• 에너지공학
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• 제13권2호
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• pp.93-100
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• 2004

간접법을 이용한 표면오염도 측정 시 시료채취와 동시에 방사선 검출이 가능한 스메어 매체를 제조하고 성능을 평가하였다. 스메어 매체는 무기섬광체를 고분자 막에 함침시킨 것으로서, 용매로는 디메틸포름아마이드(DMF)와 메틸렌클로라이드(MC) 그리고 고분자 소재로서 폴리설폰(PSF)을 사용하였고, 무기섬광체는 CAYS(cerium activated yttrium silicate)를 사용하였다. 함침막은 단일 및 이중구조로 제조하였고, 물. 메타놀 등 비용매성 욕조에 침지하거나 용매 증발을 통하여 고형화하여 특성을 비교하였다. 방사선과의 상호작용에 의하여 무기섬광물질 함침막으로부터 방출되는 광자의 계측은 광전증배관과 고전압원, 증폭기. 계수기로 구성된 원형계수기를 사용하였다. $^{14}$ C표면오염에 대해 무기섬광 함침막을 이용해 얻은 계수율을 통상의 저준위 알파/베타 계수기로 얻은 결과와 비교할 때 상대 감도가 약 50%로 나타났다. 또한, 계수효율이 상대적으로 낮았지만 저에너지 베타선 방출핵종인 $^3$H표면오염도측정이 가능하다는 것을 확인하였다.

• 대기
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• 제29권4호
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• pp.501-509
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• 2019

Asian Dust is a meteorological phenomenon that sand particles are raised from the arid and semi-arid regions-Taklamakan Desert, Gobi Desert and Inner Mongolia in China-and transported by westerlies and deposited on the surface. Asian dust results in a negative effect on human health as well as environmental, social and economic aspects. For monitoring of Asian Dust, Korea Meteorological Administration operates 29 stations using a continuous ambient particulate monitor. Kim et al. (2016) developed an automatic quality check (AQC) algorithm for objective and systematic quality check of observed PM₁₀ concentration and evaluated AQC with results of a manual quality check (MQC). The results showed the AQC algorithm could detect abnormal observations efficiently but it also presented a large number of false alarms which result from valid error check. To complement the deficiency of AQC and to develop an AQC system which can be applied in real-time, AQC has been modulated. Based on the analysis of instrument status codes, valid error check process was revised and 6 status codes were further considered as normal. Also, time continuity check and spike check were modified so that posterior data was not referred at inspection time. Two-year observed PM₁₀ concentration data and corresponding MQC results were used to evaluate the modulated AQC compared to the original AQC algorithm. The results showed a false alarm ratio decreased from 0.44 to 0.09 and the accuracy and the probability of detection were conserved well in spite of the exclusion of posterior data at inspection time.

• 천문학회보
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• 제36권2호
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• pp.61.2-61.2
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• 2011

Low-ionization nuclear emission-line regions (LINERs) have been generally regarded to be powered by active galactic nuclei (AGNs), yet still a number of alternative explanations on the origin of LINER emission are suggested; for example, planetary nebulae nuclei of massive stars, supernovae shocks from death of massive stars, and old stellar populations. Interestingly, a majority of recent star formation early-type galaxies (ETGs) in local universe presents such LINER emission lines. Given that situation, revealing the true nature of LINERs is a crucial step to constrain the evolution path to quiescent ETGs. To resolve the issue, we use Keck/LRIS to obtain spatially resolved spectra on a carefully selected ETG. The ETG SDSS J091628.05+420818.7 at redshift z ~ 0.024 shows modest LINER emission line features without any detection of 21 cm radio continuum nor X-ray emission. We perform a stellar continuum subtraction and measure emission line strengths and their uncertainties for each spectrum from five apertures along the slit with size of 1 arcsecond (~0.5 kpc). We find that extended spatial distributions of four emission lines $H{\alpha}$, $H{\beta}$, [OIII]${\lambda}5007$, and [NII]${\lambda}6583$, and they can be explained by central emission blurring effect. We conclude that the emissions seem to be centrally concentrated, indicating the AGN-nature of LINERs.