• Journal of the Korean Institute of Intelligent Systems
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• v.22 no.4
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• pp.507-514
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• 2012

XML-based standards such as CCD(Continuity of Care Document) and CCR(Continuity of Care Record) have been developed for representation, integration, and exchange of personal health record(PHR), and various of researches on PHR based on the standards have been conducted. These researches have developed and used CCD/CCR parsers each with their own different ways, but it can be hard to develop and update the parsers because of the structural complexity of the standards. Moreover, inter-exchange between CCD and CCR documents in the PHR-related medical information systems should be possible for the interoperability of the systems. Therefore, we proposed a designing method to develop the tools treating XML-based CCD/CCR documents. And we implemented CCD/CCR parser based on the proposed method and developed a converter from CCD to CCR using the parsers. To confirm the usefulness of the developed tool, we performed an experiment of creating CCD documents using the personal health data gathered from chronically ill patients in Kyungpook National University Hospital and of converting from the CCD documents to CCR documents.

• Journal of Korean Society for Geospatial Information Science
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• v.5 no.1 s.9
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• pp.159-165
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• 1997

Because CCD camera acquires the digital images without separate processing, its availabilities are increased. In this study, for CCD camera calibration DLT equation and radial or decentering distortion equation are combined and the calibration parameters are calculated using three dimensional test model. The digital images acquired by CCD camera are matched using coefficient of correlation and the three dimensional coordinates of objects are determined. Also, the potential usefulness of CCD camera in close range photogrammetry is examined.

• Korean Journal of Optics and Photonics
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• v.6 no.3
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• pp.173-177
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• 1995

The scanning type modulation transfer function (MTF) measurement system of linear charge coupled device (CCD) imagers is fabricated and the MTF of a linear CCD imager is tested. Measured MTF values are very sensitive to small angle knife-edge skew within 1 degree and show different results in several wavelengths. The MTF of the linear CCD imager is measured in different color temperatures of a tungsten filament lamp and the MTF uniformity of ti,t eel) pixels is tested.tested.

• Journal of Astronomy and Space Sciences
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• v.24 no.4
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• pp.367-378
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• 2007

We present a software which we developed for the multi-purpose CCD camera. This software can be used on the all 3 types of CCD - KAF-0401E ($768{\times}512$), KAF-1602E ($1536{\times}1024$), KAF-3200E ($2184{\times}1472$) made in KODAK Co.. For the efficient CCD camera control, the software is operated with two independent processes of the CCD control program and the temperature/shutter operation program. This software is designed to fully automatic operation as well as manually operation under LINUX system, and is controled by LINUX user signal procedure. We plan to use this software for all sky survey system and also night sky monitoring and sky observation. As our results, the read-out time of each CCD are about 15sec, 64sec, 134sec for KAF-0401E, KAF-1602E, KAF-3200E., because these time are limited by the data transmission speed of parallel port. For larger format CCD, the data transmission is required more high speed. we are considering this control software to one using USB port for high speed data transmission.

• Journal of the Institute of Electronics Engineers of Korea SC
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• v.43 no.3 s.309
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• pp.25-30
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• 2006

An infrared imaging method is proposed in which direct measurement of the spectral response of CCD sensors can be achieved through digital image processing. This method allows for a simple and economic method to detect the spectral sensitivity of commercialized CCD sensors. The key components of the apparatus are a monochromator, CCD-sample supporter and a personal computer equipped with a digital image processing systems. Tentative experimentation conducted on the commercialized CCD camera has resulted in a fairly consistent agreement with the theoretical model.

• Journal of Astronomy and Space Sciences
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• v.11 no.2
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• pp.185-195
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• 1994

Using $1024\times1024$ pixels CCD camera of ChungBuk National University Observatory (CBNUO), 62 photometric observations were made on January 11-12, 1993. A time of minimum lights of U Cep was determined as JD Hel 2448999.7274 from our data. On October 21-22 in 1993, CCD photometry in V and R for GW Cephei and V700 Cygni was carried out with 309${\times}$584 pixels cooled CCD system of Behlen Observatory, University of Nebraska-Lincoln (BOUNL) and 168 observations were obtained. From the data times of minimum lights JD Hel 2449282.8485 for GW Cep and JD Hel 2449282.7979 were determined. To developed a new CCD system of CBNUO, the CCD photometry method using at CBNUO is compared with at BOUNL.

