Simulation of Turbulent Mixing Effects on Essential NO<sub>x</sub>–O<sub>3</sub>–Hydrocarbon Photochemistry in Convective Boundary Layer

The turbulence kinetics model (TKM) describes an overall reaction rate for microscopic mass transfer phenomenon expressed as separation intensity, <i>I<sub>s</sub></i>, in a turbulent reacting flow. This study examines the effects of turbulent mixing in the convective boundar...

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Main Author: Mi-Sug Kim
Format: Article
Language:English
Published: MDPI AG 2019-01-01
Series:Applied Sciences
Subjects:
Online Access:https://www.mdpi.com/2076-3417/9/2/357
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author Mi-Sug Kim
author_facet Mi-Sug Kim
author_sort Mi-Sug Kim
collection DOAJ
description The turbulence kinetics model (TKM) describes an overall reaction rate for microscopic mass transfer phenomenon expressed as separation intensity, <i>I<sub>s</sub></i>, in a turbulent reacting flow. This study examines the effects of turbulent mixing in the convective boundary layer (CBL) on essential NOx&#8315;O<sub>3</sub>&#8315;Hydrocarbon photochemistry containing sources of NO and a surrogate reactive hydrocarbon. The modeling approach applies for all species except OH with an assumption of a photostationary steady state. The TKM results reveal principal findings as follows: (1) effects of turbulence on reaction rates lead to significant segregations throughout most of the CBL in reaction pairs NO + O<sub>3</sub>, RH + OH and NO + HO<sub>2</sub>; (2) segregations permit significantly higher concentrations of NO and RH to build up and endure in the CBL than would occur for a non-turbulent atmosphere; (3) turbulent segregation influences limit and shift the ranges of NO and O<sub>3</sub> concentrations compared to the non-turbulent case; (4) while there are differences between the TKM results and those for a published Large Eddy simulation (LES) of the same chemical system, there are also strong similarities. Therefore, a future study remains to compare model results to observations if and when appropriately time-resolved measurements of reacting species are obtained.
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spelling doaj.art-02f555df18c9455bb8cee6e8e7fa6dd02022-12-21T21:49:29ZengMDPI AGApplied Sciences2076-34172019-01-019235710.3390/app9020357app9020357Simulation of Turbulent Mixing Effects on Essential NO<sub>x</sub>–O<sub>3</sub>–Hydrocarbon Photochemistry in Convective Boundary LayerMi-Sug Kim0Department of Environmental Engineering, Mokpo National University, # B20-2012, 1666, Yeongsan-ro, Dorim-ri, Cheonggye-myeon, Muan-gun, Jeollanam-do 58554, KoreaThe turbulence kinetics model (TKM) describes an overall reaction rate for microscopic mass transfer phenomenon expressed as separation intensity, <i>I<sub>s</sub></i>, in a turbulent reacting flow. This study examines the effects of turbulent mixing in the convective boundary layer (CBL) on essential NOx&#8315;O<sub>3</sub>&#8315;Hydrocarbon photochemistry containing sources of NO and a surrogate reactive hydrocarbon. The modeling approach applies for all species except OH with an assumption of a photostationary steady state. The TKM results reveal principal findings as follows: (1) effects of turbulence on reaction rates lead to significant segregations throughout most of the CBL in reaction pairs NO + O<sub>3</sub>, RH + OH and NO + HO<sub>2</sub>; (2) segregations permit significantly higher concentrations of NO and RH to build up and endure in the CBL than would occur for a non-turbulent atmosphere; (3) turbulent segregation influences limit and shift the ranges of NO and O<sub>3</sub> concentrations compared to the non-turbulent case; (4) while there are differences between the TKM results and those for a published Large Eddy simulation (LES) of the same chemical system, there are also strong similarities. Therefore, a future study remains to compare model results to observations if and when appropriately time-resolved measurements of reacting species are obtained.https://www.mdpi.com/2076-3417/9/2/357turbulentmixingsegregationCBLphotochemistry
spellingShingle Mi-Sug Kim
Simulation of Turbulent Mixing Effects on Essential NO<sub>x</sub>–O<sub>3</sub>–Hydrocarbon Photochemistry in Convective Boundary Layer
Applied Sciences
turbulent
mixing
segregation
CBL
photochemistry
title Simulation of Turbulent Mixing Effects on Essential NO<sub>x</sub>–O<sub>3</sub>–Hydrocarbon Photochemistry in Convective Boundary Layer
title_full Simulation of Turbulent Mixing Effects on Essential NO<sub>x</sub>–O<sub>3</sub>–Hydrocarbon Photochemistry in Convective Boundary Layer
title_fullStr Simulation of Turbulent Mixing Effects on Essential NO<sub>x</sub>–O<sub>3</sub>–Hydrocarbon Photochemistry in Convective Boundary Layer
title_full_unstemmed Simulation of Turbulent Mixing Effects on Essential NO<sub>x</sub>–O<sub>3</sub>–Hydrocarbon Photochemistry in Convective Boundary Layer
title_short Simulation of Turbulent Mixing Effects on Essential NO<sub>x</sub>–O<sub>3</sub>–Hydrocarbon Photochemistry in Convective Boundary Layer
title_sort simulation of turbulent mixing effects on essential no sub x sub o sub 3 sub hydrocarbon photochemistry in convective boundary layer
topic turbulent
mixing
segregation
CBL
photochemistry
url https://www.mdpi.com/2076-3417/9/2/357
work_keys_str_mv AT misugkim simulationofturbulentmixingeffectsonessentialnosubxsubosub3subhydrocarbonphotochemistryinconvectiveboundarylayer