• Proceedings of the Korean Society of Surveying, Geodesy, Photogrammetry, and Cartography Conference
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• 2003.04a
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• pp.23-36
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• 2003

본 논문은 천문측량의 기본원리와 관측방법에 대하여 간단히 소개함과 동시에 국내에서 천문측량으로 실시된 국가경위도원점의 설치와 독도 천문측량 등 국내의 천문측량 현황에 대하여 체계적으로 고찰하였다. 그리고 재래식 천문측량의 단점이던 장비운용과 측량방법을 개선하여 디지털 천정카메라에 의한 천문측량의 자동화에 대한 외국의 사례를 소개하고 디지털 천문측량에 의한 연직선편차의 측정결과를 고찰하여 이의 활용방안을 논하였다.

• The Science & Technology
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• v.32 no.3 s.358
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• pp.27-29
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• 1999

중국 당나라때 천문학자로 이름을 떨쳤던 일행은 683년 지금의 하남성인 위주에서 태어나 45세로 요절하기까지 천문관측에 큰 공헌을 남겼다. 양귀비의 애인이었던 현종의 발탁으로 수도 생활을 마치고 장안으로 들어온 일행은 천문관측기구를 사용하여 별자리인 기본성좌 28수의 위치값을 찾아냈으며 새로운 측량기구를 만들어 세계 최초로 지구의 자오선을 측량한 과학자이다.

• Journal of Korean Society for Geospatial Information Science
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• v.15 no.1 s.39
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• pp.47-53
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• 2007

Astronomic surveying has been regarded as an important method for absolute positioning of geodetic datum in each countries under the local geodetic reference system. The purposes of this study are to determine astrogeodetic geoidal heights referred to Bessel ellipsoid and to determine deflection of the vertical and geoidal heights referred to GRS80 of World Geodetic System by astronomic surveying data which have been surveyed after 1970 in Korea. The results show that $\xi$ component of the deflection of the vertical distribute from -5.725" to 8.005" and $\eta$ component distribute from -14.917" to 6.2" and astrogeodrtic geoidal heights distribute from 23 m to 27 m in the study area. Also, we could see that GRS80 was more optimal ellipsoid than Bessel 1841 ellipsoid to Korea through comparing both astrogeotic geoidal heights referred to GRS80 and Bessel 1841 ellipsoid.

• Journal of the Korean Society of Surveying, Geodesy, Photogrammetry and Cartography
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• v.11 no.1
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• pp.61-66
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• 1993

Position fixing is determined by triangulation, traverse surveying and astronomy surveying, However, when the station like a car move, it is impossible to determine the location of car. Satellite position fixing system can be used anywhere on earth arranged in 20, 000 km high with 24 satellites. The theoretical method of the fixing composition is possible to use satellite position fixing system. This paper is the part of the experiment which is dose for the development of the system used in Car-position fixing system. Also, this study is the comparison of one point positioning system and relative positioning system.

• Journal of Korean Society for Geospatial Information Science
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• v.3 no.2 s.6
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• pp.75-82
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• 1995

The calculation of astronomic latitude and longitude have been carried by astrolabe, theodolite. Conventional procedures to determine it require clear weather conditions, time high cost. So we need more effective method to decide them. The objective here is to present method to computate astronomic latitude and longitude by mixing GPS observation result and geodetic height. Also to decide geodetic height we used GPS/leveling, DMA(n=m=180) and OSU91A(n=m=360) methods. Compared to conventional procedures we could obtain astronomic latitude and longitude using GPS by $1{\sim}3'$ difference. If the precise geoid model of Korea will be developed, we can compute astronomic latitude and longitude effectively using GPS observation only.

• Journal of the Korean Society of Surveying, Geodesy, Photogrammetry and Cartography
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• v.17 no.1
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• pp.87-95
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• 1999

In this study, we investigated the methods of computing deflection of the vertical and compared the results of deflections of the vertical computed from astronomical coordinates and GPS observations, and computed from PNU95, EGM96 geoid model. By comparing the results of the deflections of the vertical, we found out the followings; 1) The deflections of the vertical computed from astronomical coordinates and geoid models are similar to each other. 2) The difference between the deflections of the vertical computed from each geoid models was smaller than the difference of those computed from astronomic coordinates and geoid models. 3) The effects of distribution of the points on the results are less than those of the data used in the computation. If there exists reference data about the deflection of the vertical, it would be possible to evaluate the accuracy of the geoid model using this method.

