• 생물환경조절학회지
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• 제18권2호
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• pp.142-147
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• 2009

단기간 침수처리에 의한 유채의 영양생장과 생식생장기의 생리적 반응, 지방산 조성과 수확량에 관하여 조사하였다. 영양생장 단계에서 10일과 생식생장 단계에서 4일 침수한 결과를 영양생장과 생식생 장기 모두 광합성, 기공전도도와 증산량은 침수처리 기간과 회복시기에 현저하게 감소하였다. 침수처리가 끝난 처리구에서 광합성과 기공전도도는 $2{\sim}3$일 내에 대조구와 비슷한 경향을 보였다. 침수처리된 작품의 지방산 조성은 대조구에 비해 통계적 유의성의 차이를 보이지 않았지만 수확량과 관련된 요인들에서 현저하게 감소함으로 생식생장 단계에서의 단기간 침수처리가 수확량 요인에 큰 영향을 줌으로서 종자 수확량에 영향을 미칠 것으로 사료된다.

• Journal of Astronomy and Space Sciences
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• 제30권4호
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• pp.213-221
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• 2013

We present the first BVRI CCD photometric observations of V345 Cas made on 22 nights during the observing seasons in 2007-2008. Our light curves, resembling those of EB-type binary stars, are analyzed with the 2003 version of the Wilson-Devinney binary code. The photometric study shows that V345 Cas is a typical semi-detached binary system with the primary star being about ${\Delta}T$ = 2400 K hotter, two times more massive, but only 17% larger than the secondary star being filled with it's Roche-lobe. The orbit has a relatively large inclination of about $88^{\circ}$. A cool spot on the secondary component is modeled to explain a small light curve asymmetry. Absolute dimensions and related radiometric parameters of the eclipsing pair are calculated and their evolutionary states are discussed with the HR diagrams of mass-radius and temperature-luminosity. A period analysis of all available times of minima, including our measurements, indicates that the orbital period may vary in a cyclical way, unfortunately the secondary period for the variation can not be uniquely determined because of lack of present timing data.

• 천문학회지
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• 제1권1호
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• pp.1-18
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• 1968

The photometric orbital elements of an Algol-type eclipsing variable, DI Pegasi, are derived by means of Fourier transforms from two-color photoelectric observations. The system shows a long term variation of its orbital period, which is interpreted as due to a continuing mass loss mechanism from the secondary component. Physical dimensions and a model of the system are also suggested here.

• Preventive Nutrition and Food Science
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• 제22권1호
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• pp.30-36
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• 2017

Physicochemical properties of Fujian Yongchun aged vinegar (FYAV) and Shanxi mature vinegar (SMV) were compared in terms of the fermentation methods applied and aging periods (3, 5, 8, and 10 years), and combined E-nose/E-tongue analyses were performed to assess their flavors. Compared with submerged fermentation-derived FYAV, solid-state fermentation-derived SMV showed higher values of pH, brix, soluble solids, total phenolic content, and antioxidant activity, but not total acidity or total organic acids. Aging period resulted in an increase in pH, total phenolic content, and antioxidant activity. Principal component analysis based on E-tongue/E-nose analyses was performed to distinguish between the vinegars produced by different fermentation methods and under aging periods. Solid-state fermentation and an aging process were considered good techniques for vinegar brewing, considering the various organic acids and high levels of total phenolics and antioxidant activity.

• 대한본초학회지
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• 제30권1호
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• pp.11-18
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• 2015

Objectives : The objective of this study is to evaluate antioxidant activity and the main component content change of steaming-drying fermented Gastrodiae rhizoma extract. Methods : The antioxidant activities were determined for total polyphenol, flavonoid contents, SOD-like activity, electron donating activity, nitrite scavenging ability and major functional components(gastrodin and 4-hydroxybenzyl alcohol content) were also measured. Results : The polyphenol content of fermented Gastrodiae rhizoma by S. cerevisiae were higher than those of fermented Gastrodiae rhizoma by A. oryzae, and when the fermentation period is extended. SOD like activity of fermented Gastrodiae rhizoma showed to be increased by fermentation with S. cerevisiae than fermentation by A. oryzae. Electron donating activity of fermented Gastrodiae rhizoma were increased at almost parallel level as vitamin C, by fermentation. Notably, fermentation by A. oryzae was moderately better than fermentation by S. cerevisiae. Flavonoid content of Gastrodiae rhizoma showed to increasing by fermentation, particularly fermentation by S. cerevisiae was proven to be more effective than by A. oryzae. The more steaming-drying or increased period of fermentation would be resulted in more gastrodin contents but under the same conditions, 4-hydroxybenzyl alcohol content of fermentation by A. oryzae in case of steaming and drying 1 time and 3 time was higher than control. Conclusions : These results has strongly hint the possible applicability of fermentation might be effective to improve the diverse biological activities of Gastrodiae rhizoma and may further supports to develop a functional food materials.

