• 미생물학회지
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• 제6권4호
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• pp.122-130
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• 1968

Action of various wavelengths of visible light on ultraviolet-radiation damage to haploid yeast cells, Saccharomyces cerevisiae 23971, was studied. The results were obtained on the basis of the survival and respiration rates by pre- and post-illuminations of various wavelengths before and after U.V.-irradiations on the yeast cells. Among the wavelengths tested, 635 $m{\mu}$, 429 $m{\mu}$ and white light which caused increase of respiration in pre-treatment alone, induced less resistance to the U. V.-damage than in the control, in both pre- and U.V.-treatment. On the contrary, such wavelengths as 574 $m{\mu}$and 530 $m{\mu}$, showing a weak effect on respiration in pre-treatment increased the susceptability to U.V.-radiation. Photoinactivation was generally obtained by both pre- and post- illuminations along with U.V.-treatment. At 635 $m{\mu}$ the PI rate was the lowest and also a low PI rate was shown at 429 $m{\mu}$. But 429 $m{\mu}$, in the post-treatment of the yeast cells pre-treated by the white light and the darkness respectively, showed the highest PI rate. In both pre- and post- treatment of 574, 530 and 473 $m{\mu}$,the PI rates were high to the same degree. Post-treatments of the wavelengths on U.V.-treated yeasts incubated rather under the white light than the darkness induced lower PI rate. It is assumed that there are great differences in action even of the same wavelength, depending upon the various combination of pre- and post-treatments, and that, moreover, the action of various wavelengths of visible light on U.V.-damage on the cells are concerned with the doses and dose rates of U.V. and visible lights. These observations led to an interpretation that each wavelength of visible light might exert distinctively different effects oil U. V.-damage, mainly causing the inhibition or stimulation of enzymes in the yeast cells.

• 한국재료학회지
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• 제23권2호
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• pp.116-122
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• 2013

For fabricating silicon solar cells with high conversion efficiency, texturing is one of the most effective techniques to increase short circuit current by enhancing light trapping. In this study, four different types of textures, large V-groove, large U-groove, small V-groove, and small U-groove, were prepared by a wet etching process. Silicon substrates with V-grooves were fabricated by an anisotropic etching process using a KOH solution mixed with isopropyl alcohol (IPA), and the size of the V-grooves was controlled by varying the concentration of IPA. The isotropic etching process following anisotropic etching resulted in U-grooves and the isotropic etching time was determined to obtain U-grooves with an opening angle of approximately $60^{\circ}$. The results indicated that U-grooves had a larger diffuse reflectance than V-grooves and the reflectances of small grooves was slightly higher than those of large grooves depending on the size of the grooves. Then amorphous Si:H thin film solar cells were fabricated on textured substrates to investigate the light trapping effect of textures with different shapes and sizes. Among the textures fabricated in this work, the solar cells on the substrate with small U-grooves had the largest short circuit current, 19.20 mA/$cm^2$. External quantum efficiency data also demonstrated that the small, U-shape textures are more effective for light trapping than large, V-shape textures.

• 한국의상디자인학회지
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• 제2권1호
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• pp.113-121
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• 2000

The effect of Sunlight exposure on reducing the microorganism counts in the bedding materials was experimented by using 3 kinds of microorganisms(S. aureus, K. pnenmoniae and E. coli) and 3 kinds of fabrics (cotton, silk and polyester). Counts of the microorganism were examined before and after sunlight exposure. The sunlights were controlled U.V and Daylight D50 using MacBeth artificial light source. The specimens were exposed for 5 min, 10 min and 30 minutes under the $20^{\circ}C$ and 60% R.H, distance is 50cm from the light source. Results were as follows, 1. The reduction rate of the 3kinds of microorganisms was remarkably great under the U.V exposure. The U.V. exposure was very effective way to sterlize the bedding materials in the house care. 2. S. aureus was the most susceptible to U.V. exposure and the sunlight exposure. E. coli was the most resistant to the U.V and the sunlight exposure. 3. The reduction rate of the 3 kinds of fabrics was not significantly different. The polyester is more resistant than the silk and the cotton. Those were shown good reduction rate if all kinds of microorganism under the U.V and daylight.

• 한국수산과학회지
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• 제28권4호
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• pp.428-434
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• 1995

생선 횟집의 활어용 수조수에 대한 위생 대책 수립의 일환으로 자외선을 이용한 제균 효과를 검토하였다. 1. 물 두께 10mm (유수량: 730ml/sec, 등; 5조, 통과 시간: 2.4초)와 자외선 조사량 75W의 조건에서 자외선 등 통과 직후의 해수에서의 생균수 감소율은 평균 $85.0\%$였다. 2. 장염 비브리오균의 경우, 자외선 조사 후 1시간만에 3 log cycle 감소하였으며, 그 이후 큰 변화가 없었다. 3. 한편 쥐치에 같은 조건으로 72시간 처리했을 때 내장 세균의 감소는 거의 없었으나, 돌돔 및 쥐치의 표피와 아가미에서의 생균수 감소율은 약 2log cycle이었다. 4. 패류의 여수율을 좋게 하기 위하여 수조수의 온도를 $20-23^{\circ}C$로 조절한 수조에서 홍합과 굴을 같은 조건으로 처리했을 때 24시간 후에 생균수의 감소율은 홍합과 굴에서 각각 2 log cycle 정도였으며, 분변계 대장균의 경우는 각각 3 log cycle, 1.5 log cycle 정도 감소하였다.

