• Journal of the Korean Wood Science and Technology
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• 제47권2호
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• pp.200-209
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• 2019

To improve the water resistance of melamine-urea-formaldehyde (MUF) resins, different levels of blocked polymeric 4,4 diphenyl methane diisocyanate (B-pMDI) were blended with MUF resins to prepare B-pMDI/MUF hybrid adhesives, and their adhesion performances were evaluated for the surface lamination of fancy veneer on plywood. FT-IR spectra showed that the de-blocked -NCO groups reacted with the -OH of hydroxymethyl groups of the MUF resins to form urethane bonds at 2% B-pMDI/MUF, which was detected before and after their hydrolysis. The mass loss after the hydrolysis consistently decreased as the B-pMDI level increased, indicating an improvement in the water resistance. As the B-pMDI level increased, the activation energy of hybrid adhesives decreased, which improved the reactivity of the hybrid adhesives. Additionally, the water resistance improvement of the hybrid adhesives increased the tensile shear strength of the surface laminated plywood in semi-water proof and water-proof by 23 % and 8 %, respectively, at 2% B-pMDI level. This was likely due to the urethane linkages in the hybrid adhesives. However, the formaldehyde emission from plywood panels bonded with the hybrid adhesives increased in the dry state, indicating incomplete curing of the hybrid adhesives.

• Journal of the Korean Wood Science and Technology
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• 제45권5호
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• pp.580-587
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• 2017

목섬유 단열재는 친환경 고단열성에 기인하여 저에너지 및 쾌적하고 안전한 주거 공간 형성을 위한 핵심 건축재료로 고려된다. 본 연구에서는 서로 다른 접착제로 제조한 단열재용 저밀도섬유판의 폼알데하이드(HCHO) 총휘발성유기화합물(TVOC) 방출 및 화염에 의한 연소 형상을 조사하였다. 멜라민 요소 폼알데하이드(MUF), 페놀 폼알데하이드(PF), emulsified methylene diphenyl diisocyanate (eMDI) 및 라텍스 수지 접착제 등으로 제조한 저밀도섬유판 4종의 HCHO TVOC 방출 특성 및 연소 형상은 각각 챔버법과 화염실험을 통하여 분석하였다. 그 결과 MUF, eMDI, 라텍스 수지 접착제로 제조한 저밀도섬유판들은 Super $E_0$급의 우수한 HCHO 저방출 성능을 나타냈다. 반면 PF 수지로 제조된 저밀도섬유판은 $E_0$급 성능을 나타내었다. TVOC 방출량은 모든 저밀도섬유판이 국내 실내공기질 기준(이하 $400{\mu}g/m^2{\cdot}h$)을 만족하였으며, 기존 석유계 합성원료 기반의 단열재보다 낮은 수치를 나타냈다. 그중에서도 특히 eMDI 수지 접착제로 제조한 경우에서는 HCHO 및 TVOC 방출량이 각각 $0.14mg/{\ell}$, $12{\mu}g/m^2{\cdot}h$로 가장 낮게 측정되었다. 그러나 eMDI로 제조한 저밀도섬유판에서 방출된 VOC의 성분을 조사한 결과, 톨루엔 성분($3{\mu}g/m^2{\cdot}h$)이 소량 검출되었다. 화염에 의한 연소시험에서는 MUF 수지 접착제로 제조한 저밀도섬유판이 다른 경우에 비하여 연소 후 비교적 가장 양호한 형상을 나타내었다. HCHO 및 TVOC 방출 특성, 연소 형상을 고려하였을 때 단열재용 저밀도섬유판은 MUF 수지 접착제가 가장 적합할 것으로 판단된다.

