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contributor authorRen, Tao
contributor authorModest, Michael F.
contributor authorRoy, Somesh
date accessioned2019-02-28T10:58:14Z
date available2019-02-28T10:58:14Z
date copyright12/12/2017 12:00:00 AM
date issued2018
identifier issn0742-4795
identifier othergtp_140_05_051503.pdf
identifier urihttp://yetl.yabesh.ir/yetl1/handle/yetl/4251283
description abstractRadiative heat transfer is studied numerically for reacting swirling flow in an industrial gas turbine burner operating at a pressure of 15 bar. The reacting field characteristics are computed by Reynolds-averaged Navier–Stokes (RANS) equations using the k-ϵ model with the partially stirred reactor (PaSR) combustion model. The GRI-Mech 2.11 mechanism, which includes nitrogen chemistry, is used to demonstrate the ability of reducing NOx emissions of the combustion system. A photon Monte Carlo (PMC) method coupled with a line-by-line (LBL) spectral model is employed to accurately account for the radiation effects. Optically thin (OT) and PMC–gray models are also employed to show the differences between the simplest radiative calculation models and the most accurate radiative calculation model, i.e., PMC–LBL, for the gas turbine burner. It was found that radiation does not significantly alter the temperature level as well as CO2 and H2O concentrations. However, it has significant impacts on the NOx levels at downstream locations.
publisherThe American Society of Mechanical Engineers (ASME)
titleMonte Carlo Simulation for Radiative Transfer in a High-Pressure Industrial Gas Turbine Combustion Chamber
typeJournal Paper
journal volume140
journal issue5
journal titleJournal of Engineering for Gas Turbines and Power
identifier doi10.1115/1.4038153
journal fristpage51503
journal lastpage051503-10
treeJournal of Engineering for Gas Turbines and Power:;2018:;volume( 140 ):;issue: 005
contenttypeFulltext


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