Velocity and concentration field measurements and large eddy simulation of a shaped film cooling hole
Introduction
A variant of the canonical jet in crossflow, the inclined jet in crossflow, is commonly used in gas turbines to release coolant flow onto the surface of turbine blades, protecting them from hot combustion gases in a technique called film cooling (Bogard and Thole, 2006). Hole shape is an important parameter governing the flow and can lead to dramatic changes in flow structures, mixing, and film cooling effectiveness. The most prevalent shaped hole found in film cooling literature is the laidback fan-shaped diffuser hole, which is defined by the forward and lateral expansion angles. Diffuser holes are favored over cylindrical holes because they slow down the coolant flow and thus mitigate the negative effects of the counter-rotating vortex pair and reduce or eliminate jet blow-off. A thorough review of the literature in the field of shaped hole film cooling is given by Bunker (2005).
Laidback fan-shaped diffuser exits are prone to separation within the diffuser if the expansion angles are too large. Thole et al. (1998) found evidence of separation inside shaped holes with large expansion angles based on turbulence levels. Gunady et al. (2019) measured the velocity field of a laidback fan-shaped hole with forward and lateral expansion angles of 12° using Magnetic Resonance Velocimetry (MRV) and observed separated flow at the inlet of the metering section of the hole as well as in the diffuser. Gritsch et al. (1998) measured adiabatic effectiveness of a similar hole with 15° forward expansion and 14° lateral expansion. In both studies of holes with large expansion angles by Gunady et al., 2019, Gritsch et al., 1998, the flow separated on one side of the laidback diffuser portion of the hole due to the large expansion angles.
The present study focuses on a specific hole geometry known as the “7-7-7 shaped hole,” a laidback fan-shaped diffuser hole designed by Schroeder and Thole (2014) with forward and lateral expansion angles of 7°. The smaller expansion angle compared to some other holes is intended to reduce flow separation inside the diffuser section of the hole. Schroeder and Thole (2014) used an infrared camera to measure the adiabatic effectiveness of the 7-7-7 shaped hole at density ratios of 1.2 and 1.5, blowing ratios between 1 and 3, and various freestream turbulence intensities. In addition to flowfield and adiabatic effectiveness measurements, Schroeder and Thole (2017b) used a thermal rake to collect thermal field measurements for different blowing ratios and freestream turbulence intensities. Haydt and Lynch, 2018b, Schroeder and Thole, 2017a measured the flowfield of the 7-7-7 shaped hole using particle image velocimetry (PIV) for varying compound angles, freestream turbulence intensities, in–hole roughness, and blowing ratios.
The 7-7-7 geometry is important because it is used as a benchmark to which the performance of new hole geometries are compared (Hossain et al., 2020, Thurman et al., 2016, Snyder and Thole, 2020). Numerous other studies have been conducted using the 7-7-7 shaped hole geometry or other similar geometries. However, many of these studies use laser based techniques or hot-wire anemometry, both of which have limitations on where data can be taken due to optical or physical access requirements. Separated flow in the metering section of the hole or in the diffuser can be inferred based on downstream turbulence intensity or adiabatic effectiveness contours, but the existence or absence of separated flow is seldom directly observed. Detailed experimental data of 3D velocity fields, especially inside of the hole, are needed to gain a more complete understanding of the flow resulting from the 7-7-7 hole geometry.
The 7-7-7 shaped hole has also been studied using simulations. In addition to adiabatic effectiveness measurements, Haydt and Lynch (2018a) conducted RANS CFD predictions of the 7-7-7 hole at various compound angles. Oliver et al. (2019) performed compressible high fidelity simulations of the 7-7-7 geometry to study Mach number sensitivity; they observed in–hole separation in all cases, and flow asymmetry only in their high Mach number simulation.
Although diffuser holes mitigate the counter-rotating vortex pair, jet lift off, and excessive mixing with the freestream, complex in–hole flows, such as separation, can still negatively impact performance. Separated flow can create a jetting effect inside the hole, reducing the effective area ratio of the diffuser.
Conventional CFD does not consistently capture the detailed flow features of real film cooling flows. There is a glaring need for fully 3D data to inform the development of improved models. Many experimental methods exist for measuring 3D velocity and concentration fields. Some of these methods can result in time-resolved data. However, laser based techniques can be complex and are limited by geometry and optical access. Magnetic Resonance Velocimetry (MRV) and Magnetic Resonance Concentration (MRC) can be used to acquire the 3D mean velocity and scalar concentration field, respectively, of an arbitrarily complex geometry. When applied to film cooling, flow structures and the resulting adiabatic effectiveness can be studied in three dimensions. Large Eddy Simulation (LES) can compliment MRV and MRC results by providing near-wall results and turbulent statistics. Milani et al. (2019) studied an inclined round hole using 3D data from MRI and LES. Effects of asymmetry caused by the plenum conditions and persisting through the metering section are observed in the flow. Flow inside the diffuser section of shaped diffuser holes could be affected by asymmetric flow in the metering section of such holes.
In this study, MRV and MRC experiments as well as a LES of the 7-7-7 shaped hole geometry are conducted. The MRV and MRC are used to validate the LES, and adiabatic effectiveness results from the MRC and LES are compared with data from Schroeder and Thole (2014).
Section snippets
Setup
The 7-7-7 shaped hole geometry described in Schroeder and Thole (2014) is used in this work. The hole has a diameter in the metering section and is inclined at . After the circular metering section, the hole expands 7° in the forward and both lateral directions to a laidback fan-shaped diffuser. The metering and diffuser sections have non-dimensional lengths and , respectively. All edges in the diffuser are rounded to a radius of . A top view of the hole
Computational methodology
The hole geometry, channel cross-sectional area, and flow rates used in the computational study are identical to the one used for the MRI-based experiments. The computational setup follows the framework described in detail by Milani et al. (2019). To summarize, a highly resolved Large Eddy Simulation (LES) is run using the incompressible solver Vida from Cascade Technologies. The filtered incompressible continuity (Eq. (5)) and Navier–Stokes equations (Eq. (6)) as well as the filtered equation
Comparison with other experiments
To effectively cool the surface, the coolant jet must stay attached to the wall after injection. The pressure the mainstream flow exerts on the coolant is responsible for turning the jet towards the wall. If the jet detaches from the wall, the film cooling performance is significantly reduced and is dominated by the mixing of the coolant in the mainstream flow. This mixing is carried out by turbulence originating in the shear layer at injection and scales with the velocity ratio. If the jet
Conclusions
The laidback fan-shaped film cooling hole featured in this study is the 7-7-7 geometry developed by Schroeder and Thole (2014). The time-averaged, 3D, 3-component velocity field from this hole is obtained using MRV. The 3D time-averaged scalar concentration field is obtained using MRC. The velocity and scalar concentration field are also computed using LES. Both the MRV and LES show that a region of separation is present inside the hole. However, the position of the separated region is
Declaration of competing interest
The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.
Acknowledgements
The authors thank Honeywell Aerospace for the financial support. The authors thank the Steady Thermal Aero Research Turbine (START) Laboratory and the Experimental and Computational Convection Laboratory (ExCCL) at Penn State for sharing the 7-7-7 shaped hole geometry and their experimental data.
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