• 접착 및 계면
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• 제7권4호
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• pp.53-59
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• 2006

The paper highlights technical advances and introduces recent innovations such as smart curing laminating adhesives for flexible packaging with low migration rates of aromatic isocyanates and amines. Latent reactive one-part systems on the basis of surface deactivated solid isocyanates open up new dimensions for heat setting adhesives and waterborne PU dispersions. The new generation of Purmelt Micro Emission adhesives contains less than 0.1% of MDI monomer, thereby drastically reducing the emission of hazardous isocyanate vapors during processing and setting a significantly improved technical standard in occupational safety. Once again, polyurethane adhesives have demonstrated their unique ability to adapt to new process, product, safety and environmental requirements.

• Bulletin of the Korean Chemical Society
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• 제32권spc8호
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• pp.2988-2996
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• 2011

Shape memory polyurethane (SMPU), grafted with a fluorescent dye (Rhodamine, Mehylene violet, or Fluorescein) through an allophanate linking, was tested for the fluorescence and the shape recovery effect. The main chain of SMPU was composed of 4,4'-methylenebis(phenylisocyanate) (MDI), poly(tetramethyleneglycol) (PTMG), and 1,4-butanediol (BD), and a fluorescent dye was connected through a second MDI linked to the carbamate moiety of the main chain. Three series of SMPU, differing according to their dye content, were prepared to compare their shape recovery and fluorescence properties. In tensile mechanical property, maximum stress increased up to 350% compared to the linear SMPU, and strain remained above 2000%. Shape recovery went to as high as 97%, and remained almost same after repetitive shape recovery test cycles. Finally, the fluorescence emission of SMPU was demonstrated in the luminescence spectrum and fluorescent light emission pictures. In addition, the response of SMPU to external stimuli such as metal ions was investigated.

• 천문학회지
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• 제50권4호
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• pp.105-109
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• 2017

The well-known solar cycle controls almost the entire appearance of the solar photosphere. We therefore presume that the continuous emission of visible light from the solar surface follows the solar cyclic variation. In this study, we examine the solar cyclic variation of photospheric brightness in the visible range using solar images taken by the Solar and Heliospheric Observatory (SOHO)/Michelson Doppler Imager (MDI). The photospheric brightness in the visible range is quantified via the relative intensity acquired from in the raw solar images. In contrast to total solar irradiance, the relative intensity is out of phase with the solar cycle. During the solar minimum of solar cycles 23-24, the relative intensity shows enhanced heliolatitudinal asymmetry due to a positive asymmetry of the sunspot number. This result can be explained by the strength of the solar magnetic field that controls the strength of convection, implying that the emission in the visible range is controlled by the strength of convection. This agrees with the photospheric brightness increasing during a period of long spotless days.

• 천문학회보
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• 제35권1호
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• pp.27.2-27.2
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• 2010

We have studied the formation of coronal holes (CHs) associated with halo CMEs. For this study, we used multi-wavelength data from Yohkoh Soft X-ray Telescope (SXT), GOES Soft X-ray Imager (SXI), SOHO EIT 195 ${\AA}$, SOHO MDI magnetogram, MLSO He I 10830 ${\AA}$, and BBSO H-alpha. The CHs are characterized by open magentic field regions with low emission, density, and temperature and their open fields drive high speed solar winds which cause geomagnetic storms. So far, the formation and the evolution of CHs are not well understood. The formation of the dark region associated with the eruption of a CME is well known as "coronal dimming" which may be caused by the mass depletion near the CME footpoint. It is different from a typical CH since it persists for only one or two days. In this study, we present three cases that show the formation of coronal holes which are associated with three halo CMEs: 1) 2000 Jul 14, 2) 2003 Oct 28, 3) 2005 May 13. In the first case, hot plasma was ejected during a weak eruption and then filled out the pre-existing CH. After the halo CME occurred, the hot plasma region becomes a CH again. In the second and the third cases, we found newly formed CHs just after their associated CMEs. All three coronal holes are associated with strong flares and persist over 3 days until they disappeared by the solar rotation. Examining the MDI magnetograms, we found that the magnetic polarity of each CH region has one polarity. Based on these results, we suggest that the coronal holes can be formed by the CMEs and they should be distinguished from the coronal dimming.

