对数零相位谱在雷达目标识别中的应用研究

高分辨距离像的频谱相位包含了大部分目标信息,对数零相位谱特征能够保留这些信息,且具有平移不变性。提出一种对数零相位谱最小距离雷达目标识别方法,并利用外场实测数据计算仿真,比较了最小欧氏距离与最小马氏距离准则下对数零相位谱的识别性能,同时与功率谱、幅度谱做对比,验证了该方法的可行性与有效性。     

Off-axis irradiation and the polarization of broad emission lines in active galactic nuclei

The stokes Monte Carlo radiative transfer code has been extended to model the velocity dependence of the polarization of emission lines. We use stokes to present improved modeling of the velocity-dependent polarization of broad emission lines in active galactic nuclei. We confirm that off-axis continuum emission can produce observed velocity dependencies of both the degree and position angle of polarization. The characteristic features are a dip in the percentage polarization and an S-shaped swing in the position angle of the polarization across the line profile. Some differences between our stokes results and previous modeling of polarization due to off-axis emission are noted. In particular we find that the presence of an offset between the maximum in line flux and the dip in the percentage of polarization or the central velocity of the swing in position angle does not necessarily imply that the scattering material is moving radially. Our model is an alternative scenario to the equatorial scattering disk described by Smith et al. (2005). We discuss strategies to discriminate between both interpretations and to constrain their relative contributions to the observed velocity-resolved line and polarization.     

On the Lyman α and O VI Line Profiles in Streamers and Coronal Holes

The profiles of the Lyα line at 1215.6 Å and of the O VI doublet at 1031.9 Å and 1037.6 Å in the extended solar corona have been analyzed vs. latitude and radial direction, performing observations with the Ultraviolet Coronagraph Spectrometer (UVCS) on board the ESA-NASA solar satellite SOHO (Solar and Heliospheric Observatory). The results show that these lines behave differently with latitude: the H I Ly α line has larger full width at half maximum (FWHM) values in the streamer region and narrower values towards the pole, while the FWHM of O VI lines has a minimum at the center of the streamer and slightly increases towards the polar regions. We briefly discuss the impact of the results on coronal heating theories.     

蒸发式Z形值班火焰稳定器的点火性能

针对一种蒸发式Z形值班火焰稳定器进行了点火性能试验研究,采用高速摄影和图像处理的方法获得了不同点火位置下初始火核的生成及发展过程,并对回流区油雾分布及时均火焰结构进行分析。试验结果表明:相比传统薄膜蒸发式火焰稳定器,蒸发式Z形火焰稳定器的贫油点熄火当量比在马赫数超02时能降低311%和194%。Z形值班火焰稳定器具有双燃烧反应区特征,点火位置影响初始火核的形成,当第二反应区对火核生成起主导作用时值班火焰稳定器的点火性能较好、火核发展较快。点火位置位于Z形槽下拐角附近时能获得较好的点火性能,而靠近回流区与主流交界面时点火性能较差;同时低温高速条件下低燃油蒸发率导致的燃油分布不均会带来点火性能的展向差异。     

Testing the no-hair theorem with observations of black holes in the electromagnetic spectrum

According to the no-hair theorem, astrophysical black holes are uniquely described by their mass and spin. In this paper, we review a new framework for testing the no-hair hypothesis with observations in the electromagnetic spectrum. The approach is formulated in terms of a Kerr-like spacetime containing a quadrupole moment that is independent of both mass and spin. If the no-hair theorem is correct, then any deviation from the Kerr metric quadrupole has to be zero. We show how upcoming VLBI imaging observations of Sgr A∗ as well as spectroscopic observations of iron lines from accreting black holes with IXO may lead to the first astrophysical test of the no-hair theorem.     

Variation of Polar Coronal Hole Profiles with Solar Cycle

We compared the H I Lyα polar coronal hole profiles obtained during the three Spartan 201 flights (in 1993, 1994, and 1995) and during the more recent UVCS/SOHO mission. We found that at 2.1 R_⊙ there are no significant variations of the line shape over the several years of the descending phase of the solar cycle. However, there may be some evidence for the 1.8 R_⊙ profiles being broader towards solar minimum. The profiles at 2.1 R_⊙ are different from profiles obtained at 1.8 R_⊙; they have clearly narrower cores and wide wings. We fitted the profiles with single and/or multiple Gaussian functions and calculated their typical 1/e half widths. This revised version was published online in June 2006 with corrections to the Cover Date.     

Integrated Entry Guidance for Reusable Launch Vehicle

A method for the implementation of integrated three-degree-of-freedom constrained entry guidance for reusable launch vehicle is presented. Given any feasible entry conditions, terminal area energy management interface conditions, and the reference trajectory generated onboard then, the method can generate a longitudinal guidance profile rapidly, featuring linear quadratic regular method and a proportional-integral-derivative tracking law with time-varying gains, which satisfies all the entry corridor constraints and meets the requirements with high precision. Afterwards, by utilizing special features of crossrange parameter, establishing bank-reversal corridor, and determining bank-reversals according to dynamically adjusted method, the algorithm enables the lateral entry guidance system to fly a wide range of missions and provides reliable and good performance in the presence of significant aerodynamic modeling uncertainty. Fast trajectory guidance profiles and simulations with a reusable launch vehicle model for various missions and aerodynamic uncertain-ties are presented to demonstrate the capacity and reliability of this method.     

智能型减压器试验台的研制

主要介绍了基于硬件设备和软件编程基础上的智能型减压器试验台的设计与应用。测试系统保留了最通常的手动操作系统，增加了全新的自动数据采集系统。试验台可精确、同步测量高入口压力值时的瞬时出口压力值，同时，增加了入口压力控制系统，大大提高了工作效率。     

弹道导弹动态全极化一维像仿真研究

研究了弹道导弹动态全极化一维像的仿真方法,可以为雷达目标检测、识别算法的研究提供基础。对弹道导弹的弹道和运动特性进行了建模,通过对弹头缩比模型静态测量数据进行插值,可以获得任意时刻、任意姿态下弹头的全极化一维距离像;比较了典型宽带雷达体制的信号形式,推导了它们之间的仿真参数转换关系。在计算机上进行了仿真实验,对仿真结果的分析表明本文提出的仿真方法是切实可行的。     

Comparison of the CHAMP radio occultation data with the Canadian advanced digital ionosonde in the Polar Regions

In this paper we present the results of the comparison of the retrieved electron density profiles of the Ionospheric Radio Occultation (IRO) experiment on board CHAMP (CHAllenging Minisatellite Payload), with the ground ionosonde profiles for the Polar Regions. IRO retrieved electron density profiles from CHAMP are compared with Canadian Advanced Digital Ionosonde (CADI) measurements at two vertical sounding stations well within the Polar Cap, Eureka (geog. 80°13′ N; 86°11′ W) and Resolute Bay (geog. 74°41′ N; 94°54′ W). We compared the ionospheric parameters such as the peak electron density of the F-layer (NmF₂) and the peak height of the F-layer (h_mF₂) for a 3-year period, 2004–2006. CHAMP derived NmF₂ shows reasonable agreement with the ionosonde retrieved NmF₂ for both the stations (0.76 and 0.71 correlation coefficient, for Eureka and Resolute Bay, respectively) whereas the h_mF₂ agreement is not that acceptable (0.25 and 0.37 correlation coefficient, respectively). The h_mF₂ from vertical sounding showed less spread than the CHAMP h_mF₂.