• Transactions on Electrical and Electronic Materials
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• 제15권6호
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• pp.315-319
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• 2014

In this paper, we investigate visible light stress instability in radio frequency (RF) sputtered a-IGZO thin film transistors (TFTs). The oxygen flow rate differs during deposition to control the concentration of oxygen vacancies, which is confirmed via RT PL. A negative shift is observed in the threshold voltage ($V_{TH}$) under illumination with/without the gate bias, and the amount of shift in $V_{TH}$ is proportional to the concentration of oxygen vacancies. This can be explained to be consistent with the ionization oxygen vacancy model where the instability in $V_{TH}$ under illumination is caused by the increase in the channel conductivity by electrons that are photo-generated from oxygen vacancies, and it is maintained after the illumination is removed due to the negative-U center properties.

• Journal of Astronomy and Space Sciences
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• 제21권2호
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• pp.73-82
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• 2004

Samec et al.(1997)의 UBV 광도곡선과 Lu ＆ Rucinski(1999)의 시선속도곡선을 2003년에 개정한 Wilson-Devinney 쌍성모델을 적용하여 W형 과접촉쌍성 V417 Aql의 측광 및 분광학적 해를 새롭게 산출하였다. 광도곡선 분석에서 Qian(2003)이 제안한 제3천체의 광도를 광도곡선 분석에서 고려한 결과, 삼체의 광도가 U, B, V 필터에서 각각 2.7%, 2.2%, 0.4% 존재하고, 삼체의 광도를 고려한 경우가 그렇지 않은 경우보다 이론치와 관측치가 극심 부근에서 더 잘 일치하였다. 우리의 해로부터 V417 Aql의 절대 물리량을 $M_1$= 0.53 $M_{ }$, $M_2$= 1.45 $M_{*}$, $R_1$= 0.84 $R_{*}$, 그리고 $R_2$= 1.31 $M_{*}$으로, 거리를 216pc으로 산출하였다. 우리가 구한 거리는 Rucinski ＆ Duerbeck(1997)의 관계식 $M_{v}$ = $M_{v}$(log P, B-V)으로부터 계산한 거리(204pc)와 잘 일치하는 반면, Hipparcos 삼각시차에 의한 거리(131$\pm$40pc)보다 멀다. 그 차이는 Hipparcos 시차의 비교적 큰 오차 때문에 생긴 것일 수 있다. 수 있다.

• 한국환경과학회지
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• 제5권3호
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• pp.329-335
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• 1996

This project studies marine Vibrio vulnificus in oysters in the marine environment and attempts to correlate this bacteria's presence within various environmental parameters; we design this study to determine how different storage temperatures affect the survival of V. vuinficus in oysters and whether V. vulnificus is able to persist in oysters after exposure to UV light-disinfected seawater. Experimental depuration systems consist of aquaria containing temperature-controlled seawater treated with UV light and 0.2 ㎛ pore size filtration. Results showed that depuration at temperatures higher than 25℃ caused V. vuinificus counts to increase in oysters. Throughout the process, depuration water contained high concentrations of U vuinificus indicating"that the disinfection properties of UV radiation and 0.2 ㎛ pore size filtration were less than 어e release of V. vuinificus into seawater, In contrast, when depuration seawater was maintained at 10℃, the numbers of V. vuinificus were very little and multiplication in oysters was inhibited.

• Journal of Astronomy and Space Sciences
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• 제5권1호
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• pp.9-18
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• 1988

연세대학교 천문대에서 1983~1987 기간에 Be 성 $\gamma$ Cas을 총 31일 밤 광전측광관측을 하여 312개의 UBV관측점을 얻었다. 우리가 얻은 자료 중에서 비교적 관측시간이 길었던 5일분의 자료로, V, B-V, U-B광도 곡선을 만들었고, $\gamma$Case 의 일반적인 측광학적 특성을, V/R번화와 최근 IUE 인공위성관측에서 나타난 high velocity narrow component(hvnc)의 시기와 관련시켜 검토하였다. 또한, $\epsilon$ Per는 $H\beta$선의 모양(line, profile)이 심하게 변하는 이색적인 B형 별인데, 우리는 1984년에 IUE인공위성에서 관측한 이 별의 스펙트럼 image data 6개조를 분석하여 $H\beta$선에서와 같은 흡수선의 모양 변화가 UV영역의 SiIVsk CIV선에서도 일어나고 있는지를 비교검토한 결과, 이 6개 자료에서는 어떤 변화도 발견하지 못했다.

• 한국중재학회지:중재연구
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• 제24권3호
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• pp.79-103
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• 2014

In light of increasing international trade in recent years, international arbitration has been more widely used by international parties to resolve their conflicts. Thus, the need for reliable and effective enforcement of foreign arbitral awards has amplified. To facilitate the enforcement of foreign arbitral awards, the New York Convention lists grounds for the refusal of recognition and enforcement in Article V. This paper examines prominent U.S. case law on Article V(1)(b), which is put in place to ensure that arbitration proceedings are conducted properly in accordance with due process requirements: proper notice to parties and an opportunity to a fundamentally fair hearing. This examination of case law conveys that U.S. courts refuse to enforce foreign arbitral awards pursuant to Article V(1)(b) only when due process rights of the party against whom the award is to be enforced are clearly violated by the arbitral tribunal. This paper also reveals that U.S. courts mainly defer to arbitral tribunals' discretion, especially as to evidentiary matters. Therefore, it is predicted that U.S. courts will likely continue to narrowly construe the grounds in Article V to facilitate reliable and effective enforcement of foreign arbitral awards in the U.S.

• 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.