基于通用微机的雷达终端系统设计

雷达终端是雷达系统的核心组成部分,有必要采用当前先进的软硬件技术来设计.考虑到雷达终端发展现状,着重分析了雷达的功能要求和系统中的信息流,构建了基于通用微机的模块化、软件化的雷达终端系统,并详细讨论了系统的结构及硬件和软件的设计.系统由通用微机和雷达信号处理板sD754lA来实现,在运行过程中稳定可靠,满足雷达信号数据实时处理和显示的需求.     

二次通用旋转组合设计试验在造粒技术领域的应用研究

本文研究了利用二次通用旋转组合设计来进行多因素影响的振动流化床喷雾造粒试验,建立数学模型,得出了具有一定参数价值的最佳操作参数。     

主被动传感器UT-DC目标定位算法

主被动传感器融合定位具有高度非线性,针对采用传统的线性化方法计算变量统计特性,理论定位结果与实际定位结果相差较大的情况,文章提出了基于不敏变换(UT)的数据压缩(DC)融合定位算法。首先,通过不敏变换精确计算了二维变量的统计特性,减小了非线性误差的影响;其次,针对数据压缩过程中量测信息重复利用的问题进行去相关性处理,获得较高的定位精度;最后,通过理论分析和仿真结果验证,相较于传统的线性化处理方式相差较大的情况,基于不敏变换的数据压缩融合定位方法理论结果与实际结果相吻合。     

提升通用飞机气动效率的设计策略研究

针对目前通用飞机借鉴大中型运输类飞机常规设计方法造成的气动效率较低、经济性较差的现状,分析通用飞机相对于其他飞机所具有的不同的设计特点;从空气动力学基本原理出发,结合通用飞机的特点,推导并分析其气动效率低下主要是由两个方面的矛盾耦合所造成的;提出可以有效改善通用飞机气动效率的设计策略;通过通用飞机总体参数设计优化实例印证新设计策略的有效性。结果表明:新设计策略可有效改善通用飞机的气动性能,提高其经济性,但相关研究具有较大的挑战性。     

基于超光滑表面工艺过程的PSD评价技术研究

基于功率谱密度简化公式,通过数据拟合提取出PSD曲线的两个重要评价参数.研究PSD曲线变化与超光滑表面加工工艺相关性,提出基于超光滑表面工艺过程的PSD评价技术,以指导工艺改进和新工艺的开发.     

X-ray redshifts with the International X-ray Observatory (IXO)

We explore the capabilities of the future space science mission IXO (International X-ray Observatory) for obtaining cosmological redshifts of distant Active Galactic Nuclei (AGNs) using the X-ray data only. We first find in which regions of the X-ray luminosity (L_X) versus redshift (z) plane the weak but ubiquitous Fe Kα narrow emission line can deliver an accurate redshift (δz < 5%) as a function of exposure time, using a CCD-based Wide Field Imager (IXO/WFI) as the one baselined for IXO. Down to a 2–10 keV X-ray flux of 10⁻¹⁴ erg cm⁻² s⁻¹ IXO/WFI exposures of 100 ks, 300 ks and 1 Ms will deliver 20%, 40% and 60% of the redshifts. This means that in a typical 18′ × 18′ IXO/WFI field of view, 4, 10 and 25 redshifts will be obtained for free from the X-ray data alone, spanning a wide range up to z ∼ 2–3 and fairly sampling the real distribution. Measuring redshifts of fainter sources will indeed need spectroscopy at other wavebands.     

载人航天器发射场总装测试厂房设计需求分析研究

文章依据航天器技术指标和工作内容,提出载人航天器发射场总装测试厂房的设计需求分析方法,列出设计需求要素,包括厂房建筑规模需求,厂房支持能力需求、厂房保障条件需求等.分别阐述各需求要素的作用、计算方法以及需要依照的建筑设计规范,给出了设计需求指标确定方法.     

提高人文水平 加强素质教育

素质教育提倡科学教育与人文教育整合，以培养高素质的科技人才。而目前，我国的大学英语教学又是以理工科学生为主要对象。在这种情况下，在英语教学中加强人文教育有重要的意义。     

Cassini Radio Science

Cassini radio science investigations will be conducted both during the cruise (gravitational wave and conjunction experiments) and the Saturnian tour of the mission (atmospheric and ionospheric occultations, ring occultations, determinations of masses and gravity fields). New technologies in the construction of the instrument, which consists of a portion on-board the spacecraft and another portion on the ground, including the use of the Ka-band signal in addition to that of the S- and X-bands, open opportunities for important discoveries in each of the above scientific areas, due to increased accuracy, resolution, sensitivity, and dynamic range.This revised version was published online in July 2005 with a corrected cover date.     

Gamma astrometric measurement experiment (GAME) – Science case

We report here on the science case of a concept for a satellite orbiting at 1 AU from the Sun and using a baffled Fizeau interferometer to look as close as possible to its limb. This configuration, and the need for looking nearby the Sun, is required for the main scientific driver of the mission, namely the measure of the γ parameter of the Parameterized Post-Newtonian formulation to the 10⁻⁶–10⁻⁷ level at least. This would lead to an accurate test of the General Theory of Relativity against other alternative theories of gravity, and set stringent constraints on some of the most significant issues of Astrophysics like those involving exotic forms of dark matter and dark energy. Exploiting the possibilities offered by the observation strategy, it is also possible to target other interesting scientific goals. One is, again, in the realm of General Relativity and aims at measuring the light deflection nearby the Giant Planets to detect asymmetric effects induced by their quadrupoles, predicted by GR but never measured so far. Others can be found in the observation of selected extrasolar systems where, e.g., the astrometric and photometric capabilities of GAME will help to improve on the knowledge of the brown-dwarf regime and on the search for exo-planets with the transit method, respectively.