• The Bulletin of The Korean Astronomical Society
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• v.25 no.2
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• pp.70-70
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• 2000

• Proceedings of the Acoustical Society of Korea Conference
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• 1998.06c
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• pp.491-494
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• 1998

해양음향 토모그래피는 해수중을 전파하는 음파의 전파시간을 측정하여 이것으로부터 수온 및 유속의 분포를 구하는 새로운 관측기법이다. 해양음향 토모그래피에 의한 실시간 유속측정 시스템을 구축하기 위한 기초실험으로서 해양음향 토모그래피의 유속측정 유효성을 검증하기 위하여 쌍방향 음파전파의 해양음향 토모그래피 실험을 1997년 4월중에 거제도 남쪽해역에서 실시하였다. 실험시의 해양물리 환경을 고찰하고 토모그래피에 의한 유속측정 결과를 초음파 유속계(ADCP)에 의한 유속측정 결과와 비교 분석하였다. 그 결과 토모그래피에 의한 유속측정은 매우 양호하게 나타나, 향후 유속측정법으로 활용성이 크리라 기대되었다.

• Journal of the Korean Institute of Telematics and Electronics
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• v.26 no.2
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• pp.18-28
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• 1989

In this paper, we describe a pointing accuracy establishment and efficiency measurement of 13.7 m antenna for observing cosmic radio wave which is in the first stage just after finishing its installation. The initial stage of pointing model, 1 and 2 were set up with the observational data of Sun and Moon which are large in visual diameter and also strong in radio intensity. Based on this model, model 3 and 4 were established within the available operational range, i.e., 3.8" in azimuth deviation, 10.5" in elevation deviation, with the observational data of SiO maser source which is a point source and distributed in overall sky. Both apeture efficiency anhd beam efficiency were measured by observing Venus whose brightness temperature is well-known. The resulting corrected efficiencies were 35% and 50% respectively.

• Journal of Astronomy and Space Sciences
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• v.19 no.4
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• pp.327-340
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• 2002

In this paper, we performed the design study of a wide-band digital autocorrelation spectrometer for the observation study of an extra-galaxy's spectral lines and the survey research of the special radio sources in field of the radio astronomy observational research. The autocorrelation spectrometer designed in this paper can be used to their spectrometer of any system because this spectrometer has a wide dynamic power and frequency range properties. In this system we use the aliasing sampling method to minimize the band loss. For the output signal of the correlator we can increase the signal processing speed using by a special DSP chip, the integration and the FFT using hardware, so this spectrometer can support the newest developed technique for the radio astronomy observation so called “On the fly” method.

• 한국해양학회지
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• v.14 no.2
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• pp.78-85
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• 1979

Korea has not any fixed station for Radio Navigation systems yet. In some part of the Korean Sea, however, Japanese stations can be utilized for the Radio Navigation. 3 Decca chains were proposed to install the Decca Navigation network for Korea. Only for the coverage area, 1 Decca chain is sufficient for the sea around Korea instead of 3 chains. At present, Omega system is the most recommendable for the positioning in the farther area. In nearshore area, Raydist or Decca Trisponder is is useful for obtaining the position with high accuracy.

• Journal of the Korean Vacuum Society
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• v.20 no.2
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• pp.114-126
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• 2011

The light propagation along a long positive column has been observed in a cold cathode fluorescent lamp. The optical signals are observed with the DC and AC voltage power during lamp operation. The light propagating is observed in the operation with the DC-rippled voltage as well as the AC-voltage. The optical signals propagate from the high voltage side to the ground. These signals show two kinds of features according to the before and after Townsend breakdown. At the dark current before Townsend breakdown, the optical intensity is damped and the propagation velocity is $10^4{\sim}10^5m/s$. At the high current of normal glow after Townsend breakdown, the propagation velocity is 1$10^5{\sim}10^6m/s$ without damping.

• The Bulletin of The Korean Astronomical Society
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• v.36 no.2
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• pp.106.1-106.1
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• 2011

오리온 A에 대한 관측은 지난 2010년 11월부터 2011년 5월까지 총 350시간에 걸쳐서 대덕전파천문대의 14 m 망원경으로 수행했다. 관측 주파수는 12CO와 13CO로 하고 $3{\times}3$ array를 사용해서 오리온성운을 중심으로 한 $1^{\circ}{\times}1^{\circ}$ 영역을 관측했다. 데이터의 질을 다른 관측 결과들과 비교했을 때, 전체적으로는 양호하다 할 수 있겠으나, 몇 가지 시급하게 개선해야 할 점을 보여주었다. 데이터에는 오리온 A의 구조 가운데 여러 가지 특징적인 구조들이 나타나 있으며, 그 중에 별탄생 과정과 연관되었을 것으로 추론되고 있는 필라멘트 구조에 대해서 논의하였다.

• 한국지구과학회:학술대회논문집
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• 2010.04a
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• pp.117-117
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• 2010

외뿔소자리 신성 1975는 발견 당시에는 백색왜성과 적색왜성의 근접쌍성계인 것으로 알려졌으나, 엑스선 관측과 그에 따른 표준 정류 상태 원반 모형에 근거한 해석으로 중성자별 또는 블랙홀의 가능성이 대두되었다. 곧이어, 광학관측에 의하여 블랙홀 이중성임이 간접적으로 동정되었다. 최근 들어 1975젼 당시의 많지 않은 전파 관측 자료들을 재해석하여 상대론적인 물질 분출 현상, 즉 마이크로퀘이사 현상이 있었을 가능성이 관측적으로 제시되었다. 우리는 시간 종속적 열적 불안정성 모형을 바탕으로 수치모형을 계산하여 관측적으로 제시된 물질분출의 가능성을 이론적으로도 제시할 수 있음을 보인다

• Economic and Environmental Geology
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• v.39 no.4 s.179
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• pp.495-505
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• 2006

Atmospheric infrasound is defined as low frequency inaudible sound waves generated from natural phenomena and human activities. One property of long-distance travelling of infrasound makes it possible to detect the wave propagated from remote sound sources and to understand many geophysical phenomena generating it. Recently, advanced global infrasound sensor arrays are being deployed to monitor the clandestine nuclear test and to study geophysical phenomena in the world. In Korea, five seismo-acoustic arrays consisting of co-located seismometer and micro-barometer have been operated to discriminate the artificial explosions from the natural earthquakes in and around the Korean Peninsula. In addition to the discrimination purpose, these ways also record distinct infrasonic signals from natural phenomena on global scale such as large earthquake, bolide event, volcanic explosion, typhoon, and so on. As a new frontier in monitoring the earth, infrasound is being applied to understand various phenomena in and above the earth's surface.

• Journal of Satellite, Information and Communications
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• v.6 no.2
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• pp.97-101
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• 2011

Interplanetary space between Sun and Earth is area of flowing very fast solar wind which is contained X ray, flare, corona mass, etc. occurred Sun surface to Earth. This solar wind is affected directly to Earth magnetosphere and ionosphere so that this bring out broadcasting and communication interruptions, satellite operation obstacles and power gird defects and etc..Solar wind flow in interplanetary space is measured as solar wind speed, density and direction by measuring scintillation value to be produced during radio source is passed through solar wind. The wider effective collective areas and the more radio sources, accuracy of solar wind measuring is got higher. Function test was performed using 3 tiles which was manufactured as prototype. Restriction of quantity of tiles, test was performed to confirm whether measured beam pattern is complied with requirement or not. In this paper, it is shown design and their specification of ground interplanetary radio measurement system as well as technical issues and resolutions which were raised during design phase. Also result of function verification test using prototype is suggested. It is confirmed that measured beam pattern was met with requirement.