• 제목/요약/키워드: passive scalar

검색결과 23건 처리시간 0.02초

Direct numerical simulation of passive scalar in decaying compressible turbulence

  • Li Xinliang;Fu Dexun;Ma Yanwen
    • 한국전산유체공학회:학술대회논문집
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    • 한국전산유체공학회 2003년도 The Fifth Asian Computational Fluid Dynamics Conference
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    • pp.39-41
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    • 2003
  • n this paper, direct numerical simulation of decaying compressible turbulence with passive scalar is performed by using 7th order upwind difference scheme or 8th order group velocity control scheme. The start Reynolds number (defined by Taylor scale) is 72 and turbulent Mach numbers are 0.2-0.9. The Schmidt numbers of passive scalar are 2-10. The Batchelor k-1 range are found in scalar spectra, and the high wavenumber spectra decays faster with increasing turbulent Mach number. The extend self-similarity (ESS) is found in the passive scalar in compressible turbulence.

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미소 채널의 형상변화에 의한 혼합효율에 관한 수치 해석적 연구 (Numerical Analysis on Mixing Efficiency in a Micro-channel with Varied Geometry)

  • 윤준용;한규석;변성준
    • 공업화학
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    • 제16권2호
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    • pp.275-281
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    • 2005
  • 본 연구에서는 격자 볼츠만 방법 중 Scalar Passive 코드를 사용하여 미소채널 내에서의 수동형 믹서의 혼합에 대하여 계산을 수행하였다. 미소채널 내에서의 수동형 믹서의 혼합에 대하여 유선과 압력분포를 통해 혼합과 압력 강하를 물리적으로 규명하였으며, 혼합에 영향을 주는 인자에 대해서 알아보았다. 수동형 믹서의 경우 고정물의 간격보다는 고정물의 개수와 고정물의 크기가 혼합효율과 압력강하에 큰 영향을 주었다.

The fate of an infalling circumgalactic gas clump and the growth of the central massive black hole in a high-redshift quasar

  • Jo, Yongseok;Kim, Ji-hoon
    • 천문학회보
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    • 제45권1호
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    • pp.35.1-35.1
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    • 2020
  • Since the discovery of SMBHs at z > 6, the growth spurt of a BH in a relatively short time—a few hundred Myr—has been a challenging topic for many observers and theorists. Super-Eddington accretion, major and minor merger have been compelling candidate machanisms to account for such growth. We introduce a passive scalar field to trace the infalling of circumgalactic gas clump onto high-z quasar. With the scalar field, we investigate e.g. where the most of the gas clump eventually reside in the host galaxy and how much gas is accreted onto the central massive black hole. In addition, we have studied the impact of thermal feedback of stars on the growth of black hole and the infalling gas. We will also discuss the future application of passive scalar field in e.g. minor and major mergers of high-z quasar.

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대와류모사 기법을 이용한 강한 벽분사가 있는 채널 내에서의 난류 유동장 및 온도장 해석 (Large Eddy Simulation of Turbulent Passive Scalar in a Channel with Strong Wall Injection)

  • 김학종;나양
    • 대한기계학회논문집B
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    • 제28권6호
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    • pp.628-637
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    • 2004
  • The present study investigates the performance of dynamic mixed model (DMM; Zang et ai.) in a channel with strong wall injection through a Large eddy simulation (LES) technique. The DMM results are compared with those of DNS and the results obtained with popular dynamic Smagorinsky model (DSM). Better agreement is achieved when using the DMM with box filter than DSM and coarse DNS in predicting the first and second order statistics as well as large-scale structures of velocity and temperature fields. Such favorable features of DMM are attributed to the fact that it explicitly calculates the modified Leonard stress term and only models the remaining cross and the SGS Reynolds stress terms and, thus, it reduces the excessive burden put on the model coefficient of DSM. Also it is demonstrated that the DMM can be successfully extended to the prediction of temperature (passive scalar) field where strong streamwise inhomogeneity exists.

