• Tribology and Lubricants
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• 제14권4호
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• pp.108-113
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• 1998

In order to investigate the characteristics of top ring groove deposit formation in diesel engine, engine test and simulation test were performed. From component analysis of used oils sampled from actual running engines, soot content in engine oil was selected as a main parameter for evaluating oil degradation. Deposit formation is highly related to soot content in lubricating oils. And high soot content oil accelerates deposit formation even in low temperature region below 26$0^{\circ}C$. In low temperature region below 26$0^{\circ}C$, deposit formation rate is mainly affected by top ring groove temperature. However, in high temperature region above 26$0^{\circ}C$, deposit formation rate is affected by soot content as well as top ring groove temperature. Therefore, soot content as well as top ring groove temperature should be kept a certain level in order to prevent troubles due to carbon deposit formation.

• 천문학회보
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• 제38권1호
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• pp.31.2-31.2
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• 2013

We use grid-based hydrodynamic simulations to study star formation in nuclear rings in barred galaxies. The gaseous medium is assumed to be infinitesimally thin, isothermal, and unmagnetized. To investigate various situations, we vary the total gas content in the bar regions and the bar growth time. We find that star formation rate (SFR) in a nuclear ring is determined by the mass inflow rate to the ring rather than the total gas mass in the ring. The SFR shows a strong primary burst and weak secondary bursts at early time, and declines to small values at late time. The primary burst is caused by the rapid gas infall to the ring due to the bar growth, with its duration and peak depending on the bar growth time. The secondary bursts result from re-infall of the ejected gas by star formation feedback of the primary burst. When the SFR is low, ages of young star clusters exhibit an azimuthal gradient along the ring since star formation takes place mostly near the contact points between the dust lanes and the nuclear ring. When the SFR is large, on the other hand, star formation is widely distributed throughout the whole length of the ring, with no apparent age gradient of star clusters. Regardless of SFR, star clusters have a positive radial age gradient, with younger clusters located closer to the ring, since the ring shrinks in size over time.

• 대한기계학회논문집A
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• 제28권10호
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• pp.1492-1499
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• 2004

In this paper, defect formation in ring rolling is revealed by computer simulation of ring rolling processes. The rigid-plastic finite element method is employed for this study. An analysis model having relatively fine mesh system near the roll gap is used for reducing the computational time and a scheme of minimizing the volume change is applied. The formation of the central cavity formation defect in ring rolling of a taper roller bearing outer race and the polygonal shape defect in ring rolling of a ball bearing outer race has been simulated. It has been seen that the results are qualitatively good with actual phenomena.

• Tribology and Lubricants
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• 제13권4호
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• pp.33-39
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• 1997

In order to establish a new temperature criterion to prevent the pistons from ring sticking due to deposit formation, bench test and engine test were performed. The effects of oil degradation and temperature on deposit formation was studied by a modified panel coking test. Oil degradation was analyzed by FTIR. Oil oxidation and nitration were selected as a factors to evaluate oil degradation. Bench test results show that oil oxidation is more effective to the deposit formation than oil nitration. And the temperature increase accelerates deposit formation and deposit formation increase rapidly above 26$0^{\circ}C$. Especially, in case of degraded oil, the deposit formation increases so rapidly that ring sticking can occur. The effect of piston temperature on the deposit formation was confirmed by engine test.

• 터널과지하공간
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• 제16권1호
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• pp.38-49
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• 2006

복공식 LNG 지하저장기지 건설을 위해서는 암반역학, 열역학 및 수리지질특성과 관련된 여러 가지 기술이 요구되며, 이러한 기술의 적용성을 입증하기 위한 일환으로 대전에 Pilot cavern을 건설하였다. 이 논문에서는 Pilot cavern에 적용된 기술 중 배수시스템 평가과 Ice ring모사에 관한 수치해석 연구를 수행하였다. 대수층관점의 Modflow와 유동시스템 관점의 Seep/W 해석을 통해 적용된 배수시스템이 효율적으로 작용하였음을 확인하였다. Ice ring 형성은 열전달과 지하수 흐름의 상호작용을 통해 모사될 수 있는데, 이에 대한 모사를 위해 Temp/W-Seep/W 프로그램을 이용한 냉열수리 연동해석을 수행하였다. 이러한 해석을 통해 Ice ring의 형성 위치를 추정 할 수 있었고, Ice ring형성에 지하수 유동 속도 및 방향이 영향을 크게 미친다는 것을 확인했다.

