• 한국지리정보학회지
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• 제16권1호
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• pp.36-46
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• 2013

세계 최초의 정지궤도 해양관측 위성인 천리안 위성의 해색 센서인 Geostationary Ocean Color Imager (GOCI)는 2011년 4월부터 원시 자료를 생산하고 있다. 본 연구에서는 GOCI 원시 자료로부터 보다 자연색에 가까운 컬러합성영상 제작을 위한 방법론과 자료처리용 소프트웨어인 GOCI RGB Maker를 개발하였다. GOCI 원시자료는 대기보정과 재투영 기법을 이용하여 최종적으로 컬러합성영상을 제작할 수 있도록 최적화된 알고리듬을 구현하였다. 이 알고리즘이 적용된 소프트웨어는 다양한 하드웨어 환경에서도 선택적으로 관심영역과 출력창의 크기를 입력받아 처리할 수 있도록 제작되어 교육적 효과를 높였다. GOCI RGB Maker는 공개용 소프트웨어로서, GOCI 자료에 대한 이해와 활용을 증대시킬 수 있을 것이다. 또한, 정지궤도 관측 영상은 관측 영역의 환경특성 변화를 감시하는데 훌륭한 역할을 할 수 있을 것으로 기대된다.

• 대한원격탐사학회:학술대회논문집
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• 대한원격탐사학회 2007년도 Proceedings of ISRS 2007
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• pp.159-161
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• 2007

Geostationary Ocean Color Imager (GOCI), the world-first ocean remote sensing instrument on geostationary Communication, Ocean, Meteorological Satellite (COMS), will be able to take a picture of a large region several times a day (almost with every one hour interval). We, KORDI, are in charge for developing the GOCI data processing system (GDPS) which is the basic software for processing the data from GOCI. The GDPS will be based on windows operating system to produce the GOCI level 2 data products (useful for oceanographic environmental analysis) automatically in real-time mode. Also, the GDPS will be a user-interactive program by well-organized graphical user interfaces for data processing and visualization. Its products will be the chlorophyll concentration, amount of total suspended sediments (TSS), colored dissolved organic matters (CDOM) and red tide from water leaving radiance or remote sensing reflectance. In addition, the GDPS will be able to produce daily products such as water current vector, primary productivity, water quality categorization, vegetation index, using individual observation data composed from several subscenes provided by GOCI for each slit within the target area. The resulting GOCI level 2 data will be disseminated through LRIT using satellite dissemination system and through online request and download systems. This software is carefully designed and implemented, and will be tested by sub-contractual company until the end of this year. It will need to be updated in effect with respect to new/improved algorithms and the calibration/validation activities.

• 시큐리티연구
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• 제2호
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• pp.227-258
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• 1999

In a broad sense, ‘After-care SYSTEM’ for discharged prisoners mean legal actions of prisoners who have been released from lawful detention In its narrow sense, mean preventive protection and observation activities under regular guidance and supervision against those released from penal facilities after a certain period of detention Therefore, they should not be viewed as objects of mere concern or social work programs but preventive protection should he provided to them as part of national criminal policy After-care system is in the following two ways, The one is based on individual prisoner's request and consent, which is called 'Voluntary After-care system', The other is the one which is not based in personal request or consent but is based on obligation, which is named 'Compulsory After-care system In Korea, however no Compulsory After-care system is in practice Voluntary After-care system is to be carried out 6 method in the following by existing Probation, Parole Law. (1) offer of board and lodging (2) allowance of Traveling expense (3) allowance of occupation instrument or lending rehabilitation fund (4) training of occupation and vocational guidance (5) self-reliance support for After-care probationer (6) guidance of good deed And then to establish the society without offenders is the ideal of human beings, but criminal acts don't fade away, so in the field of the science of criminology, the importance of correctional system has become greater. The correctional idea has moved from severe punishment to educational rehabilitation for the goal of protecting both offender and security from the threat of crime in to day Some it is required that Compulsory After-care system is most important system in effective measures, and that existing Probation, Parole Law in Korea is renewed into Compulsory After-care system in the future.