• The Bulletin of The Korean Astronomical Society
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• v.46 no.1
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• pp.49.2-49.2
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• 2021

천체관측은 무한대 거리에서 오는 광자의 양을 측정하는 분야로 미량의 광자를 측정하기 위하여 측정기의 냉각은 아주 중요한 문제가 되었다. 과거에는 측정기 냉각에 드라이아이스가 사용되어 왔으며, 1980년대에는 액체질소를 이용한 냉각이 주를 이뤘다. 액체질소를 이용한 냉각 방식은 액체질소를 생성하거나 구입하여야 하는 불편함이 있었으며, 주입시 낮은 온도로 인하여 항상 안전사고에 대비하여야 했다. 1990년대 이후 다양한 상업용 CCD의 개발로 인하여 상대적으로 저렴한 CCD를 판매하였으며, 상업용 CCD는 이전 -110℃의 냉각이 아닌 -30℃의 냉각 성능을 보였다. 상업용 CCD는 CCD 칩 내부의 진공 구현이 미비하였으며, 초기 판매시 아르곤 가스 또는 실리카겔 등으로 CCD 칩 내부의 습도를 낮춰왔으나, 구입 후 1~2년이 지나면 점차 가스 누설로 인하여 CCD 칩 내부에 얼음이 생기는 문제가 발생하기 시작하였다. 이번 연구는 CCD 칩 내부 공간에 진공튜브를 삽입하여 실시간 진공상태를 측정하는 한편, 10Torr 이상 진공 도달시 자동으로 내부 공기를 흡입하여 CCD 칩 내부를 항시 10Torr 이하로 유지하도록 개발하였으며, 10Torr 이하의 진공 유지시 습도 99%의 환경에서 최대 냉각인 -35℃를 유지하여도 전혀 얼음이 생기지 않음을 확인하였다. 이번연구로 개발된 자동 진공조절시스템이 각 천문대에서 사용중인 상업용 CCD에 적용된다면, 날씨환경에 관계없이 항상 최대냉각 상태로 천체관측을 진행할 수 있으리라 기대된다.

• Journal of Astronomy and Space Sciences
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• v.24 no.4
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• pp.349-366
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• 2007

We designed and developed a multi-purpose CCD camera system for three kinds of CCDs; KAF-0401E($768{\times}512$), KAF-1602E($1536{\times}1024$), KAF-3200E($2184{\times}1472$) made by KODAK Co.. The system supports fast USB port as well as parallel port for data I/O and control signal. The packing is based on two stage circuit boards for size reduction and contains built-in filter wheel. Basic hardware components include clock pattern circuit, A/D conversion circuit, CCD data flow control circuit, and CCD temperature control unit. The CCD temperature can be controlled with accuracy of approximately $0.4^{\circ}C$ in the max. range of temperature, ${\Delta}33^{\circ}C$. This CCD camera system has with readout noise $6\;e^-$, and system gain $5\;e^-/ADU$. A total of 10 CCD camera systems were produced and our tests show that all of them show passable performance.

• Journal of The Korean Astronomical Society
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• v.29 no.spc1
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• pp.385-386
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• 1996

A wide-field CCD detector for solar eclipse observations is discussed. The CCD is supposed to be of a moderate size, and the image of the corona is obtained by scanning the field of view. Results of the 1995 solar eclipse observation are shown which have been made with a prototype of the scanning CCD detector.

• Journal of Astronomy and Space Sciences
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• v.19 no.1
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• pp.39-46
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• 2002

BV observations for V523 Cas were performed with 1.8m telescope and 2K CCD camera at Bohyunsan Optical Astronomy Observatory, Korea, on October 27, 1999. ${\Delta}m$ light curves for 11 comparison objects were made. It was found that their light curve slopes are different each other. Factor analysis for items of slope, (b-v) , magnitude, X pixel, and Y pixel results that there is strong correlation between the slope and the location (X,Y). It might be due to problems of CCD cooling system.