OPTICAL TELEPHONE CORD PASSING THROUGH LONG PIPE WITH SPIRAL FLOW

A new effective technique, useful in telecommunications industry for passing an optical telephone cord attached to a connector through pipeline,has been developed using the spiral flow. Using this technique, the cord could be passed through a straight pipeline 150 meters long and a roll of vinyl tube 50 meters long. However, under the same condition, the cord could not pass through when using the turbulent flow. To obtain a high speed stable spiral flow, a nozzle with an annular slit connected to a conical cylinder was used. A pressurized fluid with no tangential flow was supplied through this slit and the fluid, passing through the conical cylinder, was deformed into spiral flow with the steeper axial velocity distribution compared to that of turbulence pipe flow due to Coanda effect and instability. As a result, the cord was attracted to the axis area of the pipe, which effectively increased the ability for the work of cord passing. This high ability for cord passing is attributed mainly to the reduct     

一种采用介质谐振器的X波段GaAsFET振荡器

一种采用介质谐振器的高稳定X波段GaAsFET振荡器已经研制出来。这种振荡器的频率稳定度低于±1MHz(-40℃～85℃),其外形尺寸大大地缩小了(20.3mm×12.6mm×8.8mm)。为介质谐振器研制了一种新材料Ba(NiTa)为O3—Ba(ZrZnTa)为O3,这种新型材料具有非常高的Q值和高的温度稳定性。在10GHz和Tf=0ppm/℃时,谐振器的特性为K=29,Q=10000。     

Comparison of Diurnal,Seasonal and Solar Cycle Variations of High-latitude,Mid-latitude and Low-latitude Ionosphere

Comparison of regular (diurnal, seasonal and solar cycle) variations of high-latitude,mid-latitude and low-latitude ionospheric characteristics has been provided on basis of local empirical models of the peak electron density and the peak height. The local empirical models were derived from the hand-scaled ionogram data recorded by DPS-4 digisondes located at Norilsk (69°N, 88°E), Irkutsk (52°N, 104°E) and Hainan (19°N, 109°E) for a 6-year period from December, 2002 to December, 2008. The technique used to build the local empirical model is described. The primary focus is diurnal-seasonal behavior under low solar activity and its change with increasing solar activity. Both common and specific features of the high-latitude (Norilsk), mid-latitude (Irkutsk) and low-latitude (Hainan) regular variations were revealed using their local empirical models.      

A facility for long-term Mars simulation experiments: the Mars Environmental Simulation Chamber (MESCH)

We describe the design, construction, and pilot operation of a Mars simulation facility comprised of a cryogenic environmental chamber, an atmospheric gas analyzer, and a xenon/mercury discharge source for UV generation. The Mars Environmental Simulation Chamber (MESCH) consists of a double-walled cylindrical chamber. The double wall provides a cooling mantle through which liquid N(2) can be circulated. A load-lock system that consists of a small pressure-exchange chamber, which can be evacuated, allows for the exchange of samples without changing the chamber environment. Fitted within the MESCH is a carousel, which holds up to 10 steel sample tubes. Rotation of the carousel is controlled by an external motor. Each sample in the carousel can be placed at any desired position. Environmental data, such as temperature, pressure, and UV exposure time, are computer logged and used in automated feedback mechanisms, enabling a wide variety of experiments that include time series. Tests of the simulation facility have successfully demonstrated its ability to produce temperature cycles and maintain low temperature (down to -140 degrees C), low atmospheric pressure (5-10 mbar), and a gas composition like that of Mars during long-term experiments.     

中频雷达风场的双谱分析

对中纬度中频雷达１９９７年６月８２ｋｍ高度的小时平均风场数据进行了动态谱分析和双谱分析,得到了中层顶区域谱行为具有多样性和各向异性的特点,以及行星波,潮汐波和重力波之间相位相干的现象,讨论了中层顶行星波,潮汐波和重力波之间存在非线性相互作用的可能性。     

A regenerable carbon dioxide removal and oxygen recovery system for the Japanese Experiment Module

The Japanese Space Station Program is now under Phase B study by the National Space Development Agency of Japan in participation with the U.S. Space Station Program. A Japanese Space Station participation will be a dedicated pressurized module to be attached to the U.S. Space Station, and is called Japanese Experiment Module (JEM). Astronaut scientists will conduct various experimental operations there. Thus an environment control and life support system is required. Regenerable carbon dioxide removal and collection technique as well as oxygen recovery technique has been studied and investigated for several years. A regenerable carbon dioxide removal subsystem using steam desorbed solid amine and an oxygen recovery subsystem using Sabatier methane cracking have a good possibility for the application to the Japanese Experiment Module. Basic performance characteristics of the carbon dioxide removal and oxygen recovery subsystem are presented according to the results of a fundamental performance test program. The trace contaminant removal process is also investigated and discussed. The solvent recovery plant for the regeneration of various industrial solvents, such as hydrocarbons, alcohols and so on, utilizes the multi-bed solvent adsorption and steam desorption process, which is very similar to the carbon dioxide removal subsystem. Therefore, to develop essential components including adsorption tank (bed), condenser. process controller and energy saving system, the technology obtained from the experience to construct solvent recovery plant can be easily and effectively applicable to the carbon dioxide removal subsystem. The energy saving efficiency is evaluated for blower power reduction, steam reduction and waste heat utilization technique. According to the above background, the entire environment control and life support system for the Japanese Experiment Module including the carbon dioxide removal and oxygen recovery subsystem is evaluated and proposed.     

对下一代卫星操作控制的系统研究

自1975年发射首颗ETS-1卫星以来,总计已发射了28颗NASDA(日本空间局)卫星。关于卫星的操作,NASDA已经开发了实时遥测/遥控处理系统,可通用于不同类型卫星。目前第三代系统已投入使用。而卫星操作的最新发展趋势则是更加复杂,例如正在出现采纳CCSDS建议的卫星,而且计算机技术也发展的相当迅速。 此外,NASDA在卫星操作中的任务正从主要是卫星星体操作发展为实验/整个卫星任务操作。根据这些情况,NASDA已经开始研究适于操作未来卫星的下一代操作系统。研究中考虑到以下几点: ·任务支持的要求 ·卫星设计的趋势 ·计算机环境的进展 本文是该研究的阶段性报告。