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Transition to turbulence in the rotating-disk boundary-layer flow with stationary vortices
KTH, Skolan för teknikvetenskap (SCI), Mekanik.ORCID-id: 0000-0002-9859-6169
KTH, Skolan för teknikvetenskap (SCI), Mekanik.ORCID-id: 0000-0001-9627-5903
KTH, Skolan för teknikvetenskap (SCI), Mekanik.ORCID-id: 0000-0002-1146-3241
KTH, Skolan för teknikvetenskap (SCI), Mekanik.
(engelsk)Artikkel i tidsskrift (Fagfellevurdert) Submitted
HSV kategori
Identifikatorer
URN: urn:nbn:se:kth:diva-200906OAI: oai:DiVA.org:kth-200906DiVA, id: diva2:1071216
Merknad

QC 20170203

Tilgjengelig fra: 2017-02-03 Laget: 2017-02-03 Sist oppdatert: 2017-02-03bibliografisk kontrollert
Inngår i avhandling
1. The rotating-disk boundary-layer flow studied through numerical simulations
Åpne denne publikasjonen i ny fane eller vindu >>The rotating-disk boundary-layer flow studied through numerical simulations
2017 (engelsk)Doktoravhandling, med artikler (Annet vitenskapelig)
Abstract [en]

This thesis deals with the instabilities of the incompressible boundary-layer flow thatis induced by a disk rotating in otherwise still fluid. The results presented include bothwork in the linear and nonlinear regime and are derived from direct numerical sim-ulations (DNS). Comparisons are made both to theoretical and experimental resultsproviding new insights into the transition route to turbulence. The simulation codeNek5000 has been chosen for the DNS using a spectral-element method (SEM) witha high-order discretization, and the results were obtained through large-scale paral-lel simulations. The known similarity solution of the Navier–Stokes equations for therotating-disk flow, also called the von K ́arm ́an rotating-disk flow, is reproduced by theDNS. With the addition of modelled small simulated roughnesses on the disk surface,convective instabilities appear and data from the linear region in the DNS are anal-ysed and compared with experimental and theoretical data, all corresponding verywell. A theoretical analysis is also presented using a local linear-stability approach,where two stability solvers have been developed based on earlier work. Furthermore,the impulse response of the rotating-disk boundary layer is investigated using DNS.The local response is known to be absolutely unstable and the global response, onthe contrary, is stable if the edge of the disk is assumed to be at radius infinity. Herecomparisons with a finite domain using various boundary conditions give a globalbehaviour that can be both linearly stable and unstable, however always nonlinearlyunstable. The global frequency of the flow is found to be determined by the Rey-nolds number at the confinement of the domain, either by the edge (linear case) or bythe turbulence appearance (nonlinear case). Moreover, secondary instabilities on topof the convective instabilities induced by roughness elements were investigated andfound to be globally unstable. This behaviour agrees well with the experimental flowand acts at a smaller radial distance than the primary global instability. The sharpline corresponding to transition to turbulence seen in experiments of the rotating diskcan thus be explained by the secondary global instability. Finally, turbulence datawere compared with experiments and investigated thoroughly.

sted, utgiver, år, opplag, sider
Stockholm: KTH Royal Institute of Technology, 2017. s. 47
Serie
TRITA-MEK, ISSN 0348-467X ; 2017:01
Emneord
laminar-turbulent transition, convective instability, absolute instability, crossflow instability, direct numerical simulations
HSV kategori
Forskningsprogram
Fysik
Identifikatorer
urn:nbn:se:kth:diva-200827 (URN)978-91-7729-269-2 (ISBN)
Disputas
2017-02-24, F3, Lindstedtsvägen 26, Stockholm, 10:15 (engelsk)
Opponent
Veileder
Merknad

QC 20170203

Tilgjengelig fra: 2017-02-03 Laget: 2017-02-03 Sist oppdatert: 2017-02-03bibliografisk kontrollert

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