末制导雷达测控系统与检测接口标准化

简述了末制导雷达测控系统的发展，指出末制导雷达检测接口对测控系统的重要性。在分析现役反舰导弹末制导雷达检测接口状况以及接口信号特征的基础上，提出末制导雷达检测接口标准化思想，并给出了一种能够覆盖我海军所有现役反舰导弹末制导雷达检测接口而且可扩展的末制导雷达通用检测接口。     

基于ATE技术的末制导雷达“天线对零”实现方案

在叙述“天线对零”过程重要性的基础上,介绍了基于ATE技术的末制导雷达“天线对零”自动过程的实现方案。该自动“天线对零”方案已经应用在“末制导雷达通用检测系统”中,保证了系统的高精度自动化测量。     

一种可扩展的末制导雷达通用检测系统

介绍了采用ＩＥＥＥ－４８８总线标准实现的末制导雷达通用检测系统,概述了其硬件的组成和系统特点。并针对末制导雷达的测试规程和要求,阐述了软件系统的模块化设计思想,介绍了采用虚拟面板和虚拟仪器技术的ＡＴＥ软件设计方法。     

末制导雷达检测接口标准化初探

分析现役反舰导弹末制导雷达检测接口现状及存在问题的基础上,提出了末制导雷达检测接口标准化思想,并设计了一种能够覆盖我海军所有现役反舰导弹末制导雷达检测接口而且可扩展的末制导雷达标准检测接口。     

末制导雷达检测接口标准化初探

在分析现役反舰导弹末制导雷达检测接口现状及存在问题的基础上,提出了末制导雷达检测接口标准化思想,并设计了一种能够覆盖我海军所有现役反舰导弹末制导雷达检测接口而且可扩展的末制导雷达标准检测接口。     

专用捷变频信号源校准系统研制

捷变频末制导雷达可有效提高武器系统的抗干扰能力,但是作为其专用测试设备的捷变频信号源的计量检定问题却难以得到有效解决。通过分析现有的测试技术,使用通用仪器设备构建测试平台,可实现专用捷变频信号源的自动计量校准。系统采用两路差频形成中频频差的检测方法进行瞬时频率测量,采用单脉冲引频激励测试技术,利用通用测试仪器实现捷变频参数的校准,将捷变频计量技术推向工程应用阶段,可避免通过研制生产专用的计量设备造成其本身难以计量的问题。     

一种防空导弹制导精度影响因素的定量分析方法

主动雷达制导是先进防空导弹的主要制导方式之一。主动雷达导引头的作用距离、测角精度、时间常数等决定了末制导精度,但具体影响情况却较难量化,导致制导控制系统指标分解的合理性无法评估。本文提出了一种基于物理模型的制导精度快速评估方法,从建立主动雷达导引头指标描述的数学表征出发,采用数值评估手段,获得比例导引末制导精度影响因素的定量分析准则。数值结果表明,提出的方法可快速得到初始指向误差、导引头测角精度、探测盲距、导弹过载等对制导精度影响的定量化结果,为导弹制导控制系统指标分解提供依据。     

某雷达导引头通用自动测试设备的研制

以往的雷达自动化测试设备基本为专用测试设备,由于每一种型号的雷达的测试接口均不相同,故只能专机专用。随着装备部队的武器系统数量越来越多,性能越来越高,构成越来越复杂,部队对测试设备的自动化、标准化和通用性的要求越加迫切。阐述了雷达与测试设备之间接口的物理特性、功能特性、电气特性以及信号特征的通用要求,通过适配器、多频段VX I捷变频信号源等技术实现了测试设备自动化、标准化和通用性。     

末制导导引头定位精度的雷达误差分析

研究复合制导的战术导弹中末制导交班的导引头预定精度问题.提出用小扰动法分析导引头预定参数对误差源的误差敏感性关系.以中远程防空导弹为例,结合导弹运动方程组和目标运动模型,计算了中末制导交班的导引头预定参数,并计算了在制导站雷达测量误差下的末制导导引头预定参数的计算精度.可知,导引头定位参数的计算误差随着弹目距离的接近而显著增大,得到中末制导交班不能太晚的重要结论.     

频率微调在导弹末制导雷达自动检测系统中的实现方法

介绍了频率微调及频率调整概念及手动频率微调的方法,指出频率微调在末制导雷达性能测试中的重要性,给出了一种在自动检测系统中的自动频率微调方法.     