On the Large Eddy Simulation of Scalar Transport with Prandtl Number up to 10 Using Dynamic Mixed Model

  • Na Yang
    • Journal of Mechanical Science and Technology
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    • 제19권3호
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    • pp.913-923
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    • 2005
  • The dynamic mixed model (DMM) combined with a box filter of Zang et. al. (1993) has been generalized for passive scalar transport and applied to large eddy simulation of turbulent channel flows with Prandtl number up to 10. Results from a priori test showed that DMM is capable of predicting both subgrid-scale (SGS) scalar flux and dissipation rather accurately for the Prandtl numbers considered. This would suggest that the favorable feature of DMM, originally developed for the velocity field, works equally well for scalar transport problem. The validity of the DMM has also been tested a posteriori. The results of the large eddy simulation showed that DMM is superior to the dynamic Smagorinsky model in the prediction of scalar field and the model performance of DMM depends to a lesser degree on the ratio of test to grid filter widths, unlike in the a priori test.

LES기법을 이용한 벽면 분출이 있는 채널 내부의 난류 유동 및 스칼라장 특성 해석 (Analysis on Turbulent Scalar Field in a Channel with Wall Injection using LES Technique)

  • 나양
    • 한국추진공학회지
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    • 제13권2호
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    • pp.54-63
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    • 2009
  • 이상화된 하이브리드 로켓모터 내부의 난류 유동 및 온도장의 발달과정을 대와류모사 기법을 사용하여 살펴보았다. 화학반응 및 밀도의 변화를 고려하지는 않았으나, 물리적으로 타당한 난류 입구조건과 22,500의 높은 Reynolds수 및 regression에 의한 벽면분출을 고려하여, 벽면근처에서 일어나는 난류유동의 시간 특성을 파악하였다. 하이브리드 모터 내부에서 발생한 혼합전단층의 불안정성에 기인한 특정 시간스케일(St~0.5)이 수동스칼라장에서 검출되지 않았다는 사실은 난류 온도장 해석에 난류 Prandtl 수를 상수로 가정하는 기존의 접근방식이 상당한 오차를 발생시킬 수 있다는 것을 의미한다.

동적혼성 모델을 이용한 난류채널의 온도장 해석 (On the Large Eddy Simulation of Temperature Field Using Dynamic Mixed Model in a Turbulent Channel)

  • 이건호;나양
    • 대한기계학회논문집B
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    • 제28권10호
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    • pp.1255-1263
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    • 2004
  • An a priori test has been conducted for the dynamic mixed model which was generalized for the prediction of passive scalar field in a turbulent channel flow The results from a priori tests indicated that dynamic mixed model is capable of predicting both subgrid-scale heat flux and dissipation rather accurately. The success is attributed to the explicitly calculated resolved term incorporated into the model. The actual test of the model in a LES a posteriori showed that dynamic mixed model is superior to the widely used dynamic Smagorinsky model in the prediction of temperature statistics.

전산유체역학 기법을 이용한 공기연령 산정 방법의 개발 (Development of Straightforward Method of Estimating LMA and LMR using Computational Fluid Dynamics Technology)

  • 박세준;이인복;홍세운;권경석;하태환;윤남규;김형권;권순홍
    • 한국농공학회논문집
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    • 제55권6호
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    • pp.135-144
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    • 2013
  • Ventilation efficiency has an important role in agricultural facilities such as greenhouse and livestock house to keep internally optimum environmental condition. Age-of-air concept allows to assess the ventilation efficiency of an agricultural facility according to estimating the ability of fresh air supply and contaminants emission using LMA and LMR. Most of these methods use a tracer gas method which has some limitations in experiment like dealing unstable and invisible gas. Therefore, the aim of this study was to develop a straightforward method to calculate age-of-air values with CFD simulation which has the advantage of saving computational time and resources and these method can solve the limitations in experiment using tracer gas method. The main idea of LMA computation is to solve the passive scalar transport equation with the assumption that the production of the time scalar throughout the room is uniform. In case of LMR calculation, the transport of the time scalar was reversed compulsively using UDF. The methodology to validate the results of this study was established by comparing with preceding research that had performed a computing LMA and LMR value by laboratory experiments and CFD simulations using tracer gas. As a result, the error was presented similarly level of results of preceding research. Some big errors could be caused by stagnated area and incongruity turbulence model. while the computational time was reduced to almost one fourth of that by preceding research.