• 한국소음진동공학회논문집
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• 제12권7호
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• pp.520-526
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• 2002

Identification of noose sources, their locations and strengths, has been taken great attention. The methods that can identify noise sources normally assume that noise sources are located in a free field. However, the sound in a reverberant field consists of that coming directly from the source plus sound reflected or scattered by the walls or objects in the field. In contrast to the exterior sound field. reflections are added to sound field. Therefore, we haute to consider the reverberation effect on the source identification method. The main objective of this paper is to identify noise source in the reverberant field. At fist, we try to identify noise sources in a rigid wall emc;psire using the beamforming method. In many cases of practical interest, the wall has admittance so that random reflections occur in an enclosure. In this paper, we assumed the complex reverberant field in the enclosure to be the sum of plane caves with random Incidence and magnitude. Then we try to explain effects of reverberant field at interior source identification.

• Current Photovoltaic Research
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• 제3권1호
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• pp.5-9
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• 2015

Absorption and luminescence characteristics of disperse red-19 (DR-19) and $TiO_2$ composite have been investigated with various poling electric field strengths. Two step synthetic processes were employed to employ the DR-19 to the $TiO_2$ sol-gel. Firstly, urethane bond formation between DR-19 (-OH) and 3-isocyanatopropyl triethoxysilane (ICPTES, -N=C=O) performed (ICPDR) prior incorporation to the $TiO_2$ sol-gel. Secondary, the hydrolysis of the ethoxy group from the ICPTES and condensation reaction between silanol groups from ICPTES and $TiO_2$ sol-gel were performed. The ICPDR and $TiO_2$ sol-gel ($DRTiO_2$) were mixed and stirred for several days. The composite was coated to the ITO coated glass substrate. Corona poling were performed before drying the composite with various electric field strengths. The absorption intensity decreased with the increase of the poling field strength, which resulted in the increase of poling efficiency. The photoluminescence also decreased as the poling field strength increased. There is long luminescence tail for the poled $DRTiO_2$ film compared with unpoled $DRTiO_2$ film. The luminescence long tail indicates that the self-trapped excitons and polarons were generated when the $DRTiO_2$ film was poled with electric field.

• 한국소음진동공학회:학술대회논문집
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• 한국소음진동공학회 2001년도 춘계학술대회논문집
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• pp.1203-1209
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• 2001

Identification of noise sources, their locations and strengths, have been taken great attention. The method that can identify noise sources normally assumes that noise sources are located at a free field. However, the sound in a reverberant field consists of that coming directly from the source plus sound reflected or scattered by the walls or objects in the field. In contrast to the exterior sound field, reflections are added to sound field. Therefore, we have to consider the reverberation effect on the source identification method. The main objective of this paper is to identify noise source in the reverberant field. At fist, we try to identify noise sources in a rigid wall enclosure using the spherical beamforming method. In many case of practical interest, the wall has an admittance so that complex reflection process occurred. In this paper, we assumed the complex reverberant field in the enclosure to be the sum of plane waves with random incidence and magnitude. Then the effects of reverberant field at interior source identification have been studied theoretically as well as experimentally

• 한국도로학회논문집
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• 제12권1호
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• pp.47-54
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• 2010

본 연구에서는 콘크리트 포장의 균열, 스폴링 등의 파손문제를 해결하기 위해 국내 시공사례가 없는 이층 포설 공법의 도입 및 기술 경제적 타당성을 검토하고자 하였다. 본 포장공법중 하나인 강섬유 보강 콘크리트(SFRC, Steel Fiber Reinforced Concrete)의 포장 배합 적용성이 검토되었다. 강섬유 함량과 포장 높이가 산정되었으며, 강섬유 보강 콘크리트의 물성 평가를 위해 압축강도, 휨강도, 휨인성 지수, 인장강도, 피로강도를 측정하였다. 슬럼프와 공기량은 대부분이 시방 기준을 만족하였으며, 28일 강도도 교통개방을 할 수준 정도로 발현되었다. 휨강도 실험 결과, 강섬유 보강 콘크리트가 무보강 콘크리트에 비해 휨인성은 증가하였지만 휨강도는 증가하지 않았다. 에너지 흡수능력, 피로 저항성 및 동결 융해저항성은 강섬유 보강 콘크리트가 무보강 콘크리트에 비해 향상되었다. 향후, 시험시공을 통해 강섬유 보강 콘크리트의 현장 적용성 및 공용성을 평가할 것이다.

• 한국융합학회논문지
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• 제13권3호
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• pp.363-370
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• 2022

본 연구는 간호대학생의 강점인식과 간호전문직관이 진로정체감에 미치는 영향을 규명하기 위하여 수행된 서술적 조사연구이다. G시와 M시 대학의 간호학과에 재학하고 있는 간호대학생을 대상으로 2021년 7월부터 9월까지 자료를 수집하였다. 수집된 자료 중 198명의 자료를 분석에 이용하였고 분석방법으로는 기술 통계, 독립표본 평균 검정(t-test), 일원 배치 분산분석(ANOVA), 피어슨 상관계수, 통제회귀분석을 이용하였다. 자료분석 결과, 강점인식(β=.473, p<.001)과 간호전문직관(β=.167, p<.01)은 진로정체감에 정적인 영향을 미쳤으며 연구모형은 진로정체감을 48.2% 설명하는 것으로 확인되었다. 이러한 연구결과는 간호대학생의 진로정체감을 높이기 위해 강점인식과 간호전문직관을 촉진하기 위한 프로그램이 간호교육 현장에서 다양하게 개발 및 운영되어야 함을 시사한다고 할 수 있다.

