• 자원환경지질
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• 제31권1호
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• pp.45-52
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• 1998

Paleomagnetic data have been obtained from the Lower Triassic Tonggo Formation which is exposed in Tanyang area comprising the Pyeongan Supergroup in eastern Korea. Mean characteristic direction of the Tonggo Formation is declination/inclination=$121.4^{\circ}/-26.4^{\circ}$ (k=52.7, ${\alpha}_{95}=7.2^{\circ}$, N=9 Sites) and paleopole at longitude/latitude=$30.7^{\circ}E/33.3^{\circ}N$ ($dp/dm=4.2^{\circ}/7.8^{\circ}$). The mean direction passes reversal test and fold test at 99% confidence level. Therefore, it is inferred to be a pre-folding component. The paleopole position of this study is close to the Triassic pole positions of the North China Block; it is far from those of the South China Block. Therefore, a first order correlation between the Korean Peninsula and North China at least since Lower Triassic times is identified in this study.

• 한국태양에너지학회:학술대회논문집
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• 한국태양에너지학회 2009년도 춘계학술발표대회 논문집
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• pp.245-249
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• 2009

Antarctic King Sejong Station was established in King George Island, the South Pole in 1988, and has been executing the monitoring studies on the change of antarctic natural environment. As an available power, the wind energy generator has been used in the form of hybrid with mainly diesel generator. Because the wind generation power sharply changes by wind energy, it must be careful during the system operation. When the power system becomes stable, the output performance of wind energy generator becomes stable. But, in case of unstable system, the errors frequently occur on the wind energy generator and it badly impacts the power system by output of wind energy generator. The purpose of this paper is to analyze suitability while operating the system of 10kW wind energy generator at Antarctic King Sejong Station, an isolated area, and to analyze the problem and improvements by power quality.

• 천문학회보
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• 제42권1호
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• pp.29.4-30
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• 2017

Korea Astronomy and Space Science Institute We present a weak-lensing study of the galaxy cluster SPT-CL J2106-5844 at z=1.132 discovered in the South Pole Telescope Sunyaev-Zel'dovich (SPT-SZ) survey. The cluster is claimed to be the most massive system at z > 1 in the SPT-SZ survey. The inferred mass ($M_{200c}=(1.27{\pm}0.21){\times}10^{15}M_{sun}$) is somewhat unusual at such a high redshift given the current ΛCDM prediction. The mass estimates, however, may be biased because the hydrostatic assumption may not hold when the universe was about 40% of the current age. In this work, we reconstruct the dark matter distribution and measure the mass of this interesting cluster using weak-lensing analysis based on the images from the Advanced Camera for Surveys and Wide Field Camera 3 on-board the Hubble Space Telescope. We find that the mass distribution of the cluster is unimodal with no significant substructures. The centroid of the dark matter agrees with both galaxy luminosity and number density distributions, as well as the hot gas centroid. We confirm that the cluster is indeed extremely massive ($M_{200c}=(1.81{\pm}0.47){\times}10^{15}M_{sun}$) supporting the previous non-lensing measurements. We also discuss the rarity of the cluster in the ΛCDM cosmology, comparing with the expected abundance of similarly massive clusters.

• 한국기계가공학회지
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• 제20권12호
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• pp.71-77
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• 2021

An impeller identification technique that is essential for adding viscosity measurement functions to overhead stirrers is presented in this study. Previous studies have revealed that using magnets facing the same poles arranged in a row can aid in distinguishing the types of impellers by detecting the number of magnets in a non-contact manner. However, as these previous studies measured the magnetic fields using analog Hall sensors, a converting circuit for the digital signals is required that can interface with the MCU. In this study, it was demonstrated that the number of magnets can be distinguished without using a separate conversion circuit by using a Hall sensor with a digital output. Owing to the unique hysteresis characteristics of digital Hall sensors, it was confirmed through experiments that the complex and diverse outputs appear depending on the direction of the magnetic field, the arrangement of magnetic poles, and the moving direction of the magnet. The measurement of the magnetic field showed that an edge signal equal to the number of magnets inserted into the impeller was detected when the radial direction was used, and the south pole was first approached.

