• 제목/요약/키워드: polar energy

검색결과 340건 처리시간 0.025초

대기압 플라즈마로 처리된 폴리프로필렌 필름의 표면 자유에너지 변화 (Surface Free Energy Change of Polypropylene Film treated by Atmospheric Pressure Plasma)

  • 권오준;탕쉰;루나;최호석
    • 접착 및 계면
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    • 제4권4호
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    • pp.1-6
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    • 2003
  • 대기압 플라즈마를 이용하여 폴리프로필렌 필름의 표면을 처리한 후 각각 극성 용매(water)와 비극성 용매(diiodomethane)를 사용한 접촉각 측정기로 필름 표면의 접촉각을 측정하였다. 측정된 접촉각을 이용해 표면 자유에너지 변화를 계산한 후 대기압 플라즈마 처리 전후의 폴리프로필렌 필름의 접촉각과 표면 자유에너지 상태를 비교, 분석하였다. 또한 대기압 플라즈마의 처리 조건을 바꿔가며 폴리프로필렌 필름 표면을 처리함으로써 접촉각과 표면 자유에너지가 각각의 처리 조건에 따라 어떠한 영향을 받는지 연구하였다. 대기압 플라즈마 처리 조건에 따라 접촉각 및 표면 자유에너지는 최적값을 보여주거나 일정한 값에 도달하는 경향을 보여 주었다.

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Estimation of Polar Cap Potential and the Role of PC Index

  • Moon, Ga-Hee
    • Journal of Astronomy and Space Sciences
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    • 제29권3호
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    • pp.259-267
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    • 2012
  • Polar cap potential has long been considered as an indicator for the amount of energy flowing in the magnetosphere-ionosphere system. Thus, the estimation of polar cap potential is important to understand the physical process of the magnetosphere. To estimate the polar cap potential in the Northern Hemisphere, merging electric field by Kan & Lee (1979) is adopted. Relationships between the PC index and calculated merging electric field ($E^*$) are examined during full-time and storm-time periods separately. For this purpose Dst, AL, and PC indices and solar wind data are utilized during the period from 1996-2003. From this linear relationship, polar cap potential (${\Phi}^*$) is estimated using the formula by Doyle & Burke (1983). The values are represented as $58.1{\pm}26.9$ kV for the full-time period and $123.7{\pm}84.1$ kV for a storm-time period separately. Considering that the average value of polar cap potential of Doyle & Burke (1983) is about 47 kV during moderately quiet intervals with the S3-2 measurements, these results are similar to such. The monthly averaged variation of Dst, AL, and PC indices are then compared. The Dst and AL indices show distinct characteristics with peaks during equinoctial season whereas the average PC index according to the month shows higher values in autumn than in spring. The monthly variations of the linear correlation coefficients between solar wind parameters and geomagnetic indices are also examined. The PC-AL linear correlation coefficient is highest, being 0.82 with peaks during the equinoctial season. As with the AL index, the PC index may also prove useful for predicting the intensity of an auroral substorm. Generally, the linear correlation coefficients are shown low in summer due to conductance differences and other factors. To assess the role of the PC index during the recovery phase of a storm, the relation between the cumulative PC index and the duration is examined. Although the correlation coefficient lowers with the storm size, it is clear that the average correlation coefficient is high. There is a tendency that duration of the recovery phase is longer as the PC index increases.

광전소자 응용을 위한 무극성 6H-SiC 기판의 특성 (Characterization of Non-polar 6H-SiC Substrates for Optoelectronic Device Applications)

