• 제목/요약/키워드: low mass flux

검색결과 166건 처리시간 0.033초

수평미세관내 R-290의 비등열전달 특성 (Boiling Heat Transfer Characteristics of R-290 in Horizontal Smooth Minichannel)

  • 최광일;;오종택
    • 설비공학논문집
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    • 제18권11호
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    • pp.906-914
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    • 2006
  • The present paper dealt with an experimental study of boiling heat transfer characteristics of R-290. Pressure gradient and heat transfer coefficient of the refrigerant flow inside horizontal smooth minichannel were obtained with inner tube diameter of 3.0 mm and length of 2,000 mm. The direct electric heating method was applied for supplying a heat to the refrigerant uniformly. The experiments were conducted with R-290 purity of 99.99%, at saturation temperature of 0 to $10^{\circ}C$, a mass flux range of $50{\sim}250kg/m^2s$, and a heat flux range of $5{\sim}20kW/m^2$. The heat transfer coefficients of R-290 increased with increasing mass flux and saturation temperature, wherein the effect of mass flux was higher than that of the saturation temperature. Heat flux has a low effect on the increasing of heat transfer coefficient. The heat transfer coefficient was compared with six existing heat transfer coefficient correlations. The Zhang et al.'s correlation (2004) gave the best prediction of heat transfer coefficient. A new correlation to predict the two-phase flow heat transfer coefficient was developed based on the Chen correlation. The new correlation predicted the experimental data well with a mean deviation of 11.78% and average deviation of -0.07%.

공조용 알루미늄 납작관 내의 R-410A 대류 비등 (Convective Boiling of R-410A in an Aluminum Flat Tube for Air-Conditioning Application)

  • 김내현
    • 한국산학기술학회논문지
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    • 제16권5호
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    • pp.3006-3013
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    • 2015
  • 원관 열교환기보다 납작관 열교환기를 사용하면 전열성능을 한층 향상시킬 수 있다. 납작관 열교환기를 적절히 설계하기 위해서는 관 내측 열전달계수를 알아야 한다. 본 실험에서는 수력직경 1.41mm인 알루미늄 납작관 내 R-410A 대류 비등 열전달계수를 구하였다. 실험범위는 질량유속 $200{\sim}600kg/m^2s$, 열유속 $5{\sim}15kg/m^2$, 포화온도 $5{\sim}15^{\circ}C$이다. 실험 결과 열전달계수는 임계 건도를 기점으로 감소함을 보였다. 임계 건도는 열유속이 증가할수록 감소하고, 질량유속이 감소할수록 감소하였다. 이는 높은 열유속 또는 낮은 질량유속에서 대류의 영향이 작게 되고 따라서 조기에 dryout이 발생되기 때문에 나타나는 현상으로 판단된다. 열전달계수는 질량유속이 증가할수록 증가하였다. 그러나 낮은 건도에서는 질량유속의 영향은 미미하였다. 열전달계수는 포화온도가 증가할수록 증가하였다. 하지만 이런 경향은 열유속이 작아지면 감소하였다. Shah와 Kaew-On et al. 상관식은 본 실험자료를 적절히 예측하였다.

2016년 1월 23일~25일에 발생한 서해안 대설 발달 메커니즘 분석 (Analysis of the West Coast Heavy Snowfall Development Mechanism from 23 to 25 January 2016)

  • 이재근;민기홍
    • 대기
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    • 제28권1호
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    • pp.53-67
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    • 2018
  • This study examined the lake effect of the Yellow Sea which was induced by the Siberian High pressure system moving over the open waters. The development mechanism of the convective cells over the ocean was studied in detail using the Weather Research and Forecasting model. Numerical experiments consist of the control experiment (CTL) and an experiment changing the yellow sea to dry land (EXP). The CTL simulation result showed distinct high area of relative vorticity, convergence and low-level atmospheric instability than that of the EXP. The result indicates that large surface vorticity and convergence induced vertical motion and low level instability over the ocean when the arctic Siberian air mass moved south over the Yellow Sea. The sensible heat flux at the sea surface gradually decreased while latent heat flux gradually increased. At the beginning stage of air mass modification, sensible heat was the main energy source for convective cell generation. However, in the later stage, latent heat became the main energy source for the development of convective cells. In conclusion, the mechanism of the west coast heavy snowfall caused by modification of the Siberian air mass over the Yellow Sea can be explained by air-sea interaction instability in the following order: (a) cyclonic vorticity caused by diabatic heating induce Ekman pumping and convergence at the surface, (b) sensible heat at the sea surface produce convection, and (c) this leads to latent heat release, and the development of convective cells. The overall process is a manifestation of air-sea interaction and enhancement of convection from positive feedback mechanism.

