• Journal of Radiation Protection and Research
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• 제38권3호
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• pp.132-137
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• 2013

기존에 많이 사용된 반도체 검출기의 분해능은 통계학적 이론으로 그 분해능의 한계가 따른다. 이러한 이유로 최근에 반도체 검출기가 갖는 에너지 분해능의 한계를 뛰어넘는 저온 검출기를 이용하여 다양한 방사성 핵종 분석을 시도하고 있다. 본 논문에서는 $2{\times}2{\times}0.05mm^3$ 크기 금막 흡수체에 입사하는 에너지 때문에 흡수체의 온도가 상승하는 원리를 이용해 $^{241}Am$ 알파 선원의 에너지를 측정하였다. 흡수체의 온도 변화 측정에는 자기양자센서인 Au:Er를 이용하였으며 이는 순수한 Au에 핵스핀이 0 인 $^{168}Er$을 수백 ppm을 첨가하여 얻은 상자성 합금이다. 알파 입자 흡수에 의한 미세한 온도증가를 측정하기 위해서 희석식 냉동기보다 작동이 편리한 무냉매 자기냉동기를 이용해 mK 온도 영역의 저온환경을 구성하였다. $^{241}Am$ 선원 측정 결과 5.5 MeV에서 6.8 keV의 FWHM의 에너지 고 분해능을 얻었다.

• 한국환경과학회지
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• 제22권11호
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• pp.1415-1419
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• 2013

This study was conducted to investigate the seasonal variation characteristics of phytoncide in trail of Ulsan Metropolitan. Air samples were collected from May to December 2011. They were collected using Tenax Ta tube and phytoncides were detected and quantified using a Gas Chromatograph Mass Spectrometer (GC/MSD). This study are summarized as follows; The seasonal concentrations of phytoncide are Munsu Mt. 272.3 ${\mu}g/m^3$, Samho Mt. 192.4 ${\mu}g/m^3$, Shinbul Mt. 50.9 ${\mu}g/m^3$, Sibli Bamboo forest 22.4 ${\mu}g/m^3$ and Joongbu Fire Station 24.4 ${\mu}g/m^3$. In Munsu Mt., Samho Mt. and Shinbul Mt. major component ratio is ${\alpha}$-Pinene > ${\beta}$-Pinene+Myrcene >Limonene >Camphene > ${\gamma}$-Terpinene > ${\alpha}$-Terpinene. Bamboo forest and Joongbu fire station major component ratio is ${\alpha}$-Pinene >Limonene > ${\beta}$-Pinene+Myrcene >Camphene > ${\alpha}$-Terpinene. The variation of seasonal concentration is summer >spring >fall >winter. The phytoncide concentration of coniferous forest(Munsu Mt., Samho Mt.) is higher than broadleaf forest(Shinbul Mt.).

• 임산에너지
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• 24권2호
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• pp.24-30
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• 2005

향나무 잎을 채취하여 분쇄한 후 MeOH로 추출하고 분획한 다음 EtOAc 및 수용성 화합물을 칼럼크로마토그래피법을 사용하여 4개의 화합물 (+)-catechin (1), (-)-epicatechin (2), myricitrin (3) 및 hinokiflavone (4)을 단리하였다. 단리 화합물은 NMR 및 질량분석기를 사용하여 그 구조를 구명하였으며 DPPH radical 소거법을 이용하여 항산화 활성 검정을 시행하였다. 4가지 화합물 모두 우수한 활성을 보였으며 화합물 1, 2 및 3은 대조구로 사용한 ${\alpha}-tocopherol$, BHT 및 curcumin 보다 우수하였으나 화합물 4는 대조구보다 약간 낮은 활성을 나타내었다.