• 한국과학교육학회지
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• 제22권3호
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• pp.455-465
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• 2002

본 연구는 중학교 1학년 학생 30명을 대상으로 반복 측정, 대푯값 선정, 오차, 측정의 불확실성에 대한 신개념을 관찰 및 면담을 통하여 조사하였다. 조사 결과 50%의 학생들이 단 두 번만 측정하였고, 5번 이상 측정한 학생은 없었다. 반복 측정 후에 77%의 학생들은 자신의 느낌에 의거하여 측정값 중에서 대푯값을 선택하였고, 13%의 학생만 평균값을 계산하여 대푯값으로 정하였다. 60%의 학생은 측정 오차의 원인을 환경이나 측정 도구보다는 자신의 과실 때문이라고 하였다. 또한 대부분의 학생들은 다른 사람들에 의한 측정값이나 사간차를 둔 측정값이 달라지는 원인을 인간 때문이라고 생각하였다. 측정의 불확실성에 대하여 묻는 질문에 대하여 완전히 정확한 측정이 가능하다고 응답한 학생이 40%, 측정은 불확실하다고 응답한 학생이 33% 이었다. 학생들은 이에 대한 판단 근거로 주로 인간의 한계를 생각하였다. 결론적으로 과반수 이상의 학생들이 반복 측정 및 대푯값 선정에 대하여 이해하지 못하였고 측정 오차의 원인을 자신의 과실로 생각하였다. 또한 대부분의 학생들은 측정 결과가 다르거나, 측정이 불확실한 원인을 인간으로 생각하였다.

• 임상간호연구
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• 제18권2호
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• pp.296-306
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• 2012

Purpose: This study was done to compare the physical injury, emotional response and unplanned self-removal of medical devices in patients with physical restraints and patients not restrained. Methods: Eighty patients admitted to the intensive care unit (ICU) of a university hospital in Seoul participated in this study. Forty patients made up each group and the group not restrained was matched with the restraint group for age and history of smoking and alcohol consumption. Data on occurrence of physical injury, intensity of anxiety, stage of agitation and unplanned self-removal of medical devices were collected by observation and medical chart review using a structured instrument. Statistical processing of collected data was done with the SPSS WIN 17.0 program. Results: The physically restrained group experienced more physical injuries and recorded significantly higher levels of anxiety and agitation than the unrestrained group. However, there were no significant differences between the groups in occurrence of unplanned self-removal of medical devices. Conclusion: Results indicate a need for critical care nurses to carefully monitor physical injuries and emotional responses of physically restrained patients and to develop nursing interventions to prevent adverse effects associated with restraint use. There is also a need to develop patient safety guidelines when using physical restraints.

• 임상간호연구
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• 제18권2호
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• pp.251-263
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• 2012

Purpose: It was necessary for developing a neonatal classification system based on nursing needs and direct care time. This study was, thus, aimed at identifying nursing activities and measuring the standard nursing practice time for developing a neonatal patient classification system in Neonatal Intensive Care Unit (NICU). Methods: The study was taken place in 8 general hospitals located in Seoul and Kyungi province, South Korea from Dec, 2009 to Jan, 2010. By using 'the modified Workload Management System for critical care Nurses' (WMSN), nursing categories, activities, standard time, and task frequencies were measured with direct observation. The data were analyzed by using descriptive statistics. Results: Neonatal nursing activities were categorized into 8 areas: vital signs (manual), monitoring, activity of daily living (ADL), feeding, medication, treatment and procedure, respiratory therapy, and education-emotional support. The most frequent and time-consuming area was an ADL, unlike that of adult patients. Conclusion: The findings of the study provide a foundation for developing a neonatal patient classification system in NICU. Further research is warranted to verify the reliability and validity of the instrument.

• 천문학논총
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• 제21권2호
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• pp.51-59
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• 2006

We have successfully developed the KASI (Korea Astronomy and Space Science Institute) Solar Imaging Spectrograph (KSIS), which has been originally upgraded from the KASI solar spectrograph that was able to record solar spectra for a given slit region and to inspect the response function of narrow band filters. A prototype KSIS was developed in 2004 by using a scanning mirror in front of the spectrograph slit and a SBIG ST-8XE CCD camera. Its main disadvantage is that it took a long time (about 13 minutes) to scan a whole active region. In this work, we have upgraded the KSIS by installing a much faster Dalsa 1M15 CCD camera, which gives a data acquisition time of about 2.5 minutes. The software for KSIS was also improved for the new CCD camera on the basis of component-based development method. We have successfully made a test observation for a simple and small active region (AR10910) using the improved KSIS system. Our observations show that H-alpha images for several wavelengths have typical features in a sunspot as well as a H-alpha centerline image is quite similar to a BBSO H-alpha image, demonstrating the capability of the KSIS system.