  • 여임규;이태우;최정우;서정두;구갑렬;이원재;신병철;김영희
    • 한국전기전자재료학회논문지
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    • 제22권5호
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    • pp.390-396
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    • 2009
  • The present research was focused to investigate the quality of non-polar SiC substrates grown by a conventional PVT method for optoelectronic applications. The half part of the PVT-grown 6H-SiC crystal boules was sliced along a-direction and m-direction to extensively analyze non-polar planes and then remaining part of that was sliced along the basal plane to produce wafers. The non-polar SiC m-plane and a-plane exhibited apparent peaks around 2 theta=$120^{\circ}$((3-300) plane) and 2 theta=$60^{\circ}$ ((11-20) plane), respectively. FWHM values of m-plane measured along a-direction and c-direction were 60 arc see and 57 arcsec respectively, a-plane measured along m-direction and c-direction were 41 arcsec and 51 arcsec respectively. The typical absorption spectra of SiC crystals indicated that each of SiC crystals were the 6H-SiC with fundamental absorption energy of about 3.04 eV. Non-polar planes contained no micropipe on etched surface. The carrier concentration and mobility of non-polar SiC wafers have estimated by Raman spectrum. It was observed that the carrier mobility is low in the area far from seed crystal with compared to other places.

Rheological Consideration of Sub-micron Sized Hollow Polyaniline Malonate Salts Suspension under the Electric Field

  • Choi, Ung-Su
    • KSTLE International Journal
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    • 제8권1호
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    • pp.7-10
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    • 2007
  • The rheological property of hollow PANI malonate suspension in silicone oil was investigated by varying the electric fields and shear rates, respectively. The hollow PANI malonate susepnsion showed a typical electrorheological (ER) response caused by the polarizability of an amide polar group and shear yield stress due to the formation of chains upon application of an electric field. The shear stress for the hollow PANI malonate suspension exhibited an electric field power of 0.90. On the basis of the experimental results, the newly synthesized hollow PANI malonate suspension was found to be an anhydrous ER fluid.

MAGNETOSPHERIC STRUCTURE OF THE INTERMEDIATE POLAR

  • Kim, Yong-Gi
    • Journal of Astronomy and Space Sciences
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    • 제11권1호
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    • pp.1-12
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    • 1994
  • The structure of the magnetic funnel element in the intermediate polar is considered in terms of an important site for the X-ray absorption and the reemission of the X-ray as the optical light. In this paper the column density and the optical depth vary with the filling factor, which is introduced to characterize the structure of matter in the magnetic funnel element. The results of the energy dependence of the X-ray spectrum and the modulation depth of the X-ray light curve are discussed.

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이성분 용매 추출에 의한 미세조류로 부터의 바이오디젤용 지질 분리 (Extraction of Lipids from Microalgae Using Polar and Nonpolar Bi-solvent Systems)

  • 홍연기;김정배;잉사이먼
    • 한국태양에너지학회 논문집
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    • 제31권6호
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    • pp.66-71
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    • 2011
  • Various single solvents were tested to find the effective solvent for the extraction of algae oil from wet-form Chlorella minutissima. In the case of single solvents, their extractabilities for algae oil were increased with their polarity because the water in wet algae cell is to form a solvent shell around the lipids. Based on these results, the wet-form algae samples were treated with a polar alcohol solvent and then a nonpolar solvent was added in algae residue. In the algae oil extraction by ethanol/n-hexane, total lipid contents were 40-50% and composition of triglyceride in extracted oil was 46.50%. Considering solvent toxicity of conventional solvent mixture such as chloroform and methanol for algae oil extraction, the ethanol/n-hexane system was identified as the effective one for the oil extraction from wet-form Chlorella minutissima.

극축 회전을 이용한 태양광 추적 장치에 관한 연구 (Chronological solar tracking system using polar axis rotation)

  • 박태양;문창범;채상훈;김우영;채수조
    • 한국신재생에너지학회:학술대회논문집
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    • 한국신재생에너지학회 2009년도 춘계학술대회 논문집
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    • pp.61-64
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    • 2009
  • 본 논문에서는 단축과 2축 회전형추적시스템의 장점을 가진 시간 제어 극축회전형(Chronological Polar axis tracking) 태양광추적발전시스템에 대한 연구결과를 보여주고 있다. 천체 망원경의 별 추적 방식과 같은 시간 제어 극축 회전 방식으로 태양 추적방법의 정밀도를 높이면서 제어를 간소화하였고 계절 변화에 따른 태양 남중고도의 변화를 패널이 동시 추적 가능하도록 하였다. 향후 집광형태양광발전시스템에 적용가능성을 보였다.

