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5GHZ대 연속 전파 수신 시스템의 개발
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  • 5GHZ대 연속 전파 수신 시스템의 개발
저자명
변도영,최한규,이정원,구본철,Byeon. Do-Yeong,Choi. Han-Gyu,Lee. Jeong-Won,Gu. Bon-Cheol
간행물명
천문학논총
권/호정보
1996년|11권 1호|pp.109-123 (15 pages)
발행정보
한국천문학회
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기타
이 논문은 한국과학기술정보연구원과 논문 연계를 통해 무료로 제공되는 원문입니다.
서지반출

기타언어초록

We have developed a 5GHz continuum receiver system. The receiver is a direct type receiver. In order to reduce the noise due to the fluctuation of the gain in the amplifiers, the system employs the Dicke switching method. We made the 5GHz low-noise amplifier and the bandpass filter. The low-noise amplifier gives ${sim}35dB$ gain and has ${sim}210K$ noise temperature. The bandpass filter has a passband between 4.3 and 5.4GHz. We also made switch driver, video amplifiers, phase detector, and integrator. Using a 1.8 meter offset parabolic antenna, we measured the efficiency of the system. Since the antenna does not have a driver to track objects, observations were performed with the antenna fixed. The measured noise temperature of the system is ${sim}650K$. From the observation of the blank sky, noise level was measured. It was found that the systematic noise(${sim}0.5K$: peak to peak value) is much larger than the thermal noise. The systematic noise is possibly related to the stability of the DC power supplied to the receiver system. Besides the noise of the system, it was found that the airplanes are the very serious noise sources. We measured the radio flux of the Sun using the developed system. The observed radio flux of the Sun is ${sim}10^6Jy$, which is close to the known value of the quiet Sun. The test observation of the Sun shows that the angular beam size of the antenna is ${sim}2.2^{circ}$.