• Journal of Korean Society for Geospatial Information Science
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• v.5 no.1 s.9
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• pp.57-70
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• 1997

Conventional procedures to determine vertical deflections and astronomical coordinates require the stellar observations which be under restraints of clear night-time weather conditions, surrounding environment, long observation time and the use of instruments, etc. Therefore the more effective observation method subjugatting these problems has requested. The objective of this study is to propose method to compute vertical deflections, astronomical coordinates(latitude and longitude), and astronomical azimuth by mixing GPS observation results and orthometric heights. For this study, programmed the program which able to obtain the change in geoid undulation by using the GPS- determined geodetic height difference and the orthometric height difference, and GPS satellite surveying was performed at both ten points of astronomical points and four triangulation points around each astronomical station in South Korea. The Astronomical results determined from GPS observations compared to those determined from both conventional astronomical measurements and the recent earth gravitational Model(EGM96).

• Journal of the Korean Society of Surveying, Geodesy, Photogrammetry and Cartography
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• v.9 no.2
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• pp.1-8
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• 1991

The geoid is the one of major suject in Geophysics and Geodesy. The iregularities of the geoid will affect the computation of precise geodetic coordinates and moreover will cause an errors in trajectory computations and reference directions for inertial guidance system. The aim of this study is to develope the best local geoid model for Korea. For this purpose, an astrogeodetic levelling and surface fitting techniques have been applied in determination of the geoid as a first trials. As a result of it, a local geoid has been obtained with the standard errors of $\pm$0.49m and $\pm$0.66m respectively and the maximum geoid undulation in Korea is found as 22m~23m approximately.

• Journal of the Korean Society of Surveying, Geodesy, Photogrammetry and Cartography
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• v.3 no.2
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• pp.11-17
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• 1985

In the three dimensional Cartesian Coordinate System such as the satellite geodesy the relationship of the geoid and the reference ellipsoid must be known. Therefore, the determination of geoidal heights is regarded as one of the most important problem in geodesy. This paper deals with determination of astro-geodetic geoid by the spherical surface polynomials interpolation method. The data that astronomical deflection of the vertical was published by National Geography Institute is applied. The map of geoidal heights is drawn out. This shows that Tokyo Datum have influenced on Korea.

• The Bulletin of The Korean Astronomical Society
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• v.35 no.2
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• pp.85.2-85.2
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• 2010

우리나라에는 조선 태조와 숙종대에 돌에 새겨 만든 두 개의 천상열차분야지도(天象列次分野之圖)가 남아 전하고 있다. 숙종본 천문도는 태조본을 다시 복각한 것으로 알려져 있으며 천문도의 구성은 태조본의 뒷면과 같은 모습이다. 국보 228호로 지정된 태조본 천문도는 오랜 시간의 흐름에 따른 표면 마모로 명문이나 별자리 확인이 쉽지 않다. 특히, 태조본 뒷면은 심한 훼손으로 별의 크기 뿐 아니라 대부분의 별자리 확인도 어려운 상황이다. 지금까지 천문도 표면의 훼손으로 인해 태조본의 앞 뒷면과 숙종본에 새겨진 별의 위치와 크기를 정량적으로 비교하기가 어려웠다. 본 연구에서는 숙종본 천문도의 별자리와 함께 태조본의 앞뒷면 천문도의 별의 위치 및 크기를 정량적으로 비교하기 위해 2008년과 2009년에 걸쳐 태조본 석각 천문도를 3차원 정밀 측정하였다. 천문도 측정은 삼각측량과 간섭효과를 활용한 3차원 스캐너인 Breukmann을 사용하였으며 0.1mm 이내의 측정 정밀도로 측정하였다. 3차원 정밀 측정 자료는 유물 훼손을 대비한 복원 자료구축, 복제품 제작을 위한 기초자료 그리고 별자리 연구를 위한 천문자료 등으로 활용할 수 있다. 우리는 3차원 측정을 통해 석각 천문도의 전체 형태뿐 아니라 모든 별의 위치와 크기의 측정 자료를 DB화 하였으며, 이를 이용해 태조본의 앞 뒷면과 숙종본에 새겨진 별의 위치와 크기를 비교하고 각각의 특성을 조사하였다. 또한 천문도에 새겨진 별의 크기와 실제 별의 밝기와의 상관관계를 알아보았다.