微型航天器的公用平台和关键技术

未来的微型航天器将采用微型公用平台——集成公用模块。文内阐述了集成公用模块的概念和应用,分别介绍了航天器实现微型化所需的关键技术——无电缆连接、多功能结构、先进的轻型材料、自主热管理的微热控系统、高密度电子线路封装和连接、集成设计环境,最后提出以集成公用模块为基础的微型航天器的设计和研制程序     

广义回归神经网络在MC-CDMA多用户检测中的应用

在简要介绍了反传(BP)神经网络,径向基神经网络(RBFN),广义回归神经网络(GRNN)的基础上,可知GRNN与传统的基于反传(BP)算法的神经网络相比,有收敛速度快,鲁棒性强等优点,本文将广义回归神经网络(GRNN)技术援引到MC-CDMA多用户检测中,进行了误码率和收敛性的仿真计算,表明了GRNN在多用户检测应用中的优越性和有效性。     

对JJG52-2013在使用中的问题探讨CSCD

一般压力表主要用于液体、气体与蒸汽的压力测量,因广泛应用使得对其开展检定工作责任重大。随着压力表检定工作的深入开展,原检定规程JJG52-1999存在一些不适应的地方,国家质量监督检验检疫总局合并了JJG52-1999、JJG573-2003两个规程,于2013年6月24日发布了新规程JJG52-2013,用于弹性元件式一般压力表、压力真空表和真空表的检定工作。用新旧比对的方法分析新版检定规程的修订内容,对JJG52-2013在使用中的问题进行探讨,并在实际应用的基础上对新版检定规程提出了具体意见及建议。     

通用ATS软件设计平台研究

通用性是当前ATS的发展方向 ,讨论了通用ATS测试软件设计平台的基本属性、软件结构 ,并重点介绍了IVI特性的基本原理。在平台内核基础上设计的TPS继承了平台内核的属性 ,具有很好的可重用性及硬件无关性。     

Southern hemisphere reference middle atmosphere

The wind part of the rocket-based empirical model of the middle atmosphere of the Southern Hemisphere is revised on the basis of new rocket and radar data. Wind and temperature values from this empirical model are compared with corresponding values from the satellite-based reference atmosphere compiled by Barnett and Corney. General similarity of the two models is confirmed, though marked discrepancies are sometimes revealed.     

Gamma Astrometric Measurement Experiment (GAME) – Implementation and performance

The GAME mission concept is aimed at testing the General Relativity, through precise measurement of the gravitational deflection of light by the Sun, by means of an optimised telescope operating in the visible and launched in orbit on a small class satellite. We describe the proposed mission profile, the preliminary payload design and the expected performance. The targeted precision on the γ parameter of the PPN formulation of General Relativity is in the range 10⁻⁶ to 10⁻⁷. The measurement principle relies on the differential astrometric signature on the stellar positions. The instrument concept is based on a dual field, multiple aperture Fizeau interferometer, observing simultaneously two sky regions close to the solar limb. A beam combiner folds the telescope line of sight on two different directions on the sky, separated by a base angle of 4°. The diluted optics approach achieves an efficient rejection of the scattered solar radiation, while retaining an acceptable angular resolution on the science targets.     

基于D-S证据理论的GPS/MM组合系统车辆定位算法

根据分段、特征提取等地图匹配关键技术探讨了地图匹配的一般原理,提出了基于D-S证据推理理论的GPS(Global Positioning System)/MM(Map Matching)组合算法,提高了GPS单点定位精度.仿真结果和跑车实验验证结果表明上述方法是行之有效的.地图匹配算法不增加系统的硬件成本,对目前广泛应用的车载GPS导航定位系统是一个有效的解决方案.      

Random walk of magnetic field lines: Subdiffusive,diffusive, and superdiffusive regimes

One- and two-dimensional models of magnetic field fluctuations and turbulence are widely used in space-, astrophysical, and laboratory contexts. In the present article we use a generalized form of the turbulence wave spectrum to calculate field line diffusion coefficients analytically and numerically. General conditions are derived for which field line wandering behaves subdiffusively, diffusively, and superdiffusively.     

Contributions from nearby pulsars to the local cosmic ray electron spectrum

PSR J0437-4715 is one of the closest millisecond pulsars (MSPs) to Earth, lying at a distance of ∼140 pc. This pulsar has a characteristic age of 4.9 Gyr and a relatively low spindown power of ∼10³⁴ ergs/s. During its rather long lifetime, a large fraction of the energy output has been in the form of multi-TeV electrons. In this paper, we investigate the possible contribution of this nearby MSP to the local interstellar electron spectrum (LIS). The old age of the system justifies a steady-state evaluation of the contribution from this pulsar to the LIS. We calculate the electron spectrum at the light cylinder in the framework of a General Relativistic polar cap (PC) model, and use this as an injection spectrum in a diffusion model. The younger Geminga pulsar is also very close to Earth and warrants investigation. A steady-state approach is however no longer justified, so we use an impulsive injection model. We will present results of a study of the contribution from these pulsars to the cosmic ray (CR) LIS. Our calculations show that pulsars like Geminga can make a non-negligible contribution to the LIS.     

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.