G-16EP通用航空电瓶充放电及寿命研究

为了对G-16EP型电瓶进行维护和保养，根据电瓶厂家规定和适航规范，总结了该型电瓶的充电和容量测试（放电）方法，指出了影响电瓶寿命的主要因素，为该型号电瓶的维护提供了参考。     

WSO-UV project

During last three decades, astronomers have enjoyed continuous access to the 100–300 nm ultraviolet (UV) spectral range where the resonance transitions of the most abundant atoms and ions (at temperatures between 3000 and 300 000 K) reside. This UV range is not accessible from ground-based facilities. The successful International Ultraviolet Explorer (IUE) observatory, the Russian ASTRON mission and successor instruments such as the Galaxy Evolution Explorer (GALEX) mission or the COS and STIS spectrographs on-board the Hubble Space Telescope (HST) prove the major impact of observations in the UV wavelength range in modern astronomy. Future access to space-based observatories is expected to be very limited. For the next decade, the post-HST era, the World Space Observatory – Ultraviolet (WSO–UV) will be the only 2-m class UV telescope with capabilities similar to the HST. WSO–UV will be equipped with instruments for imaging and spectroscopy and it will be a facility dedicated, full-time, to UV astronomy. In this article, we briefly outline the current status of the WSO–UV mission and the science management plan.     

基于6σ设计的复合推力高速直升机总体参数多目标优化

针对复合推力高速直升机总体设计阶段总体参数的选择问题,提出一种提高可靠性和鲁棒性的基于6σ设计的改进多目标遗传算法优化方法。采用叶素理论和数值积分的方法分析计算了复合推力高速直升机气动及飞行性能,并以此为基础建立了约束函数和初步目标函数模型;将6σ设计融入改进的多目标遗传算法中,构造最终目标函数;在给定有效载荷设计要求下,对复合推力高速直升机总体参数进行了多目标优化设计。该方法获得了所需的Pareto解,优化后的复合推力高速直升机飞行性能相对原机有了较大改善,算例结果表明该方法有效可行。     

全数字式操纵负荷系统设计及实现

操纵负荷系统是人在回路仿真系统中的负载模拟装置,它要完成对飞行员十分敏感的驾驶杆力和脚蹬力的仿真,其部件模型的设计满足了操纵负荷系统的通用性。此操纵负荷系统在某型机工程模拟器上的应用测试结果表明,该设计符合直升机飞行模拟器鉴定标准的C级要求。     

某型三叶螺旋桨的设计及性能试验

根据飞行速度、需用拉力、螺旋桨转速等参数,设计了某型飞机的三叶螺旋桨,获得了弦长和桨叶角沿着径向的分布.制造了三叶复合材料螺旋桨（直径为1.75m）,在螺旋桨试验台上测试了不同转速下螺旋桨的拉力.为了获得螺旋桨的动态性能,制造了螺旋桨的缩比模型（直径为0.96m）,在西北工业大学NF-3风洞的三元试验段测试了螺旋桨的气动性能数据,包括:拉力、扭矩、功率、效率.结果表明:螺旋桨最大效率为85.63%,所设计的三叶复合材料螺旋桨适用于螺旋桨需用功率为70kW左右的发动机（比如Rotax912）,提出的螺旋桨设计方法具有较好的应用价值.      

Improved bolometric corrections for WR stars

Evolutionary models allow an assignment of both a mass and a luminosity to a Wolf-Rayet (WR) star in a cluster, and hence allow a determination of the Bolometric Correction (B.C.). The B.C.'s derived for WN stars range from –4.0 to –6.0 with the expected trend of larger values (in absolute values) for stars with higher excitation spectra. For WC stars, there is little evidence for a similar trend; most observations presented here are consistent with B.C.=–4.5, as found by Smith and Maeder (1989). The convergence of B.C. values derived from evolutionary and atmospheric models is extremely satisfactory, giving increased confidence in both methods.     

软件无线电概念及直接中频采样软件接收机方案

软件无线电是最近几年提出的一种实现无线电通信的新的体系结构，文章介绍了软件无线电的概念、特点、历史和现状，并且提出和分析了直接中频采样软件接收机实现方案。     

Halo White Dwarfs and Baryonic Dark Matter

We describe the formation of hot intergalactic gas along with baryonic remnants in galaxy halos. In this scenario, the mass and metallicity of the hot intracluster and intragroup gas relates directly to the production of baryonic remnants during the collapse of galactic halos. We construct a schematic but self-consistent model in which early bursts of star formation lead to a large remnant population in the halo, and to the outflow of stellar ejecta into the halo and ultimately the Local Group. We consider local as well as high redshift constraints on this scenario. This study suggests that the microlensing objects in the Galactic halo may predominantly be 0.5M white dwarfs, assuming that the initial mass function for early star formation favored the formation of intermediate mass stars with m 1M. However, the bulk of the baryonic dark matter in this scenario is associated with the ejecta of the white dwarf progenitors, and resides in the hot intergalactic medium.     

计算大型实对称特征问题的 Lanczos-QR 算法

为了计算大型实对称特征值问题Ｋｘ＝λＭｘ的少数低阶特征值对，本文给出Ｌａｎｃｚｏｓ－ＱＲ迭代方法。首先，给定初始迭代向量ｖ１，作ｍ步Ｌａｎｃｚｏｓ分解：ＫＶｍ＝ＭＶｍＴｍ＋ｈｍｅｍＴ。取Ｔｍ的ｄ个最大特征值为移位量，对Ｔｍ进行ｄ步带原点位移的ＱＲ分解。然后，修改初始迭代向量ｖ１。迭代地重新开始这一过程，迫使初始迭代向量ｖ１进入需求的特征子空间，从而使残量‖Ｋｘ－θＭｘ‖→０。数值例子表明，该方法收敛性强，且稳定、有效。     

On the electrodynamics of counter stream in pulsar’s inner annular cap region

The electric properties of pulsar’s inner annular gap are explored in this paper. Under two main assumptions, (1) the pulsar is alive, (2) the total charge of pulsar should not vary with time, the condition for the acceleration of negative particle in the annular region is derived. The acceleration condition is j₋ ? 0.5j₊, i.e., the current carried by negative particles is greater than or equal to 0.5 times of the current carried by positive particles. This condition holds even when the backward flow of positive particles exists in the annular region. It is noted that the outflow of negative particles offers good opportunities to understand the current closure problem of pulsar as well as wide radiation beam of pulsar observed at high energy band.