赛斯纳172R飞机着陆滑行停车故障研究

针对赛斯纳172R 飞机多次发生着陆滑行停车故障，对燃调系统结构和原理进行研究，分析了不当的维护检查工作、错误的操纵方法以及维护与操纵相互影响对燃调工作特性的影响，提出了针对性的维护、使用要求，可以有效避免该类故障的再次发生。     

散乱点云自适应滤波算法

提出一种散乱点云自适应滤波算法,该算法采用改进的R*-树组织散乱点云的拓扑近邻关系,基于该结构快速准确获取局部型面参考数据,自适应调节二维高斯分布的数字特征计算滤波权值,计算局部型面参考数据对原始型面数据的影响因子,以此作为权值计算各点滤波后的坐标,采用加权平均方法实现散乱点云的自适应滤波.实验证明该算法可有效提高点云的滤波效率,在保留原始型面特征的基础上,减小点云的随机误差,提高光顺性.     

High-cadence Hα imaging of solar flares

The Hα observation is a powerful tool to study the high-energy aspect of solar flares. Spiky brightenings of flare kernels at the Hα center reflect the rapid fluctuation in particle acceleration; linear polarization of Hα emission might be evidence of accelerated protons; red-shifts of the Hα line are caused by the chromospheric evaporation. To study the spiky brightenings of flare kernels with high-cadence imaging at the Hα center, a high-speed Hα camera for the Solar Flare Telescope at Mitaka, NAOJ, had been developed and it started the regular observation in 2001 July. However, the polarimetry and the Dopplermetry are also important and they are required to be carried out in parallel with the high-cadence imaging at the Hα center. Then, we upgraded the original high-speed Hα camera to a new Hα camera system for the multi-aspect Hα observations, which performs all of the high-cadence imaging, the linear polarization measurements, and the off-band imaging for velocity measurements. The new system started the observation in 2002 July. In this paper, the multi-aspect Hα imaging system is described and sample Hα images are presented.     

HCFC-141b 型聚氨酯泡沫塑料耐环境性能

对比分析经历模拟特定环境的环境交变试验、盐雾试验、加速老化试验和太阳辐射试验前后泡沫塑料的压缩强度、闭孔率、线胀系数和热导率等性能。结果表明,HCFC-141b型聚氨酯泡沫塑料经历环境老化后,压缩强度和热导率增加,线胀系数减小,闭孔率略有增加,热导率增加。太阳辐照试验对泡沫性能影响最大,试样SD-4压缩强度提高32%,闭孔率先增加后减少,线胀系数降低19%,热导率升高30%。     

惯性/卫星组合导航系统不组合问题浅析

惯性导航系统与GPS/GLONASS(简称GNSS)组合导航系统在导航特性方面的互补性,使惯性/卫星组合导航系统获得了广泛的应用。但组合过程中出现的不组合问题对组合精度有着极大的影响。针对使用中出现的不组合问题,深入研究了组合机理,建立了相应的故障树,根据故障模式提出了常用排故策略,大幅提升了排故效率和能力。     

Gamma rays from accreting matter onto collapsed objects

In the spherical accretion onto massive objects, the matter may be heated up to temperatures as high as 10¹² °K. In such a hot plasma, the thermal bremsstrahlung (e-e and e-p) and π° decay from inelastic collisions of protons are the main γ-ray sources. We determined the γ -ray production spectra from the π° decay and from bremsstrahlung for different temperatures. The expected γ-ray spectra were evaluated too in order to fit experimental data. We have fitted COS B data from 3C 273 using a two temperatures plasma model. The best fit is for

Full-size image (1K)

(M₈ is the black hole mass in 10⁸ M) which gives . The hard X-ray measurements do not contradict the bremsstrahlung spectrum.     

An identification for GEMINGA: A review of all the available data

Dedicated X-ray, optical and radio observations aimed at the identification of the bright γ-ray source 2CG195+04 (GEMINGA) are presented. A very promising candidate is found and its properties are discussed in the context of possible astrophysical scenarios.     

空间光学遥感器天然辐射效应数据库研究

空间环境是诱发卫星异常和故障的主要原因之一。光学遥感器作为卫星最重要的有效载荷之一，在空间会受到空间辐射环境的影响。因此在研制光学遥感器的同时，需要同时考虑空间辐射环境因素，文章就空间光学遥感器天然辐射效应数据库的设计和应用进行了介绍。     

关于互斥方案决策问题的研究

互斥方案决策时，运用净现值和内部收益率指标，经常遇到结论相矛盾的情况，本文主要应用方案重复法和投资增额评价法解决这一问题。