• 공업화학
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• 제24권1호
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• pp.104-111
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• 2013

본 연구에서는 생분해성 지방족 폴리에스터 중 비교적 고가인 poly(butylene adipate-co-terephthalate) (PBAT)와 상대적으로 저가의 생분해성 고분자인 polylactic acid (PLA)의 블렌드에 3종류의 개질제를 사용하여 그 효과를 조사하였다. 개질제로는 에폭시계의 커플링제와 diisocyanate계열의 methylenediphenyl 4,4'-diisocyanate (MDI)와 hexamethylene diisocyanate (HDI)를 사용하였다. 여러 가지 조성의 블렌드에 용융흐름지수, 동적 점탄성을 조사하였다. 또한, 인장시험을 통한 기계적 물성 조사와 FE-SEM으로 시편의 파단표면을 관찰하였다. 이를 통해 PLA/PBAT 블렌드의 상용성과 개질제의 효과 및 기계적물성에 미치는 영향을 고찰하였다. 개질제로 HDI를 사용했을 때 PLA/PBAT의 인장물성이 크게 증가하였다.

• 천문학회보
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• 제35권1호
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• pp.28.2-28.2
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• 2010

We have investigated seven Extreme-Ultraviolet (EUV) bright points in the active region (AR 10926) on 2006 December 2 by the EUV imaging spectrometer (EIS) onboard Hinode spacecraft. We determined their Doppler velocities and non-thermal velocities from 15 EUV spectral lines (log T=4.7-7.2) by fitting each line profile to a Gaussian function. We present the Doppler velocity map as a function of temperature which corresponds to a different height. As a result, these active region bright points show two different types of characteristics. Type 1 bright point shows a systematic increase of Doppler velocity from -68 km/s (blue shift) at log T=4.7 to 27 km/s (red shift) at log T=6.7, while type 2 bright points have Doppler velocities in the range of -20 km/s and 20 km/s. Using MDI magnetograms, we found that only type 1 bright point was associated with the canceling magnetic feature at the rate of $2.4{\times}10^{18}$ Mx/hour. When assuming that these bright points are caused by magnetic reconnection and the Doppler shift indicates reconnection out flow, the pattern of the Doppler shift implies that type 1 bright point should be related to low atmosphere magnetic reconnection. We also determined electron densities from line ratio as well as temperatures from emission measure loci using CHIANTI atomic database. The electron densities of all bright points are comparable to typical values of active regions (log Ne=9.9-10.4). For the temperature analysis, the emission loci plots indicate that these bright points should not be isothermal though background is isothermal. The DEM analysis also show that while the background has a single peak distribution (isothermal), the EUV bright points, double peak distributions.

• Journal of the Korean Wood Science and Technology
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• 제33권3호통권131호
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• pp.22-29
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• 2005

이 연구는 숯파티클 크기에 따른 최종 매트 함수율에 관한 백탄보드의 적정제조조건을 규명할 뿐 아니라 백탄보드가 새집증후군에 대한 친환경적 재료로서 백탄의 유익한 성질을 그대로 유지하도록 하기 위하여 수행되었다. 우수한 기능성을 갖는 백탄보드는 최종매트함수율이 20~25%와 36~60%의 2개 그룹에서 생산되었다. 최종매트함수율이 높은 후자는 훨씬 우수한 결과를 나타내었고 비포름알데히드계 접착제[MDI(M), poly vinyl acetate emulsion(P)]와 30-10-$3kgf/cm^2$ (1분-1.5분-6분)의 3단계 열압공정으로 제조된 #40~60형-P15%, M5%, FMC60%와 혼합형-P15%, 5%, FMC36%의 2 종류였다. 숯파티클이 큰 쪽은 최종매트함수율이 적게 필요하였고 #6이상-M15%, FMC25%와 혼합형-M25%, FMC20%의 2 종류가 전자에 속하였다. 백탄보드는 치수안정성, 가스흡착 그리고 원적외선방사율에서 우수한 결과를 나타내었다.