• 한국문화재보존과학회:학술대회논문집
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• 한국문화재보존과학회 2004년도 제20회 발표논문집
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• pp.137-153
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• 2004

We have analyzed the ingredients of 17 pieces of Bronze Age bronze ware, and an additional 22 pieces of Koryo and Chosun dynasty bronze ware. We have also conducted analysis of the extraction sites where these bronze ware items were found. For analyzing the main ingredient the bronze ware items have been divided into 3 groups - Cu-Sn(70?75:20), Cu-Pb-Sn(70:10:10), Cu-Pb-Sn(60:10:20) type respectively. In tile cases of the Cu-Pb-Sn groups the division comes down to differences in the Cu content as the main component, and elements such as Ni, Fe, Co contribute as a micro ingredient. The geographical and periodic characteristics of ancient bronze ware items show that theircompositional element changes from Cu:Sn to Cu:Pb:Sn and the Cu content decreases with the period,while the Pb content increases with the period. Bronze ware items from Suchon Ri, Gongju (that were used in 3 B.C.) form very different categories from 3rd ${\~}$ 2nd B.C.. They additionally formed very different categories from those bronze ware items analyzed in this research. These bronze ware itemsare shown to be geographically close and periodically overlapped, but made of a new elemental composition. This shows an inflow of a production technical culture present in the new bronze wares. The main component content of Cu is lower, and the Co and Fe contents (as microelements) are much higher than that of other bronze ware items. Such facts showthat those bronze ware items used completely different materials from bronze ware items in other cultural areas, or that there were differences in smelting techniques In the places where ancient bronze ware items have been extracted, it is presumed that the materials originated from the southern parts of Korea andnorthern parts and southern parts of China. .As more bronze ware scientific research is compiled one can conclude that that there will be enough scientific evidence to study the Bronze Age culture of Koreasystematically.

• 한국식품영양과학회지
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• 제13권3호
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• pp.238-246
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• 1984

고추장의 품질향상과 양조법을 개선할 목적으로 Aspergillus oryzae, Aspergillus kawachii, Aspergillus shirousamii의 균주를 사용하여 만든 koji로 각각 고추장을 담금하고 양조과정 중의 성분을 비교하였다. 그 결과는 Aspergillus oryzae구와 Aspergillus kawachii구의 고추장 사이에는 성분이나 품질면에서 큰 차이가 없었으나 Aspergillus shirousamii 12 균주는 Aspergillus oryzae균주에 비하여 고추장의 아미노태질소 함량이 높아 숙성도가 빠르고 고추장의 향기와 색상이 현재 개량식 고추장에 널리 이용하는 Aspergillus oryzae에 비하여 우수하였고, 기타 일반 성분면에서도 손색이 없었다. 다만 pH저하가 심한 것이 결점으로 나타났다. 따라서 Aspergillus shirousamii의 pH저하를 방지하여 고추장 양조에 사용하면 고추장의 품질 향상이 가능하다고 본다.

• Journal of Astronomy and Space Sciences
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• 제11권1호
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• pp.21-30
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• 1994

VV Cep-type long period spectroscopic-eclipsing binary AZ Cas has been observed for five years, 1985 Oct~1990 Feb, UBV at the Ilsan Station of Yonsei University Observatory. A total of 431 observations (U=129, B=142 and V=160) are made for 86 nights. Instrumental differential UBV and B-V light curves made with these observations cover phases nearly a half of one period. There is no appreciable light variation in V but in other two passbands a gradual decrease of the brightness is clearly noticed. The loss of light in B resulted in a reddening in $\Delta(B-V)$ by + 0.06 at phases between 0.4~0.5 as compared with that of at phase ~0.1. This intrinsic reddening arouses a question why at the orbital phase of the transit of a hot star in front of a cool M supergiant the heating of the facing hemisphere of M supergiant by the strong radiation from the B stat is absent. With regard to this unusual situation we propose a hypothesis that a large amount of gas stream of low temperature ejected from the surface of M supergiant component towards the B star dominates the brightness of B star and the reflection effect.

• 한국자동차공학회논문집
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• 제16권5호
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• pp.164-170
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• 2008

A typical clutch system for automotive manual transmissions transfers hydraulic pressure generated by driver's pedal manipulation to the clutch diaphragm spring. The foot effort history during the period of push is different than the period of the clutch pedal's return. The effort or load difference is called clutch foot effort hysteresis. It is known that the hysteresis is caused by friction. The frictional force and moment are produced between various component contact points such as between the rubber seal and the inner wall inside the hydraulic cylinder and between the diaphragm spring and the pressure plate, etc. Understanding the clutch pedal foot effort hysteresis is essential for a clutch release system design and analysis. The dynamic model for a clutch release system is developed for the foot effort hysteresis prediction and a simulation analysis is performed to propose a tool for analysing a clutch system.

• Communications for Statistical Applications and Methods
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• 제20권4호
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• pp.271-281
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• 2013

This paper considers a problem of classification of variable stars based on functional data analysis. For a better understanding of galaxy structure and stellar evolution, various approaches for classification of variable stars have been studied. Several features that explain the characteristics of variable stars (such as color index, amplitude, period, and Fourier coefficients) were usually used to classify variable stars. Excluding other factors but focusing only on the curve shapes of variable stars, Deb and Singh (2009) proposed a classification procedure using multivariate principal component analysis. However, this approach is limited to accommodate some features of the light curve data that are unequally spaced in the phase domain and have some functional properties. In this paper, we propose a light curve estimation method that is suitable for functional data analysis, and provide a classification procedure for variable stars that combined the features of a light curve with existing functional data analysis methods. To evaluate its practical applicability, we apply the proposed classification procedure to the data sets of variable stars from the project STellar Astrophysics and Research on Exoplanets (STARE).