密闭舱室中微生物防控实践

随着人类对外太空认知的增加和探索的深入，星球之间的交叉感染问题引起了越来越多的关注。行星保护已成为航天开发领域的一个重要的关注热点。本文对生物再生生命保障地基综合试验系统"月宫一号"105天有人密闭舱室中的微生物污染问题作了实验研究。实验获取的空气微生物演替规律可为今后密闭BLSS实验中建立更有针对性的微生物防控措施提供依据，并为解决密闭舱室微生物污染问题提供重要经验。     

Height-latitude structure of stationary planetary waves in the stratosphere and lower mesosphere

Daily UK Met Office stratospheric assimilated data for the Northern and Southern Hemispheres, accumulated for the period from 2004 to 2012 and pressure range of 1000–0.1 hPa, are used in this paper. The paper presents and thoroughly discusses spatial–temporal distributions of stationary planetary wave (SPW) amplitudes and phases, calculated on the basis of geopotential height, temperature, zonal and meridional wind data for zonal wave numbers 1 and 2 (SPW1 and SPW2). The climatological planetary wave amplitudes and phases are calculated by extracting waves from three types of data: daily, monthly mean and climatological monthly mean. It has been established that magnitude of amplitudes and height-latitude distribution of amplitudes of SPW1 and SPW2 depend on data processing method for all parameters. It has also been established that height-latitude distribution amplitudes and phases significantly differ for geopotential height, temperature, zonal and meridional wind and depend on wave number and hemisphere. However, height-latitude distributions of phases are little different from each other for the used methods of data processing.     

A multi-criteria fusion feature selection algorithm for fault diagnosis of helicopter planetary gear train

Planetary gear train is a prominent component of helicopter transmission system and its health is of great significance for the flight safety of the helicopter. During health condition monitoring, the selection of a fault sensitive feature subset is meaningful for fault diagnosis of helicopter planetary gear train. According to actual situation, this paper proposed a multi-criteria fusion feature selection algorithm (MCFFSA) to identify an optimal feature subset from the high-dimensional original feature space. In MCFFSA, a fault feature set of multiple domains, including time domain, frequency domain and wavelet domain, is first extracted from the raw vibration dataset. Four targeted criteria are then fused by multi-objective evolutionary algorithm based on decomposition (MOEA/D) to find Proto-efficient subsets, wherein two criteria for measuring diagnostic performance are assessed by sparse Bayesian extreme learning machine (SBELM). Further, F-measure is adopted to identify the optimal feature subset, which was employed for subsequent fault diagnosis. The effectiveness of MCFFSA is validated through six fault recognition datasets from a real helicopter transmission platform. The experimental results illustrate the superiority of combination of MOEA/D and SBELM in MCFFSA, and comparative analysis demonstrates that the optimal feature subset provided by MCFFSA can achieve a better diagnosis performance than other algorithms.     

Helium-3: Status and Prospects

We report on our continuing efforts to determine 3He abundances in H II regions and planetary nebulae. Our detections of 3He in some PNe show that some stars produce large amounts of 3He. However the H II region abundances show no evidence for this production. From our sample of > 40 H II regions, the subsample which should yield the most reliable abundances has 3He/H abundances which scatter between 1-2 × 10-5. There is no trend with either galactocentric distance or metallicity. Even if we do not understand the underlying mechanisms, we see empirically that stars neither produce nor destroy 3He in a major way. We thus suggest that the level of the "3He Plateau" (3He/H = 1.5 _-0.5 ^+1.0 × 10^-5) is a reasonable estimate for the primordial 3He.     

液体粘性软启动装置的启动特性研究

介绍了液体粘性软启动传动装置的基本结构,建立了液体粘性制动器的粘性制动数学模型.研究结果表明,在制动过程中,摩擦片间隙、粘性转矩以及摩擦片转速之间存在耦合关系.粘性转矩的变化取决于摩擦片转速和摩擦片间隙趋近0的速度.当采用不同的摩擦片间隙变化规律时,随着该间隙的减小,相应的粘性转矩和运动摩擦片转速具有明显不同的特性.     

行星齿轮传动的功率分流动态均衡优化设计

本文研究了浮动件支承刚度对行星齿轮功率分流动态均衡性的影响,引入功率分流动态不均衡系数K_c和动载系数 K_d,定量地描述了不同支承刚度下功率在各行星齿轮间分配不均衡程度和啮合动载荷波动程度。以浮动件支承刚度为设计变量,使 K_c和 K_d 达到极小为目标函数,采用遗传算法对 2 K -H行星齿轮传动进行了动态优化设计。研究表明:优化后的行星齿轮传动不仅固有频率有所降低,而且在工作转速附近,功率分流不均衡及动载荷皆有较大改善。      

立式捏合机桨叶结构参数对混合釜流场影响的仿真分析

为揭示立式捏合机桨叶几何结构参数与混合釜流场之间的关系,以1 L两桨立式捏合机为研究对象,采用计算流体力学ANSYS Fluent 14.5软件对立式捏合机进行了三维模型仿真研究,分析了桨叶结构参数(桨桨间隙、桨叶螺旋角)的改变对混合物料挤压应力和剪切应力的影响。结果表明,增大桨桨间隙可减小桨叶对混合物料的挤压应力和剪切应力,空心桨螺旋角分别为40°、45°、50°,桨桨间隙由1.0 mm增加到3.0 mm,挤压应力、剪切应力分别平均减小了82.4%、57.23%;增大桨叶螺旋角可增大桨叶对混合物料的挤压应力和剪切应力,空心桨间隙分别为1.0、2.0 mm,桨叶螺旋角由35°增加到55°,挤压应力、剪切应力分别平均增加了92.8%、55.7%。     

Debris Discs Around Stars: The 2004 ISO Legacy

Debris discs around stars were first discovered by the Infrared Astronomical Satellite (IRAS) in 1983. For the first time material orbiting another star than the Sun, but distinct from a circumstellar envelope, was observed through its far infrared emission. This major discovery motivated astronomers to investigate those discs by further analyzing the IRAS data, using ground-based telescopes for the hunting of exoplanets, developing several projects using the Infrared Space Observatory (ISO), and now exploiting the ISO Data Archive (IDA). This review presents the main ISO results, statistical as well as individual, on debris discs in orbit around pre-main-sequence and main-sequence stars. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

Cassini Radio Science

Cassini radio science investigations will be conducted both during the cruise (gravitational wave and conjunction experiments) and the Saturnian tour of the mission (atmospheric and ionospheric occultations, ring occultations, determinations of masses and gravity fields). New technologies in the construction of the instrument, which consists of a portion on-board the spacecraft and another portion on the ground, including the use of the Ka-band signal in addition to that of the S- and X-bands, open opportunities for important discoveries in each of the above scientific areas, due to increased accuracy, resolution, sensitivity, and dynamic range.This revised version was published online in July 2005 with a corrected cover date.