芦原宇宙通信教育研究施設の概要
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概要
- 論文の詳細を見る
A new subject named The Department of Space Communication Engineering had established by Fukui Institute of Technology at April 2001. For this new department, the Space Signal Receiving and Satellite Tracking System with 10 meters parabola antenna installed the latest high technologies had been built up at the Awara campus in the May 2001. The purpose of this facility is ma, de plan of the high grade actual training of space communication techniques for the undergraduate students and for the research and observations against the graduate students and the space scientists in the world. At the original design of this facility, they requested two distinguished receiving characteristics on the performances. First, the receiving frequency range is requested the very wide from L band (1.5 GHZ ) to Ka band (45GHz). The L and S band is used to the basic training of under graduate students and the X band (cm wave length) and Ka band (mm wave length) is used for Space Science Research and Radio Astronomy. A special plastic made sub, -dish is designed for this purpose. This sub-dish is worked as perpendicular for straight feed system to L and S bands wave, and centimeter and millimeter band below 45CHz is worked as complete reflector for Cassegrane system by means of special two layer coating in the plastic material. And this slide of frequency band change has done automatically with out any switching control. Second, other special receiving characteristics that installed in this facility is an extreme high speed and an extreme wide channels communications for PM-UQPSK detection systems install in all band receivers. And all control of this system is available by only one workstation. Other two special mentions of this system are as follows; 1. Sony Type DIR-2000 Magnetic Cassette Tape Recorder. This facility has the receiving data installation characteristics with the world highest recording speed in the world. 2. Anritsu Type Hydrogen Maser Atomic Time Standard Generator. The Time Stability is always kept 10^<-16> sec. This is the best stability in the world and this performance is prepared to participate in the international millimeter VLBI (Very Long Baseline Inter-ferometer) observation project of more precise international radio astronomical research cooperation in near future.
- 福井工業大学の論文
- 2002-03-20
福井工業大学 | 論文
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