反辐射对抗技术的发展应用情况,分析并提出了雷达有源诱偏与反辐射导弹对抗性能评估试验方法,最后介绍了一种抗反辐射导弹有源诱偏路馈半实物仿真系统研制与试验情况。     

SMART STRUCTURES USING PIEZOELEMENTS FOR ACTIVE VIBRATION AND NOISE SUPPRESSION IN AVIATION AND AEROSPACE

具有减振降噪功能的压电智能结构是智能材料与结构的一个重要分支。在航空航天领域存在一些典型结构,如飞机机舱、空间站、卫星太阳能帆板和通讯天线以及直升机旋翼等,其振动与辐射噪声造成很多不利影响。为了研究这些结构的振动与噪声控制方法,制作了几个实验模型如大型薄壁复合材料圆桶、柔性梁、钢架及旋翼系统模型,通过压电传感器、驱动器布置数量和位置的优化,采用不同的控制算法,在基于个人计算机的测控平台上进行了振动控制实验,取得了明显的减振降噪效果。