• 천문학논총
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• 제30권2호
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• pp.201-204
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• 2015

The common-envelope process is a complicated phase in binary evolution. A lot of effort has been dedicated to study the common-envelope stage, but many questions related to this process are yet to be answered. If one member of the binary survives the common-envelope phase, the binary will emerge as a white dwarf accompanied by a low-mass main sequence star in close orbit, often referred as a post common-envelope binary (PCEB). SDSS J0745+2631 is among the list of newly found PCEBs from the Sloan Digital Sky Survey (SDSS). This star is proposed to be a strong eclipsing system candidate due to the ellipsoidal modulation in its light curve. In this work, we aim to confirm the eclipsing nature of SDSS J0745+2631 and to determine the stellar and orbital parameters using the software Binary Maker 3.0 (BM3.0). We detected the primary eclipse in the light curve of SDSS J0745+2631 in our follow-up observation from January 2014 using the ULTRASPEC instrument at the Thai National Observatory. The data obtained on 7th and 8th January 2014 in g filter show an evident drop in brightness during the eclipse of the white dwarf, but this eclipse is less prominent in the data taken on the next night using a clear filter. According to our preliminary model, we find that SDSS J0745+2631 hosts a rather hot white dwarf with an effective temperature of 11500K. The companion star is a red dwarf star with a temperature of 3800K and radius of 0.3100 $R_{\odot}$. The red dwarf star almost fills its Roche lobe, causing a large ellipsoidal modulation. The mass ratio of the binary given by the Binary Maker 3.0 (BM3.0) model is M2/M1 = 0.33.

• 천문학논총
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• 제30권2호
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• pp.217-218
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• 2015

In this work, we present the result of our follow-up observations of SDSS J092741.73+332959.1 and SDSS J130733.49+215636.7 using the 2.35 m Thai National Telescope and ULTRASPEC instrument. Both systems are listed among the recently found white dwarf main sequence binaries from the Sloan Digital Sky Survey. SDSS J092741.73+332959.1 is a new PCEB with a period of 2.3 days, the longest orbital period known to date for white dwarf binaries. SDSS J130733.49+215636.7 is confirmed to be an eclipsing system with a period of 0.21 days from the Catalina Survey's light curve, however the parameters for the white dwarf are still uncertain. Our goal is to determine precise parameters for both systems using the Binary Maker 3 software. The observation for SDSS J0927+3329 was done on 9 January 2014 in the SDSS r' filter while the data for SDSS J1307+2156 were taken in the z' filter on 27 April 2014. Our models show that the red dwarf companions in both systems are well constrained inside their Roche Lobes. We find that the binary M2/M1 ratio in SDSS J0927+3329 is close to 0.5, with white dwarf and M-dwarf temperatures of 12000 K and 3300 K, respectively. Our preliminary result for SDSS J1307+2156 show that this system has an extreme mass ratio of 0.3. The white dwarf in this system has a temperature of 7500 K and the companion star has an effective temperature of 3150 K.

• 천문학회보
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• 제37권2호
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• pp.239.1-239.1
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• 2012

This paper presents the results of one of early sciences with Korean VLBI Network (KVN): a large fringe survey of compact radio sources at 43GHz. We established the catalog of correlated flux densities in three ranges of baseline projection lengths of 637 sources from a 43 GHz (Q-band) survey observed with the Korean VLBI Network. Of them, 623 sources have not been observed before at Q-band with VLBI. The goal of this work in the early science phase of the new VLBI array is twofold: to evaluate the performance of the new instrument that operates in a frequency range of 22--129 GHz and to build a list of objects that can be used as targets and as calibrators. We have observed the list of 799 target sources with declinations down to $-40{\circ}$. Among them, 724 were observed before with VLBI at 22 GHz and had correlated flux densities greater than 200 mJy. The overall detection rate is 78%. The detection limit, defined as the minimum flux density for a source to be detected with 90% probability in a single observation, was in a range of 115--180 mJy depending on declination. However, some sources as weak as 70 mJy have been detected. Of 623 detected sources, 33 objects are detected for the first time in VLBI mode. We determined their coordinates with the median formal uncertainty 20 mas. The results of this work set the basis for future efforts to build the complete flux-limited sample of extragalactic sources at frequencies 22 GHz and higher at 3/4 of the celestial sphere.