Abstract:The tip vortices shed by two marine propellers are studied, relying on large-eddy simulation, using a cylindrical grid consisting of 5 billion points. A tip-loaded design, featuring winglets at the tips of its blades, is compared against a conventional one at the design advance coefficient and a model-scale Reynolds number equal to 432 000. The tip-loaded propeller achieves improved performance, but produces also more intense tip vortices. The propeller with winglets actually generates two vortices from the ti… Show more
“…2015; Posa et al. 2019, 2022 a ; Posa 2022 b ). More details on the overall methodology can be found in the works by Balaras (2004) and Yang & Balaras (2006).…”
Section: Methodsmentioning
confidence: 97%
“…However, the resolution of the computational grid and in turn the range of scales that LES is able to explicitly resolve to accurately reproduce the mechanism of wake instability has been pushed even forward in the works by Balaras, Schroeder & Posa (2015), Kumar & Mahesh (2017), Posa et al. (2019), Posa, Broglia & Balaras (2022 a ) and Posa (2022 b ).…”
Section: Introductionmentioning
confidence: 99%
“…(2019, 2022 a ) revealed the importance of the interaction between the tip vortices and the wake shed by the following blades in promoting the instability of the former, accelerated at higher rotational speeds by their decreasing pitch, shifting the streamwise location of this interaction closer to the propeller plane. More recently, Posa (2022 b ) utilized a grid of 5 billion points to simulate both conventional and tip-loaded propellers at design working conditions, to compare the development of their wakes and in particular their tip vortices. The LES computations revealed that, despite the use of pressure side winglets at the end of the tip-loaded blades, splitting the tip vortices into two smaller helical structures, tip loading still resulted in more intense tip vortices, in comparison with the conventional blade design.…”
Section: Introductionmentioning
confidence: 99%
“…While vorticity at their core was found almost proportional to the rotational speed of the propeller, the growth of both turbulence maxima and pressure minima, which are potential sources of cavitation phenomena, was verified to be faster than linear. In addition, in the earlier work by Posa (2022 b ) the wake development of the same tip-loaded propeller, including a downstream shaft, was compared against that of a conventional propeller without winglets, to assess the ability of winglets of reducing the intensity of the tip vortices, despite the higher load at the outer radii of the propeller blades.…”
Section: Introductionmentioning
confidence: 99%
“…However, the LES studies currently available in the literature typically rely on computational grids consisting of O(10 7 ) points, similar to those for the DES computations reported above, and are usually targeted at analysing the process of instability of the wake system of marine propellers and the cavitation phenomena occurring within the large coherent structures they shed (Liefvendahl 2010;Liefvendahl, Felli & Troëng 2010;Asnaghi, Svennberg & Bensow 2018a,b, 2020aHu et al 2019a;Zhu & Gao 2019;Ahmed, Croaker & Doolan 2020;Asnaghi et al 2020b;Long et al 2020;Kimmerl, Mertes & Abdel-Maksoud 2021a,b;Wang et al 2021bWang et al , 2022aWang, Liu & Wu 2022d). However, the resolution of the computational grid and in turn the range of scales that LES is able to explicitly resolve to accurately reproduce the mechanism of wake instability has been pushed even forward in the works by Balaras, Schroeder & Posa (2015), Kumar & Mahesh (2017), Posa et al (2019), Posa, Broglia & Balaras (2022a) and Posa (2022b). Kumar & Mahesh (2017) adopted an unstructured grid consisting of 181 million hexahedral cells to conduct wall-resolved computations and analyse in detail the development and eventual instability of the wake shed by the five-bladed DTMB 4381 propeller at the design working condition, using a body-fitted approach.…”
Large-eddy simulation on a grid consisting of 5 billion points was utilized to study the properties of turbulence at the core of the tip and hub vortices shed by a marine propeller across working conditions. Turbulence at the core of the tip vortices was found to be initially isotropic, moving towards a ‘cigar-shaped’ axisymmetric state as instability grows, dominated by turbulent fluctuations of the velocity component directed in the radial direction of the cylindrical reference frame centred at the wake axis. The break-up of the coherence of the tip vortices is instead characterized by turbulence recovering an isotropic state. This process is accelerated by growing load conditions of the propeller. In contrast, during instability of the hub vortex, turbulence at its core develops a ‘pancake-shaped’ axisymmetric state, dominated by the fluctuations of the radial and azimuthal velocities. However, at higher propeller loads turbulence at the core of the hub vortex keeps close to isotropy, thanks to a faster instability. Within both tip and hub vortices the deviations from Boussinesq's hypothesis were found very significant, providing evidence of the unsuitability of conventional turbulence modelling. At the core of the tip vortices they become especially large at their break-up and for increasing load conditions of the propeller, equivalent to more intense structures. In contrast, at the core of the hub vortex they were verified to be decreasing functions of the propeller load.