• Journal of Astronomy and Space Sciences
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• 제22권3호
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• pp.263-272
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• 2005

2008년 발사 예정인 통신해양기상위성의 해양 관측자료 분석에 적용할 해수면에 나타나는 태양광 반사점의 위치를 찾아주는 알고리즘을 연구하였다. 태양-위성-지구의 기하학적 위치를 고려한 위성과 태양의 방위각과 고도각의 계산을 통해 비선형 방정식을 유도하였고, 뉴톤-랩슨 수치 방법을 이용하여 해를 구하였다. 통신해양기상위성이 동경 $116.2^{\circ}E$ 혹은 $128.2^{\circ}E$에 위치하게 될 경우 위도 ${\pm}10^{\circ}(N-S)$와 경도 사이에 태양광 반사점이 분포하는 것을 알 수 있었다. 남반구의 낮 동안 태양광 반사점의 경로는 북극을 향해 휘어있고 반대로 북반구의 태양광 반사점의 경로는 남극을 향하는 분포 패턴을 도출해 내었다. 다양한 영상 센서를 가진 정지궤도 위성들의 태양광 반사점의 위치예측과 그와 관련된 연구를 수행하는데 있어 본 논문에서 연구한 알고리즘을 이용할 수 있다.

• 해양환경안전학회지
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• 제24권5호
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• pp.569-575
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• 2018

북극에 대한 관심이 높아지면서 쇄빙연구선의 필요성이 점점 커지고 있다. 특히 우리나라의 경우 2009년 진수된 7,500톤급의 아라온호가 유일한 쇄빙연구선인데, 현재 아라온호만으로는 북극과 남극의 관련 연구를 수행하는데 어려움이 있다. 이에 해양수산부에서는 제2쇄빙연구선의 건조를 추진 중에 있는데 제2쇄빙연구선 건조의 필요성과 규모의 적정성에 대한 논란이 있으므로 이러한 논란을 줄이고 보다 합리적인 의사결정을 위해서는 제2쇄빙연구선의 경제적 가치를 추정하는 것이 중요하다. 본 연구는 비시장재화의 가치측정방법론인 조건부 가치측정법을 활용하여 제2쇄빙연구선의 경제적 편익을 산정하였다. 특히 본 연구의 추정방법과 관련하여 통상적인 CVM은 가정되는 분포의 형태와 추정모형에 따라서 WTP 분석결과에 편차가 발생하게 된다. 이에 본 연구에서는 베이지안 추정법(Bayesian approach)을 활용한다. 분석결과에 따르면 가구당 연간 평균 WTP는 1,999원으로 추정되었으며 이를 전국 가구 수로 확대한 제2쇄빙연구선 건조 사업에 대한 총편익은 연간 약 373.9억 원인 것으로 산정되었다.

• 암석학회지
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• 제25권1호
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• pp.85-88
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• 2016

중앙해령에서는 해양지각으로 현무암과 같은 암석이 새로이 생겨나며, 암석에는 자기방향이 당시의 지구자기장에 따라 배열된다. 해수면상에서의 광범위한 자력탐사에 의해 대부분의 중앙해령-특히 대서양 중앙해령-의 중심축과 평행한 남-북 방향의 자기띠(또는 자기 줄무늬)가 알려져 있다. 이러한 지자기띠에 기초하여, 지구의 자기장은 지질시대 동안 여러 번에 걸쳐 반복하여 역전된 것으로 고려되어 왔다. 해양지각에서의 지자기 역전의 발견은 해양저확장과 대륙이동설 그리고 판구조론을 설명하는 중요한 증거가 되었다. 이 논문에서는 중앙해령 근처에서 지자기띠를 이루며 새로이 생겨나는 해양지각 자기역전의 가능한 메커니즘을 설명하는 간단한 장치를 소개하고자 한다. 이 장치는 중앙해령의 중심에서 암석이 가지는 특정한 자기극성을 가지도록 근처에 인접하는 자기띠가 막대자석의 역할을 함을 보인다. 따라서 새로이 생겨나는 지자기띠는 일반적인 지구자기장 뿐 만 아니라 국지적으로 마치 막대자석처럼 작용하는 중앙해령 근처에 이웃하는 기존의 지자기띠에 의해 영향을 받았을 가능성이 있는 것으로 사료된다.