• 한국연소학회:학술대회논문집
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• 한국연소학회 2014년도 제49회 KOSCO SYMPOSIUM 초록집
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• pp.339-342
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• 2014

Rotary kiln produces lime from limestone through thermal decomposition. Ring formation in kiln internal wall is known issue that decreases productivity. The cause of ring formation is temperature imbalance as flame leans toward upper wall. Therefore, burner nozzle geometry was changed to improve air-fuel mixing state which leads to prevention of ring formation. CFD simulation and experimental test were performed in this study to investigate the effect of air-fuel mixing on flame structure, temperature and $NO_X$ concentration. It is shown that combustion efficiency has been enhanced and $NO_X$ concentration has been decreased by using swirl flow for secondary combustion air. It's also shown that flame has been straightened by using straight flow for secondary combustion air.

• 천문학회보
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• 제38권2호
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• pp.39.2-39.2
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• 2013

We use grid-based hydrodynamic simulations to study star formation history in nuclear rings of barred-spiral galaxies. In our previous study, we concentrated on bar-only galaxies without spirals, finding that the star formation rate (SFR) in a nuclear ring exhibits a strong primary burst at early time before decreasing to below 1 $M_{\odot}/yr$ at late time. The rapid decline is caused by the paucity of the gas in the bar region, due to early massive gas inflows to the nuclear ring. Since star formation in nuclear rings is observed to be sustained for about 1-2 Gyr, this requires mechanisms to supply the gas to the bar regions. In this work, we study the effect of spiral arms on the radial gas inflows and related star formation in the nuclear rings. We show that spiral arms are efficient to remove angular momentum of the gas to cause significant gas inflows to the bar region, provided the patten speed of the arms is much smaller than that of the bar. The inflowing gas is added to a nuclear ring, making the ring SFR episodic over a long period of time. The time interval of multiple bursts of star formation is a few tens to hundred million years, with the mean peak SFR of ${\sim}5M_{\odot}/yr$, consistent with observations of M100.

• 천문학회보
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• 제44권1호
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• pp.34.1-34.1
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• 2019

To study the formation and evolution of stellar bars and gaseous nuclear rings in barred galaxies in realistic environments, we run fully self-consistent three-dimensional simulations of isolated disk galaxies. We consider two groups of models with cold or warm disks that differ in the radial velocity dispersion. We also vary the gas fraction of the disks. We found that a bar forms earlier and more strongly as the gas fraction increases in the cold disks, while the gas delays the bar formation in the warm disks. The bar formation enhances a central mass concentration which in turn weakens the bar strength temporarily, after which the bar regrows to become stronger in a model with a smaller gas fraction in both cold and warm disks. Although all bars rotate fast in the beginning, they rapidly turn to slow rotators. Gas infalling to the central region forms a dense star-forming nuclear ring. The ring size is very small when it first forms and grows over time. The ring star formation is episodic and bursty due to star formation feedback, and has a good correlation with the mass inflow rate to the ring. Some expanding shells produced by star formation feedback are sheared out in the bar regions and collide with dust lanes to appear as filamentary interbar spurs.

• 터널과지하공간
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• 제16권3호
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• pp.241-250
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• 2006

LNG지하저장 핵심기술 중 하나인 ice ring 형성을 열-수리 역학 해석을 통해 분석하였다. ice ring은 극저온물질의 누출에 대한 이차방벽 역할과 지하수의 저장공동 침투에 대한 일차방벽역할을 수행한다. 따라서 ice ring의 두께와 위치는 콘크리트와 PU foam 및 멤브레인으로 구성된 일차방호재의 무결성 유지에 있어서 핵심인자가 된다. 수치해석을 통해 이러한 ice ring의 위치와 두께를 추정하였으며 온도와 지하수위 결과를 계측치와 비교하였다. 수치해석결과는 PU foam 열전도도의 온도의존성과 지하수의 상변화를 고려한 경우 파일럿 공동에서 측정한 계측치와 잘 일치하였다. 본 논문에서 제시한 수치해석 기법은 실규모 저장시설의 설계에 있어서 ice ring 형성을 모델링하는 데에 바로 사용될 수 있을 것으로 판단된다.

• 한국정보통신학회논문지
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• 제7권2호
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• pp.201-207
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• 2003

일반적으로 블루투스 기술은 기기들이 한의 중심기기에 7개의 보조기기가 연결된 소형 네트워크를 피코넷 구성하게 하는 통신규약을 의미한다. 스캐터넷은 피코넷과 피코넷 간의 통신으로 이루어져 있다. 스캐터넷의 형태로는 트리와 링 형태가 있다. 그리고 링 형태가 모바일 환경에 더욱 적합하다고 한다. 본 노문은 트리와 링 구조의 성능을 비교 분석하여 어떤 형태가 모바일 환경에 적합한지를 알아보았다. 성능 측정은 단말기들이 빈번하게 추가 삭제되는 모바일 환경에서 스캐터넷 형성 알고리즘을 분석하여 스캐터넷 형성시간을 비교하였다. 실험 결과는 노드 수의 증가에 따라 트리 구조보다는 링 구조가 스캐터넷 형성 시간이 빠르고 시간의 차이의 폭이 넓어졌다.