Abstract
Hot gas ingestion refers to the phenomenon of mainstream hot gas flowing into the space cavity of a turbine wheel. Previous studies have found that mainstream annulus pressure distribution plays an important role in hot gas ingestion, but due to its complexity, the mechanism of the interaction between mainstream flow and hot gas ingestion remains unclear. This paper adopts the URANS method, and three sealing flow rates are considered, named Cw=0, Cw=500, and Cw=5000. The time-averaged annulus pressure distribution shows that an increase in the sealing flow decreases the pressure value, and the effects of the sealing flow on the pressure distribution of the leading edge of the blade are much more influential than that of the trailing edge of the vane. The unsteady pressure time-space distribution in the annulus indicates that a time-space tilted distribution of pressure at the rim exits when the sealing flow exists. This phenomenon is mainly due to the strong feedback mechanism of the sealing flow to the annulus pressure field. A comparison of the pressure and mean radial velocity distribution of the mainstream shows that the ingestion mainly occurs on the blade side, where the pressure is lower than on the vane side. The flow characteristics at the wheel rim are analyzed with a sealing flow rate Cw=5000, and under these conditions, both pressure-induced ingestion and ingestion caused by a passage vortex can be inferred. The three-dimensional and inertial effects of the mainstream at the wheel rim lead to the generation of separation vortices on the blade side, and the presence of separation vortices leads to ingestion along the blade side. At the same time, pressure on the blade side will cause the fluid to have a radial inward flow tendency, which will promote the formation of separation vortices, leading to more serious ingestion in the high-pressure region on the blade side. The blade pressure field can be more significant than the vane trailing pressure field in the rim seal ingestion, and it contributes some explanations to the open question: the effect of blade on ingestion.
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Abbreviations
- b :
-
outer radius of disk cavity/mm
- C p :
-
dimensionless pressure coefficient, Cp=(p−pavg)/q
- C w :
-
dimensionless sealing flow rate, Cw=m/µb
- ΔC p :
-
dimensionless peak-trough pressure difference in the annulus, ΔCp=Cpmax−Cpmin
- m :
-
mass flow rate/kg·s−1
- p :
-
local static pressure/Pa
- p avg :
-
line average static pressure across two pitches/Pa
- q :
-
dynamic pressure of fluid at axial velocity in the annulus/Pa, q=ρW2/2
- Re ϕ :
-
disk rotational Reynolds number, Reϕ=ρΩb2/μ
- T :
-
time for one blade passing period/s
- t :
-
time/s
- U :
-
hub speed/m·s−1, U=Ωb
- V :
-
total speed/m·s−1
- V r :
-
local radial velocity/m·s−1
- \({{\bar V}_{\rm{r}}}\) :
-
circumferential average radial velocity/m·s−1
- \({{\bar V}_{\rm{r}}}/U\) :
-
dimensionless radial average velocity by hub speed
- W :
-
axial velocity in the annulus/m·s−1
- W s :
-
streamwise vortex
- X :
-
axial coordinates from the vane trailing to the blade leading edge/m
- θ :
-
normalized tangential coordinate between two vanes
- μ :
-
dynamic viscosity/Pa·s
- Ω :
-
rotating disk angular speed/rad·s−1
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Acknowledgments
The authors wish to acknowledge the financial support of the National Natural Science Foundation Outstanding Youth Foundation (Grant No. 52122603), the National Science and Technology Major Project (J2019-III-0003-0046) and the cloud computing supported by the Beijing Super Cloud Computing Center.
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Ren, R., Du, Q., Liu, G. et al. Influence of Vanes and Blades on Ingress in Axial Rim Seal for Turbine Stages. J. Therm. Sci. 33, 833–846 (2024). https://doi.org/10.1007/s11630-024-1986-0
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DOI: https://doi.org/10.1007/s11630-024-1986-0