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On the size of transitional boundary-layer streaks
KTH, School of Engineering Sciences (SCI), Engineering Mechanics.ORCID iD: 0000-0002-1766-5557
KTH, School of Engineering Sciences (SCI), Engineering Mechanics, Fluid Mechanics.ORCID iD: 0000-0002-5913-5431
KTH, School of Engineering Sciences (SCI), Engineering Mechanics, Fluid Mechanics.ORCID iD: 0000-0001-7864-3071
2025 (English)In: Journal of Fluid Mechanics, ISSN 0022-1120, E-ISSN 1469-7645, Vol. 1007, article id R6Article in journal (Refereed) Published
Abstract [en]

A collection of secondary instability calculations in streaky boundary layers is presented. The data are retrieved from well-resolved numerical simulations of boundary layers forced by free-stream turbulence (FST), considering different geometries and FST conditions. The stability calculations are performed before streak breakdown, taking place at various $Rey_x$ the Reynolds number based on the streamwise coordinate. Despite the rich streak population of various sizes, it is found that breaking streaks have similar aspect ratios, independently of the streamwise position where they appear. This suggests that wider streaks will break down further downstream than thinner ones, making the appearance of secondary instabilities somewhat independent of the streak's wavelength. Moreover, the large difference in the integral length scale among the simulations suggests that this aspect ratio is also independent of the FST scales. An explanation for this behaviour is provided by showing that these breaking streaks are in the range of perturbations that can experience maximum transient growth according to optimal disturbance theory. This could explain why, at a given streamwise position, there is a narrow spanwise wavelength range where streak breakdown is more likely to occur.

Place, publisher, year, edition, pages
Cambridge University Press (CUP) , 2025. Vol. 1007, article id R6
Keywords [en]
boundary layer receptivity, boundary layer stability, transition to turbulence
National Category
Fusion, Plasma and Space Physics
Identifiers
URN: urn:nbn:se:kth:diva-361878DOI: 10.1017/jfm.2025.152ISI: 001444323800001Scopus ID: 2-s2.0-105000095311OAI: oai:DiVA.org:kth-361878DiVA, id: diva2:1949335
Note

QC 20250402

Available from: 2025-04-02 Created: 2025-04-02 Last updated: 2025-04-02Bibliographically approved

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Alarcón, José FaúndezHanifi, ArdeshirHenningson, Dan S.

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