• Nuclear Engineering and Technology
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• 제55권10호
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• pp.3543-3548
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• 2023

Shutdown chemistry evolution is performed in nuclear power plants at each refueling outage (RFO) to establish safe conditions to open system and minimize inventory of corrosion products in the reactor coolant system (RCS). After hydrogen peroxide is added to RCS during shutdown chemistry evolution, corrosion products are released and are removed by filters and ion exchange resins in the chemical volume control system (CVCS). Shutdown chemistry evolution including RCS clean-up time to remove released corrosion products impacts the critical path schedule during RFOs. The estimation of clean-up time prior to RFO can provide more reliable actions for RCS clean-up operations and transients to operators during shutdown chemistry. Electric Power Research Institute (EPRI) shutdown calculator (SDC) enables to provide clean-up time by Co-58 peak activity through operational data from nuclear power plants (NPPs). In this study, we have investigated the results of EPRI SDC by shutdown chemistry data of Co-58 activity using NPP data from previous cycles and modeled the estimated clean-up time by EPRI SDC using average Co-58 activity of the NPP. We selected two RFO data from the NPP to evaluate EPRI SDC results using the purification time to reach to 1.3 mCi/cc of Co-58 after hydrogen peroxide addition. Comparing two RFO data, the similar purification time between actual and computed data by EPRI SDC, 0.92 and 1.74 h respectively, was observed with the deviation of 3.7-7.2%. As the modeling the estimated clean-up time, we calculated average Co-58 peak concentration for normal cycles after cycle 10 and applied two-sigma (2σ, 95.4%) for predicted Co-58 peak concentration as upper and lower values compared to the average data. For the verification of modeling, shutdown chemistry data for RFO 17 was used. Predicted RCS clean-up time with lower and upper values was between 21.05 and 27.58 h, and clean-up time for RFO 17 was 24.75 h, within the predicted time band. Therefore, our calculated modeling band was validated. This approach can be identified that the advantage of the modeling for clean-up time with SDC is that the primary prediction of shutdown chemistry plans can be performed more reliably during shutdown chemistry. This research can contribute to improving the efficiency and safety of shutdown chemistry evolution in nuclear power plants.

• 천문학회보
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• 제38권2호
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• pp.70.1-70.1
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• 2013

We present long-term optical to NIR data of the tidal disruption object, Swift J1644+57. The data were obtained with CQUEAN, UKIRT WFCAM observations. We analyze the morphology of the host galaxy of this object and decompose the bulge component using high resolution HST WFC3 images. We conclude that the host galaxy is bulge dominant. We also estimate the multi-band fluxes of the host galaxy through the light curves based on the long-term observational data. We fit the SED models to the multi-band fluxes of the host galaxy and determine its stellar mass. Finally, we estimate the mass of the central super massive black hole which is thought to be the main role of the tidal disruption event. The estimated stellar mass and black hole mass are $10^{9.1}M_{\odot}$, $10^{6.8}M_{\odot}$ respectively. We compare our results to other results that have studied before.

• Journal of Pharmaceutical Investigation
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• 제12권4호
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• pp.126-131
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• 1982

A quantitative fluorometric method was developed to determine aspirin and salicylic acid in bulk aspirin and commercial aspirin tablets. The excitation maximum for aspirin was observed at 280 nm and the emission maximum was at 335nm. The lowest energy excitation band for salicylic acid was at 308nm and the fluorescence emission band was at 450nm. Excipients, binders, lubricants and impurities did not interfere. Excellent recoveries were obtained for aspirin and salicylic acid. Results obtained by the KP III procedure and the proposed method were compared.

• 천문학회보
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• 제39권1호
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• pp.48.2-48.2
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• 2014

We present long-term optical to NIR data of the tidal disruption object, Swift J1644+57. The data were obtained with CQUEAN, UKIRT WFCAM observations. We analyze the morphology of the host galaxy of this object and decompose the bulge component using high resolution HST WFC3 images. We conclude that the host galaxy is bulge dominant. We also estimate the multi-band fluxes of the host galaxy through the light curves based on the long-term observational data. We fit the SED models to the multi-band fluxes of the host galaxy and determine its stellar mass. Finally, we estimate the mass of the central super massive black hole which is responsible for the tidal disruption event. The estimated stellar mass and black hole mass are ${\sim}10^{9.1}M_{\odot}$, ${\sim}10^{6.8}M_{\odot}$, respectively. We compare our results to other previous estimates.

• 한국정보통신학회:학술대회논문집
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• 한국정보통신학회 2016년도 춘계학술대회
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• pp.73-74
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• 2016

본 논문에서는 DTV용 광대역 사각형 루프 안테나에 대한 설계 방법에 대하여 연구하였다. 제안된 루프 안테나는 사각형 루프 안테나와 중앙 급전점과 연결하는 원형 섹터가 결합된 형태이다. DTV응용을 위해 75옴 입력 임피던스와 정합하도록 입력 반사계수와 이득 특성을 분석하였다. 최적화된 안테나를 FR4 기판에 설계하였고, 전압 정재파비(VSWR; voltage standing wave) < 2인 대역이 464-1,310 MHz으로 DTV 대역(470-806 MHz)에서 동작하는 것을 확인하였다.