• 천문학회지
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• 제8권1호
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• pp.29-34
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• 1975

Solar electrical conductivity has been calculated, making use of Yun and Wyller's formulation. The computed results arc presented in a tabulated form as functions of temperature and pressure for given magnetic field strengths. The results of the calculation show that the magnetic field does not play any important role in characterizing the electrical conductivity of the ionized gas when the gas pressure is relatively high (e.g., $P{\geq}10^4\;dynes/cm^2$). However, when the gas pressure is low (e.g., $P{\leq}10\;dynes/cm^2$), the magnetic field becomes very effective even if its field strength is quite small (e.g., $B{\leq}0.01$ gauss). It is also found that, except for lower temperature region (e.g., $T{\leq}10^{4^{\circ}}K$), there is a certain linear relationship in a log- log graph between the pressure and the critical magnetic field strength, which is defined as a field strength capable of reducing the non-magnetic component of the electrical conductivity by 20%.

• 한국전기전자재료학회:학술대회논문집
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• 한국전기전자재료학회 1998년도 춘계학술대회 논문집
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• pp.195-198
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• 1998

In this paper, we study on the surface breakdown of Epoxy composite in silicon oil. Breakdown field strengths were simulated by using FEM with the experience data of surface breakdown of Epoxy composite. The surface endurance and field distribution (kV/mm) of Epoxy composite were calculated by FEM.

• 대한전기학회:학술대회논문집
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• 대한전기학회 2001년도 추계학술대회 논문집 전기물성,응용부문
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• pp.216-218
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• 2001

This paper deals with the control of magnetic field around the down conductor of lightning protection systems. The magnetic field strength in the vicinity of down conductor is shown to drop off rapidly with distance from the down conductor and is reversely proportional to the number of down conductor. Also the magnetic field strength is decreased in the structures as the down conductor is installed with the symmetrical arrangement, and it is zero at the center of symmetry. The magnetic field strengths for the symmetrical arrangement of two down conductors are less than one half compared with that for a down conductor. A proper arrangement of down conductor can reduce or cancel the magnetic field in a restricted place where information-oriented and computerized facilities are densely installed.

• 콘크리트학회논문집
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• 제14권1호
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• pp.24-32
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• 2002

전단문제에서는 일부 설계기준(AASHTO 1994)에 이미 수정압축장이론이 도입되었다. 그리고 현행 콘크리트 설계기준에는 콘크리트의 전단강도가 철근의 전단강도와 합하여 공칭전단강도를 계산하고 있다. 그러나 최근에 개정된 콘크리트설계기준에는 콘크리트의 비틀림강도가 공칭비틀림강도 계산에서 누락되었다. 콘크리트의 인장응력은 비록 크기가 작으나 균열후에 균열사이의 콘크리트에 존재한다. 그러나 휨과 비틀림문제에서는 균열 후 콘크리트의 인장강성은 생략되고 있다. 역학적으로 콘크리트보의 비틀림거동은 전단거동과 매우 유사하다. 그러므로 균열 후 콘크리트의 비틀림강도를 철근콘크리트 보의 공칭비틀림강도의 계산에 포함시켜야 한다. 본 논문에서는 콘크리트의 평균주인장응력이 이루는 콘크리트의 비틀림강도를 횡방향 비틀림철근의 비틀림강도와 함께 공칭비틀림강도를 구성함을 밝혔으며, 이의 타당성을 검증하기 위해 개정 전후의 ACI 의 설계기준에 의한 공칭비틀림강도와 함께 실험값과 비교하였다. 그 결과 본 논문이 제안한 모델에 의한 공칭비틀림강도가 가장 좋은 결과를 보였다.

• 천문학회보
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• 제40권2호
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• pp.31.2-31.2
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• 2015

We present a near-infrared photometric and polarimetric catalog of sources in the $39^{\prime}{\times}69^{\prime}$ fields on the northeastern part of the Large Magellanic Cloud (LMC), which was observed using SIRPOL, an imaging polarimeter of the Infrared Survey Facility (IRSF). This catalog contains 1,858 sources brighter than 14 mag at H band with polarization signal-to-noise ratio greater than 3 in at least one of J, H, and Ks bands. We examined the polarization structures around the star-forming regions, where coherent polarization position angle distributions are seen. We also estimated magnetic field strengths in some selected fields using Chandrasekhar and Fermi analysis. The magnetic field strengths are estimated to be $3{\sim}25{\mu}G$. The wavelength dependence of polarization degrees indicates that the polarization is most likely to be originated from dichroic extinctions by the local interstellar dusts in the LMC. We found that the polarization patterns are well aligned along the molecular clouds around star-forming regions.