• 한국의류산업학회지
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• 제4권2호
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• pp.198-202
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• 2002

Degummed silk from Bombyx mori was dissolved in 9.3M lithium bromide solution. The regenerated silk fibroin films were completely ${\alpha}$-randomcoil type as shown by x-ray diffraction and infrared spectroscopy. The structural changes in silk fibroin induced by immersion into methanol and dilute hydrochloric acid and its photo-yellowing effect was studied. The changes of crystallinity were measured by infrared spectrometer. Yellowness index caused by ultraviolet irradiation were observed as a function of the structural change on silk fibroin. On treatment with methanol, ${\alpha}$-randomcoil silk film is converted to the ${\beta}$-form structure. After the treatment of hydrochloric acid on ${\beta}$-form structure in silk induced by immersion into methanol, ${\beta}$-form in silk fibroin is partially decreased. Crystallization owing to ${\beta}$-form transition reduced the initial yellowness index by ultraviolet irradiation. A little ${\beta}$-form structure in silk fibroin increased the initial yellowness in comparison with more ${\beta}$-form structure.

• Applied Biological Chemistry
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• 제38권5호
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• pp.473-477
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• 1995

Hymenoxys brachyactis지상부의 디클로로메탄 추출액으로부터 3개의 sesquiterpene lactone들과 새로운 lactone화합물인 isohymenograndin을 확인하였다. 그리고 2개의 sesquiterpene lactone축합물인 biennine C와 독성이 있는 것으로 알려진 flavone화합물인 hispidulin을 분리하여 각각을 고자장 NMR, Mass등의 기기를 이용하여 구조결정 하였다. Biennine C는 gas chromatography와 Mass분석을 통하여 독성화합물 hymenoxon과 화합물 8과의 Diels-Alder축합물임을 확인하였다. biennine C를 포함한 이상의 lactone화합물들은 ${\alpha},{\beta}$-unsaturated lactone으로서 독성화합물군으로서 알려진 hymenovin과 공통적인 구조를 갖고 있어서 생체독성을 나타낼 가능성이 높은 화합물들로 사료된다.

• Journal of Electrochemical Science and Technology
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• 제10권3호
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• pp.257-270
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• 2019

The inhibition performance of sodium gluconate (SG), cetyltrimethylammonium bromide (CTAB) and their mixture (SG/CTAB) on the corrosion behavior of ${\alpha}$-brass in 0.5 M $H_2SO_4$ solution has been investigated by potentiodynamic polarization, electrochemical impedance spectroscopy (EIS), Scanning Electron Microscope with Energy-Dispersive Spectrometer (SEM-EDS), Inductively Coupled Plasma Spectrometry (ICPS) and molecular dynamics (MD) simulation techniques. The results reveal that SG with 5ppm CTAB, noted SG/CTAB, acts as a good corrosion inhibitor and its inhibition efficiency reached 89% after 24 h immersion in sulfuric acid solution, but slightly decreased at higher temperatures. The polarization curves displayed that SG/CTAB acts as a cathodic-kind inhibitor. Electrochemical impedance spectroscopy (EIS) studies revealed that the addition of 5ppm CTAB to different concentrations of SG considerably increases the corrosion resistance of ${\alpha}$-brass. The SEM-EDS and ICPS analyses support the experimental results. Further, molecular dynamics (MD) simulations were used to understand the adsorption profiles of SG/CTAB on Cu(111) and Zn(111) surfaces.

• 한국약용작물학회지
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• 제8권1호
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• pp.49-57
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• 2000

