深空探测自主导航与控制技术综述

深空探测自主导航与控制技术是深空探测任务成功实施的关键。基于开展深空探测自主导航与控制技术研究的迫切性,综合分析和评述深空探测自主导航与控制技术的研究进展,着重分析深空探测自主导航与控制的必要性和国外深空探测自主导航与控制技术的研究发展趋势,提出深空探测自主导航与控制的关键技术,根据分析,提出了发展深空探测自主导航与控制技术的建议．     

用CFD研究高压比离心叶轮内的二次流动

高压比离心压缩机正在喷气发动机和燃机中得到越来越多的应用。然而,人们对其流道内三维粘性流动的认识却非常有限。本文基于已经过实验数据确认的CFD结果,详细地分析和讨论了一种高压比离心叶轮内在近设计点的三维流场,以揭示其中激波与边界层相互作用和二次流动结构等的特征。      

统一显示器系统的技术分析及其替代产品的研制

统一显示系统采用图形叠加技术完成综合信息的显示。在一幅图象中,分时显示以快速、灵活的笔划绘制的图形与准确和以适时的光栅形成的图形。一幅光栅图形中的逐行扫描与隔行扫描分时完成并使不同信息获得清晰稳定的显示效果。选择合理的设计方法来实现在LRU内部两种产品模块的原位替代。     

外加剂对聚丙烯纤维增强混凝土的早期抗裂性影响

采用平板限制收缩试验法,研究了减水剂与膨胀剂及其复合技术对聚丙烯纤维增强高性能混凝土的早期抗裂性的影响.结果表明,聚丙烯纤维增强高性能混凝土的早期抗裂性大小顺序为:UEA-N混凝土膨胀剂与聚羧酸高效减水剂复合的纤维增强高性能混凝土＞AEA混凝土膨胀剂与聚羧酸高效减水剂复合的纤维增强高性能混凝土＞AEA混凝土膨胀剂与萘系减水剂复合的纤维增强高性能混凝土＞纤维增强高性能混凝土.因此,采用UEA-N混凝土膨胀剂与聚羧酸高效减水剂的复合外加剂技术和聚丙烯纤维增强技术是防止高性能混凝土发生塑性收缩开裂的比较理想的技术措施.     

铁路道口报警及控制系统

为了保证道口行车安全,在无人监护道口设置闪光和语音报警及道口横杆控制系统,利用单片机和无线通信技术以实现列车接近道口时,道口报警闪光器和语音扬声器同时报警,并放下道口横杆;列车离开道口时,道口闪光器和语音扬声器同时关闭,并升起道口横杆。在分析和比较几种单片机和传感器的基础上,确定本系统采用MCS51系列低功耗单片机和磁电传感器。     

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。     

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.