• 대한원격탐사학회:학술대회논문집
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• 대한원격탐사학회 2005년도 Proceedings of ISRS 2005
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• pp.538-541
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• 2005

Tidal flats develop along the south coast ofthe Korean peninsula. These areas are famous for sea farming. Specially, strong and coherent radar backscattering signals are observed over oyster sea farms that consist of artificial structures. Tide height in oyster farm is possible to measure by using interferometric phase and intensity of SAR data. It is assumed that the radar signals from oyster farm could be considered as double-bouncing returns by vertical and horizontal bars. But, detailed backscattering mechanism and polarimetric characteristics in oyster farm had not been well studied. We could not demonstrate whether the assumption is correct or not and exactly understand what the properties of back scattering were in oyster farm without full polarimetric data. The results of AIRSAR L-band POLSAR data, experiments in laboratory and JERS-l images are discussed. We carried out an experiment simulating a target structure using vector network analyser (Y.N.A.) in an anechoic chamber at Niigata University. Radar returns from vertical poles are stronger than those from horizontal poles by 10.5 dB. Single bounce components were as strong as double bounce components and more sensitive to antenna look direction. Double bounce components show quasi-linear relation with height of vertical poles. As black absorber replaced AI-plate in bottom surface, double bounce in vertical pole decreased. It is observed that not all oyster farms are characterized by double bounced scattering in AIRSAR data. The image intensity of the double bounce dominant oyster farm was investigated with respect to that of oyster farm dominated by single bounce in JERS-l SAR data. The image intensity model results in a correlation coefficient (R2 ) of 0.78 in double bounce dominant area while that of 0.54 in single bouncing dominant area. This shows that double bounce dominant area should be selected for water height measurement using In8AR technique.

• 조명전기설비학회논문지
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• 제24권2호
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• pp.33-38
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• 2010

최근 태양광 발전시스템은 정부 에너지 정책에 의해서 널리 보급되고 있다. 여기에 광전지 전력생산의 효율을 높이기 위해서는 견실한 태양 추적식이 필요하다. 하지만 태양추적 식은 추적기술의 미비에 의해서 아직 널리 보급되지 못하고 있다. 이를 해결하기 위해서 본 논문에서는 태양광전지의 최대전력추적을 위해서 태양광센서 및 신경회로망 제어알고리즘을 적용하였다. 태양추적 센서는 평판위에 한 개의 사각기둥과 동, 서, 남, 북 4개의 광센서로 구성된다. 태양추적 2축 제어는 두 개의 모터에 의해서 각각 동작되며, 모터의 제어 입력은 신경회로망 제어 알고리즘에 의해서 계산된다. 제안된 제어방식의 기능은 태양추적광 발전 실험에 의해서 확인하였으며, 본 논문의 태양추적방식은 고정식 보다 32[%]효율을 증가시켰다.

• Journal of Astronomy and Space Sciences
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• 제34권2호
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• pp.171-182
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• 2017

In this study, the internal structure of a Heumgyeonggak-nu (欽敬閣漏) was designed, and the power transmission mechanism was analyzed. Heumgyeonggak-nu is an automated water clock from the Joseon Dynasty that was installed within Heumgyeonggak (欽敬閣), and it was manufactured in the $20^{th}$ year of the reign of King Sejong (1438). As descriptions of Heumgyeonggak-nu in ancient literature have mostly focused on its external shape, the study of its internal mechanism has been difficult. A detailed analysis of the literature record on Heumgyeonggak-nu (e.g., The Annals of the Joseon Dynasty) indicates that Heumgyeonggak-nu had a three-stage water clock, included a waterfall or tilting vessel (欹器) using the overflowed water, and displayed the time using a ball. In this study, the Cheonhyeong apparatus, water wheel, scoop, and various mechanism wheels were designed so that 16 fixed-type scoops could operate at a constant speed for the water wheel with a diameter of 100 cm. As the scoop can contain 1.25 l of water and the water wheel rotates 61 times a day, a total of 1,220 l of water is required. Also, the power gear wheel was designed as a 366-tooth gear, which supported the operation of the time signal gear wheel. To implement the movement of stars on the celestial sphere, the rotation ratio of the celestial gear wheel to the diurnal motion gear ring was set to 366:365. In addition, to operate the sun movement apparatus on the ecliptic, a gear device was installed on the South Pole axis. It is expected that the results of this study can be used for the manufacture and restoration of the operation model of Heumgyeonggak-nu.