저 산화제유속 구간에서의 HDPE 및 Paraffin 연료의 연료농후가스 O/F비 특성 (Fuel Rich Gas O/F Ratio Characteristics of HDPE and Paraffin Fuel in Low Range of the Oxidizer Mass Flux)

  • 한승주;류성훈;김진곤;강태곤;문희장;김준형;고승원
    • 한국추진공학회지
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    • 제20권6호
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    • pp.54-60
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    • 2016
  • 본 연구에서는 하이브리드 추진시스템의 덕티드 로켓용 가스발생기 적용을 위하여 낮은 산화제 유속 범위에서 HDPE multi-port(7port) 그레인 및 파라핀 그레인을 이용한 연소 시험을 수행하였다. 파라핀 연료의 경우 일반적인 덕티드 로켓용 가스발생기의 O/F비 작동조건인 0.3~0.8의 범위를 충족시켜 덕티드 로켓용 가스발생기로서의 적용가능성을 확인하였다. 산화제 유속 $35kg/m^2s$ 이하의 구간에서 산화제유속에 따른 O/F비의 변화가 일어나지 않는 구간이 존재함을 확인함으로써 VFDR 가스발생기로서의 적용가능성 또한 확인할 수 있었다.

수평 다채널 관에서의 유동 비등 열전달 특성에 관한 연구 (Study on Characteristics of Flow Boiling Heat Transfer in Multi channels)

  • 최용석;임태우
    • 수산해양교육연구
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    • 제27권5호
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    • pp.1310-1317
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    • 2015
  • Two-phase flow boiling heat transfer in micro-channels was experimently investigated. The test section consisted of 15 rectangular micro-channels with a depth of 0.45mm, width of 0.20mm. The experiments were performed for heat fluxes ranging from 5.6 to 46.1kW/m2 and mass fluxes from 150 to 450kg/m2s using FC-72 as the working fluid. According to the results, at the low heat flux region, heat transfer coefficient strongly depends on the heat flux, while heat transfer coefficient at the high heat flux region was independent on the heat flux. Four correlations were used to predict the heat transfer coefficient. The measured heat transfer coefficient was compared with four correlations. It was found that Kaew-On and Wongwises's correlation well predicted the measured data, within the MAE of 40.3%.

수평 다채널에서의 열전달 계수에 관한 새로운 상관식 (A New Correlation on Heat Transfer Coefficient in Horizontal Multi Channels)

  • 최용석;임태우
    • 수산해양교육연구
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    • 제28권5호
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    • pp.1388-1394
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    • 2016
  • This paper presents a experimental study of two-phase flow boiling of FC-72 in multi channels. Flow boiling heat transfer coefficients are obtained with mass flux ranging from 152.9 to $353.9kg/m^2s$ and heat flux from 5.6 to $46.1kW/m^2$. The experimental results show that the heat transfer is governed by nucleate boiling mechanism in the low heat flux region. However, it is found that the effects of nucleate boiling and forced convection boiling are combined as the heat flux increases. A new correlation to predict the heat transfer coefficient is developed by using the dimensionless number such as Reynolds number, Weber number, boiling number. This correlation shows good predictive accuracy against the measured data.

신작동매체를 이용한 헬리컬 흡수기의 열물질전달 특성 (Characteristic of Heat and Mass Transfer on Helical Absorber Using New Working Fluid)

  • 권오경;임종극;윤정인
    • 대한기계학회:학술대회논문집
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    • 대한기계학회 2000년도 춘계학술대회논문집B
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    • pp.228-233
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    • 2000
  • An experimental study has been performed regarding heat and mass transfer in a falling film absorber of domestic small-sized absorption chiller/heater. Components were concentrically arranged in cylindrical form : from the center, with a series of low temperature generator, absorber and evaporator. The arrangement of such helical-typed heat exchangers allows to make the system more compact as compared to conventional one. Experimental measurements were conducted with a helical absorber using $LiBr+LiI+LiNO_3+LiCl$ and LiBr solutions. As a result, the heat and mass flux performance of $LiBr+LiI+LiNO_3+LiCl$ solution shows the tendency of $2{\sim}5%$ increase. Therefore, $LiBr+LiI+LiNO_3+LiCl$ solution can be taken consideration into applying to small-sized absorption chiller/heater because of using without crystal through high concentration as 4wt% comparing with LiBr solution.

