RS码的时域编码频域译码技术

通过对于RS码的时域编码／频域译码的算法进行分析,找到了它们的不同之处及转换方法,得出了时域编码／频域译码的混合编译码方法,提高了运算速度和纠错能力。     

编辑意识的内涵及培育

编辑意识是科技期刊编辑应当遵从的基本原则,主要包括职业意识、学习意识、法律意识、规范意识、伦理意识、服务意识、大局意识等。编辑应当在日常的编辑工作中,认真磨砺和养成这些良好的思想意识,并伴随着时代的发展和科学的进步,不断创新,与时俱进。     

小卫星临近作业轨道和姿态联合控制

建立了小卫星相对轨道和姿态的误差动力学模型,根据作业任务和姿态指向要求确定了小卫星相对轨道和姿态的期望运动;采用相对轨道和姿态联合控制策略,并考虑小卫星作业过程中质量和转动惯量的不确定性,设计了自适应全状态反馈控制律;数值仿真结果表明该控制律具有较强的自适应性。     

一种基于FFT的Galileo搜救信号频域检测方法

Galileo搜救系统是全球卫星搜救组织(COSPAS-SARSAT)的一部分,搭载于Galileo导航星座,能对遇险用户发出的求救信号进行定位并实施救援。经卫星转发的搜救信号信噪比很低,能否在低信噪比条件下完成卫星信号的检测对搜救系统的正常工作至关重要。为了解决这一问题,文章提出了一种基于快速傅里叶变换(FFT)运算的频域检测方法,通过理论分析和仿真验证可以看出,这种方法能有效地实现低信噪比条件下的卫星下行信号检测。     

职业院校学生异性交往问题与策略研究——以航海专业男生班为例

以航海专业男生班为实例,从人性角度,运用心理学方法,着重分析其缺少异性交往所出现的问题,探讨引导航海专业男生在异性交往中健康成长的方法与途径,给学校教育管理者在正确对待和引导学生异性交往,提高科学化、人性化教育管理水平方面提供一定的参考。     

小型热真空试验设备网络化集群测控技术

随着航天器部组件试验任务的日益增多,在人员少的情况下,高效率地完成型号任务的需求十分迫切。文章介绍了小型热真空试验设备网络化集群测控的方法与技术,以某小型热真空试验设备群为例,针对其接口复杂、数据量大、地理位置分散且要求集中管理的特点,详细阐述了采用混合B/S模式与C/S模式的网络化测控技术来实现小型热真空试验设备群集群测控的功能。该技术已在小型热真空试验设备的集群控制中得到了成功的应用。     

电子战对导弹防空系统性能影响的评估

在电子战对导弹防空系统性能影响的研究过程中,运用信息作战原理,构造基于概率的导弹防空系统性能评估模型,通过信息与火力分析平台获取电子战影响的仿真数据,对舰载导弹防空系统的信息与火力联合打击能力进行评估,初步的评估结果表明:信息和火力对打击能力的影响分别为61%和39%,信息因素比火力因素更为重要.     

新型带垫卡箍的研究

卡箍在飞机上的应用较为广泛,卡箍的质量问题也会影响飞行的安全.新型带垫卡箍结构形式优异、减震性能好,且橡胶垫片性能好、耐老化、耐燃烧,有效解决了现在军用飞机上带垫的夹紧卡箍橡胶垫片老化严重、减震性能差、拆卸、使用和维护不方便的问题,满足了军机的使用需求.     

HIRDES – The High-Resolution Double-Echelle Spectrograph for the World Space Observatory Ultraviolet (WSO/UV)

The World Space Observatory Ultraviolet (WSO/UV) is a multi-national project grown out of the needs of the astronomical community to have future access to the UV range. WSO/UV consists of a single UV telescope with a primary mirror of 1.7 m diameter feeding the UV spectrometer and UV imagers. The spectrometer comprises three different spectrographs, two high-resolution echelle spectrographs (the High-Resolution Double-Echelle Spectrograph, HIRDES) and a low-dispersion long-slit instrument. Within HIRDES the 102–310 nm spectral band is split to feed two echelle spectrographs covering the UV range 174–310 nm and the vacuum-UV range 102–176 nm with high spectral resolution (R > 50,000). The technical concept is based on the heritage of two previous ORFEUS SPAS missions. The phase-B1 development activities are described in this paper considering performance aspects, design drivers, related trade-offs (mechanical concepts, material selection etc.) and a critical functional and environmental test verification approach. The current state of other WSO/UV scientific instruments (imagers) is also described.     

Analytical approach to cosmic ray ionization by nuclei with charge Z in the middle atmosphere – Distribution of galactic CR effects

The effects of galactic and solar cosmic rays (CR) in the middle atmosphere are considered in this work. A new analytical approach for CR ionization by protons and nuclei with charge Z in the lower ionosphere and middle atmosphere is developed in this paper. For this purpose the ionization losses (dE/dh) according to the Bohr–Bethe–Bloch formula for the energetic charged particles are approximated in three different energy intervals. More accurate expressions for energy decrease E(h) and electron production rate profiles q(h) are derived. The obtained formulas allow comparatively easy computer programming. The integrand in q(h) gives the possibility for application of adequate numerical methods – such as Romberg method or Gauss quadrature, for the solution of the mathematical problem. On this way the process of interaction of cosmic ray particles with the upper, middle and lower atmosphere will be described much more realistically. Computations for cosmic ray ionization in the middle atmosphere are made. The full CR composition is taken into account: protons, Helium (α-particles), light L, medium M, heavy H and very heavy VH group of nuclei.