오미자 (Schizandra chinensis Bullion)의 건조방법에 따른 휘발성성분의 변화를 알아보고자 생체시료와 건조시료에 대한 SDE (steam distillation & extraction) 추출분석과 Headspace 분석을 하였다. 건조방법별 오미자의 정유함량은 생체시료에서 0.58%, 냉동건조시료에서 0.60%, 열풍건조 $(60^{\circ}C)$ 시료에서 0.30%를 나타냈다. SDE 추출된 정유의 성분조성을 조사한 결과, 생체시료의 주요 성분은 terpinen-4-ol(9.01%), ${\gamma}-terpinene(7.02%),\;{\beta}-myrcene(7. 55%)$, 기타 sesquiterpene류(28.48%) 등으로 나타났다. 냉동 건조시료의 경우도 비슷한 경향을 보였으나, 열풍 건조시료에서는 ${\gamma}-terpinene(5.40%),\;{\beta}-elemene(8.28%)$, 기타 sesquiterpene류(50.38%)등을 주로 함유하여 열풍건조에 의해 성분 조성이 달라졌다. Headspace 분석의 경우 SDE 분석과는 다른 성분조성을 보였는데 생체시료는 ${\beta}-myrcene(22.05%),\;{\gamma}-terpinen(9.47%),\;{\alpha}-pinene(8.91%)$, sabinene (8.48%) 등이 주성분으로 나타났다. 건조시료의 성분조성은 대체적으로 냉동건조, $(60^{\circ}C)$ 열풍건조, $(80^{\circ}C)$ 열풍건조 순으로 ${\beta}-myrcene,\;{\alpha}-terpinene$ 등은 감소하였고, ${\alpha}-ylangene,\;{\alpha}-pinene$, camphene 등은 증가하는 경향이었다. 건조조건에 따라 정유성분의 함량과 조성 이 SDE 분석과 Headspace 분석 모두에서 변화하였는데, 전반적으로 monoterpene류와 알코올류의 조성은 감소하고 상대적으로 고비점 화합물인 sesquiterpene류의 조성은 증가하는 경향을 나타냈다.

• 대한전기학회:학술대회논문집
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• 대한전기학회 2001년도 하계학술대회 논문집 C
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• pp.1478-1480
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• 2001

ZnO : Al transparent conductive thin films were prepared by facing targets sputtering system with a DC power supply which can deposit a high quality thin films and control deposition condition in all range of $O_2$ gas ratio using ZnO target containing 8 at% of Al. Sputtering was carried out at a substrate temperature of R T with a DC current of 0.6 A and $O_2$ flow rate of 0 $\sim$ 0.9. The characteristics of ZnO : Al thin films was investigated by $\alpha$-step, four point probe, X-ray diffraction and UV/VIS spectrometer.

• 천문학회지
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• 제29권spc1호
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• pp.415-418
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• 1996

Space Solar Telescope (SST) is a space project for solar research, its main parameters are that total weight 2.0T, sun synchronous polar circular orbit, altitude of the orbit 730KM, 3 axis stabilized attitude system, power 1200W, telemetry of the downlink rate 30Mb/s, size $5{\ast}2{\ast}2\;M^3$, mission life 3 years. It is expected it will be launched in 2001 or later. The main objective is structure and evolution of solar vector magnetic field with very high spatial resolution. The payloads are consisted of 6 instruments: Main optical telescope with 1-M diameter and diffraction limited resolution 0.1 arc second, EUV imaging telescope with a bundle of four telescopes and 0.5 arc second resolution, spectrometric optical coronagraph, wide band spectrometer, H-alpha and white light telescope and solar and interplanetary radiospectrometer. An assessment study between China and Germany is under operation.

• 천문학회보
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• 제36권2호
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• pp.63.1-63.1
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• 2011

In understanding AGN physics, it is fundamental to determine black hole masses. Based on the gas kinematics of the broad-line region, black hole masses can be derived from the product of the width of the broad emission lines and the continuum/line luminosities. For a sample of 37 intermediate-luminosity AGN at z~0.4, we obtained high quality spectra (S/N~100) using the Low Resolution Imaging Spectrometer(LRIS) at the KECK telescope, in order to calibrate various black hole mass estimators based on the Mg II (2798A), the $H{\beta}$ (4861A), and the $H{\alpha}$ (6563$\bar{A}$) emission lines. Based on our multicomponent fitting analysis, we subtract continuum, FeII emission, and host galaxy starlight, reducing systematic errors in measuring emission line widths. Combining low S/N SDSS spectra with our high S/N keck spectra, we determine a set of ~30 black hole masses of the sample for each emission line. Then by comparing various sets of black hole masses, we internally calibrate each mass estimators and investigate uncertainties and limitations of each mass estimator.