Publikationsdatum:
2016-04-26
Beschreibung:
Recent investigations by Hellström have uncovered certain errors in the papers by Hellström & Smits (2014) and Hellström, Ganapathisubramani & Smits (2015), which are corrected below. Hellström & Smits (2014) estimated the convective displacement between two consecutive data snapshots, based on the bulk velocity, to be 0:48R and 0:96R for Reynolds numbers 47 000 and 93 000, respectively. These displacements should be corrected to 2:20R and 4:40R. The convective length scales were not used as a part of the analysis and so the errors have no further impact on this work and do not affect its conclusions. The incorrect estimation of the convective displacement propagated to Hellström et al. (2015), where the displacement should be corrected from 0:96R to 4:77R for ReD D 104 000. This correction implies that the large-scale structures remain spatiotemporally correlated for longer than the reported 1-2R. Figure 1 shows the corrected temporal autocorrelation of the first proper orthogonal decomposition (POD) mode and third azimuthal mode number, φn.mI r/Dφ 1.3I r/, for Reynolds numbers 52 000 and 104 000. The decay to the e-1 point suggests that the streamwise spatio-temporal length of the coherent structures is approximately 3R, which is in good agreement with the streamwise extent of the corresponding conditional mode, ψ(3,1). The corrections to the estimated spatio-temporal length scale do not further impact the work, including the conclusion that these structures of O.3R/ in length are a basic building block that line up to create longer structures similar to the very large-scale motions (VLSMs). (Figure Presented). © Cambridge University Press 2016.
Print ISSN:
0022-1120
Digitale ISSN:
1469-7645
Thema:
Maschinenbau
,
Physik
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