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Excitation Processes of the CH4 Aurorae of Jupiter and Saturn

  • Kim, Sang Joon
    • 천문학회보
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    • 제43권1호
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    • pp.72.1-72.1
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    • 2018
  • Recently, an analysis of 3-micron spectra of CH4 line emission from our Gemini/GNIRS observations of Jupiter's polar regions yielded an unexpected result: The homopause (~1 microbar pressure level) located directly above the long-lasting 8-micron CH4 north-polar hot spot (Great 8-micron Hot Spot: GHS) is cool compared with the temperatures of nearby auroral regions (Kim et al. 2017). Most of the 8-micron emission of the GHS originates from CH4 at the ~1 mbar level (i.e., deeper in the stratosphere, where cooling time is several years), much longer than at the altitude of the homopause. We propose a mechanism to explain the temperature difference: locally-fixed and transient, but energetic auroral particles, which can penetrate to the 1 mbar level and deposit energy there creating and maintaining the GHS. For Saturn, thus far we have not detected distinctive 8-micron nor 3-micron CH4 hot spots in the polar regions. We will present a possible implication for this difference between Jupiter and Saturn.

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마찰 저감을 위한 비극성 첨가제에 따른 acrylonitrile butadiene styrene계 플라스틱의 stick-slip 이음 저감 연구 (Study on the reduction of stick-slip noise in acrylonitrile butadiene styrene-based plastics using non-polar additives to reduce friction)

  • 여상준;정예원;최성욱;김효준;박건욱;손민영
    • 한국음향학회지
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    • 제43권1호
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    • pp.49-59
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    • 2024
  • 최근 환경규제가 강화되고 고유가 문제로 인하여 전기차 시장이 점차 커지고 있으며 또한 내연기관 자동차에서도 엔진의 Noise, Vibration, Harshness(NVH) 관련 소음이 저감되고 외부에서 유입되는 소음의 차폐 기술이 발전됨에 따라 Buzz, Squeak, Rattle(BSR) 이음의 민감도가 증가하는 추세이다. 본 연구에서는 자동차의 Panoramic Curved Display(PCD)에서 발생하는 Stick-slip 이음과 고분자 플라스틱의 표면에너지 및 극성 성분과의 상관관계에 대하여 분석하였다. 극성 고분자 소재인 Acrylonitrile Butadiene Styrene(ABS)와 PolyCarbonate-Acrylonitrile Butadiene Styrene(PC-ABS)를 대상으로 컴파운드 소재를 제작하여 평가하였다. 결과적으로 고분자 플라스틱의 극성성분이 3.86 mN/m 이상일 때 Stick-slip 거동이 발생하였으며, 시간에 따른 마찰 거동에서 absolute transition slope가 증가할수록 Stick-slip의 이음 가능성이 증가하고 마찰계수의 값 차이가 클수록 Stick-slip 이음의 세기가 증가하였다.

극성 할로겐 탄화수소 화합물 물성 예측에 BWRS 상태 방정식의 응용 (Application of the BWRS equation of state of polar halocarbons)

  • 이태종;김부웅
    • 에너지공학
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    • 제2권3호
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    • pp.315-322
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    • 1993
  • 극성 할로겐 탄화수소 화합물의 정확한 물성예측을 얻고자 BWRS 상태 방정식의 일반화된 23개 상수를 각 물질에 대하여 최적화 하였다. Multiproperty analysis방법이 최적의 23개 상수를 구하는데 사용되었다. 각 물질의 최적 23개 상수값과 acentric factor 혹은 orientation parameter를 사용하여 물성 예측을 한 결과 O.A.A.D.는 밀도가 0.4%, 엔탈피가 0.33kcal/kg 그리고 증기압은 0.39%로 고찰하였다. 이 결과는 일반화된 23개 상수를 사용하여 얻은 물성예측 보다 월등히 향상된 결과를 보여준다.

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