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The Evolution of the Mass-Metallicity Relation at 0.20 < z < 0.35

  • Chung, Jiwon;Rey, Soo-Chang;Sung, Eon-Chang
    • Journal of Astronomy and Space Sciences
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    • 제30권1호
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    • pp.59-67
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    • 2013
  • We present a spectroscopic study of 343 blue compact galaxies (BCGs) at 0.20 < z < 0.35 from the Sloan Digital Sky Survey (SDSS) DR7 data. We derive gas phase oxygen abundance using the empirical and direct method. Stellar masses of galaxies are derived from the STARLIGHT code. We also derive star formation rates of galaxies based on $H{\alpha}$ emission line from the SDSS as well as far-ultraviolet (FUV) flux from the Galaxy Evolution Explorer GR6 data. Evolution of the luminosity-metallicity and mass-metallicity (M-Z) relations with redshift is observed. At a given luminosity and mass, galaxies at higher redshifts appear to be biased to low metallicities relative to the lower redshift counterparts. Furthermore, low mass galaxies show higher specific star formation rates (SSFRs) than more massive ones and galaxies at higher redshifts are biased to higher SSFRs compared to the lower redshift sample. By visual inspection of the SDSS images, we classify galaxy morphology into disturbed or undisturbed. In the M-Z relation, we find a hint that morphologically disturbed BCGs appear to exhibit low metallicities and high SSFRs compared to undisturbed counterparts. We suggest that our results support downsizing galaxy formation scenario and star formation histories of BCGs are closely related with their morphologies.

낮은 유량에서 외경 7.0 mm 마이크로핀 튜브 내 R-410A 증발 열전달 및 압력 손실 (Evaporation Heat Transfer and Pressure Drop of R-410A in a 7.0 mm O.D. Microfin Tube at Low Flow Rates)

  • 김내현
    • 대한기계학회논문집B
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    • 제39권9호
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    • pp.761-772
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    • 2015
  • 가정용 에어컨이나 히트 펌프에 외경 7.0 mm 마이크로핀 튜브가 널리 사용되고 있다. 한편 에어컨이나 히트펌프의 부분 부하 운전시 질량유속은 수십 $kg/m^2s$에 불과하다. 하지만 7.0 mm 튜브에 대한 기존 연구들은 질량유속 $100kg/m^2s$ 이상에서 수행되었다. 본 연구에서는 낮은 질량유속 ($50kg/m^2s$에서 $250kg/m^2s$)에서 외경 7.0 mm 마이크로핀 튜브 내 R-410A 증발 열전달 실험을 수행하였다. 실험 중 포화온도는 $8^{\circ}C$, 열유속 $4.0kW/m^2$으로 유지하였다. 비교를 위해 외경 7.0mm 평활관에 대한 실험도 수행하였다. 실험결과 마이크로핀 튜브의 전열촉진비는 질량유속이 감소할수록 증가하다 $150kg/m^2s$를 기점으로 감소함을 보였다. 이는 마이크로 핀튜브 내 유동이 환상류에서 성층류로 변화하기 때문이다. 실험 범위에서 마이크로핀 튜브의 마찰손실과 평활관의 마찰손실은 거의 같게 나타났다. 실험데이터를 기존 상관식의 예측치와 비교하였다.

Experimental study of the frost formation on the cryogenic flat plate with temperature distribution

  • Fujimatsu, Kiyoto;Tanatsugu, Nobuhiro;Sato, Tetsuya
    • 한국추진공학회:학술대회논문집
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    • 한국추진공학회 2004년도 제22회 춘계학술대회논문집
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    • pp.657-664
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    • 2004
  • In this study, a fundamental experiment was carried out to investigate the frost formation on a cryogenic flat plate with/without temperature distribution from 230K to 160K under the convective flow. The effects of mixing ethanol as a condensable substance were also researched. From the test results, when surface temperature at the upstream is 230K, mass flux is high. On the other hand, when surface temperature at the downstream is 160K, mass flux is low. The degree of improvement to restrain frost formation by ethanol mixing is relatively larger at the upstream than at the downstream.

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