“…2015; Posa et al. 2019, 2022 a ; Posa 2022 b ). More details on the overall methodology can be found in the works by Balaras (2004) and Yang & Balaras (2006).…”
Section: Methodsmentioning
confidence: 97%
“…However, the resolution of the computational grid and in turn the range of scales that LES is able to explicitly resolve to accurately reproduce the mechanism of wake instability has been pushed even forward in the works by Balaras, Schroeder & Posa (2015), Kumar & Mahesh (2017), Posa et al. (2019), Posa, Broglia & Balaras (2022 a ) and Posa (2022 b ).…”
Section: Introductionmentioning
confidence: 99%
“…(2019, 2022 a ) revealed the importance of the interaction between the tip vortices and the wake shed by the following blades in promoting the instability of the former, accelerated at higher rotational speeds by their decreasing pitch, shifting the streamwise location of this interaction closer to the propeller plane. More recently, Posa (2022 b ) utilized a grid of 5 billion points to simulate both conventional and tip-loaded propellers at design working conditions, to compare the development of their wakes and in particular their tip vortices. The LES computations revealed that, despite the use of pressure side winglets at the end of the tip-loaded blades, splitting the tip vortices into two smaller helical structures, tip loading still resulted in more intense tip vortices, in comparison with the conventional blade design.…”
Section: Introductionmentioning
confidence: 99%
“…While vorticity at their core was found almost proportional to the rotational speed of the propeller, the growth of both turbulence maxima and pressure minima, which are potential sources of cavitation phenomena, was verified to be faster than linear. In addition, in the earlier work by Posa (2022 b ) the wake development of the same tip-loaded propeller, including a downstream shaft, was compared against that of a conventional propeller without winglets, to assess the ability of winglets of reducing the intensity of the tip vortices, despite the higher load at the outer radii of the propeller blades.…”
Section: Introductionmentioning
confidence: 99%
“…However, the LES studies currently available in the literature typically rely on computational grids consisting of O(10 7 ) points, similar to those for the DES computations reported above, and are usually targeted at analysing the process of instability of the wake system of marine propellers and the cavitation phenomena occurring within the large coherent structures they shed (Liefvendahl 2010;Liefvendahl, Felli & Troëng 2010;Asnaghi, Svennberg & Bensow 2018a,b, 2020aHu et al 2019a;Zhu & Gao 2019;Ahmed, Croaker & Doolan 2020;Asnaghi et al 2020b;Long et al 2020;Kimmerl, Mertes & Abdel-Maksoud 2021a,b;Wang et al 2021bWang et al , 2022aWang, Liu & Wu 2022d). However, the resolution of the computational grid and in turn the range of scales that LES is able to explicitly resolve to accurately reproduce the mechanism of wake instability has been pushed even forward in the works by Balaras, Schroeder & Posa (2015), Kumar & Mahesh (2017), Posa et al (2019), Posa, Broglia & Balaras (2022a) and Posa (2022b). Kumar & Mahesh (2017) adopted an unstructured grid consisting of 181 million hexahedral cells to conduct wall-resolved computations and analyse in detail the development and eventual instability of the wake shed by the five-bladed DTMB 4381 propeller at the design working condition, using a body-fitted approach.…”
Large-eddy simulation on a grid consisting of 5 billion points was utilized to study the properties of turbulence at the core of the tip and hub vortices shed by a marine propeller across working conditions. Turbulence at the core of the tip vortices was found to be initially isotropic, moving towards a ‘cigar-shaped’ axisymmetric state as instability grows, dominated by turbulent fluctuations of the velocity component directed in the radial direction of the cylindrical reference frame centred at the wake axis. The break-up of the coherence of the tip vortices is instead characterized by turbulence recovering an isotropic state. This process is accelerated by growing load conditions of the propeller. In contrast, during instability of the hub vortex, turbulence at its core develops a ‘pancake-shaped’ axisymmetric state, dominated by the fluctuations of the radial and azimuthal velocities. However, at higher propeller loads turbulence at the core of the hub vortex keeps close to isotropy, thanks to a faster instability. Within both tip and hub vortices the deviations from Boussinesq's hypothesis were found very significant, providing evidence of the unsuitability of conventional turbulence modelling. At the core of the tip vortices they become especially large at their break-up and for increasing load conditions of the propeller, equivalent to more intense structures. In contrast, at the core of the hub vortex they were verified to be decreasing functions of the propeller load.
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