• Journal of the Korean Physical Society
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• 제73권11호
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• pp.1631-1636
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• 2018

Unpolarized 1.047-GeV proton inelastic scatterings from the Ni isotopes $^{62}Ni$ and $^{64}Ni$ are analyzed phenomenologically employing an optical potential model and the first-order collective model in the relativistic Dirac coupled channel formalism. The Dirac equations are reduced to $Schr{\ddot{o}}dinger-like$ second-order differential equations, and the effective central and spin-orbit optical potentials are analyzed by considering the mass-number dependence. The multistep excitation via the $2^+$ state is found to be important for the $4^+$ state excitation in the ground state rotational band for proton inelastic scatterings from the Ni isotopes. The calculated deformation parameters for the $2^+$ and the $4^+$ states of the ground state rotational band and for the first $3^-$ state are found to agree pretty well with those obtained from nonrelativistic calculations.

• 대한전자공학회논문지TC
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• 제48권2호
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• pp.79-84
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• 2011

본 논문에서는 아이솔레이션 에이드를 사용하여 격리도를 향상시킨 무선랜용 MIMO안테나를 설계하였다. IEEE 802.11.n의 무선랜대역인 2.4GHz대역과 5GHz대역에서 사용이 가능한 PIFA를 안테나 프레임과 접지면을 기준으로 대칭으로 배치하였다. 두 안테나 사이에 아이솔레이션 에이드를 삽입하여 2.4GHz대역의 격리도를 최대 5dB향상시켰고, 5GHz대역의 격리도를 최대 7dB향상 시켰다. 제안된 안테나의 전체효율은 60%이상이며, 계산된 ECC(Envelope Correlation Coefficient)는 0.1이하이다.

• 식물병연구
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• 제10권1호
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• pp.30-33
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• 2004

현재까지 벼 줄무의잎마름병(Rice stripe virus, RSV)은 남부지방에 국한되어 발생되어 왔다. 그러나 최근에는 RSV의 발생이 충청도, 경기도를 포함한 중부지방까지 확산되는 경향을 나타내고 있다. 이병의 병징은 육안으로는 생리적인 장해 현상과 구분하기가 힘들다 본 실험에서는 이병주 및 애멸구(Laodelphax striatellus)로 부터 viral RNA를 추출한 후 RNA복제효소 및 외피단백질유전자에 특이적인 primer를 제작하여 RT-PCR법에 의해 RSV를 검정하였다. 그결과 이병식물체 및 보독 애멸구로부터 RNA복제효소 유전자에 특이적인 band(1,023 bp) 및 외피단백질유전자에 특이적인 band(969 bp)가 관찰되었다.

• Bulletin of the Korean Chemical Society
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• 제22권7호
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• pp.743-747
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• 2001

New azomethine metal complexes were synthesized systematically and characterized. Beryllium, magnesium, or zinc ions were used as a central metal cation and aromatic azomethines (L1-L4) were employed as a chelating anionic ligand. Emission peaks o f the complexes in both solution and solid states were observed mostly at the region of 400-500 nm in the luminescence spectra, where blue light was emitted. Three of them (BeL1 (Ⅰ), ZnL2 (Ⅱ), and ZnL3 (Ⅲ)) were sublimable and thus were applied to the organic light-emitting devices (OLED) as an emitting layer, respectively. The device including the emitting layer of Ⅰ exhibited white emission with the broad luminescence spectral range. The device with the emitting layer of Ⅱ showed blue luminescence with the maximum emission peak at 460 nm. Their ionization potentials, electron affinities, and electrochemical band gaps were investigated with cyclic voltammetry. The electrochemical gaps of 2.98 for I, 2.70 for Ⅱ, and 2.63 eV for Ⅲ were found to be consistent with their respective optical band gaps of 3.01, 2.95 and 2.61 eV within an experimental error. The structure of OLED manufactured in this study reveals that these complexes can work as electron transporting materials as well.

• 천문학회보
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• 제40권1호
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• pp.78.3-78.3
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• 2015

About 70 high redshift quasars with $z{\geq}5$ have been discovered through combinations of standard broad-band filters to distinguish them from contaminating sources. However, among the discovered quasars so far, there is a redshift gap at $5{\leq}z{\leq}6$ due to the limitation of traditional filter sets and selection techniques. To understand the early mass growth of supermassive black holes and the final stage of the cosmic reionization, it is important to find a statistically meaningful sample of quasars with various physical properties. Here we suggest a new selection technique of high redshift quasars using medium-band filters: nine filters with bandwidths of 50nm and central wavelengths from 625 to 1025nm. Photometry with these medium-bands traces the spectral energy distribution (SED) of a source, similar to spectroscopy with R~15. We installed these filters to SED camera for QUasars in EArly uNiverse (SQUEAN) on the 2.1m telescope at McDonald Observatory, and conducted test observations of known high redshift quasars at $4.7{\leq}z{\leq}6.1$ and also dwarf stars for comparison. We found differences in SED shapes between high redshift quasars and dwarf stars, determined their locations on color-color diagrams, and demonstrated that the medium-band filters can enhance the efficiency of selecting robust quasar candidates in this redshift range. In this poster, we propose an effective selection method of high redshift quasars using these medium-band filters and discuss its effect on our high redshift quasar survey.