• Aucun résultat trouvé

Stability of coaxial swirling jets

N/A
N/A
Protected

Academic year: 2021

Partager "Stability of coaxial swirling jets"

Copied!
2
0
0

Texte intégral

(1)



$Q\FRUUHVSRQGHQFHFRQFHUQLQJWKLVVHUYLFHVKRXOGEHVHQWWRWKHUHSRVLWRU\DGPLQLVWUDWRU WHFKRDWDR#OLVWHVGLIILQSWRXORXVHIU

2

SHQ

$

UFKLYH

7

RXORXVH

$

UFKLYH

2

XYHUWH

2$7$2



2$7$2 LV DQ RSHQ DFFHVV UHSRVLWRU\ WKDW FROOHFWV WKH ZRUN RI VRPH 7RXORXVH UHVHDUFKHUVDQGPDNHVLWIUHHO\DYDLODEOHRYHUWKHZHEZKHUHSRVVLEOH 7KLVLVYHUVLRQSXEOLVKHGLQ 7RFLWHWKLVYHUVLRQ 



    an author's https://oatao.univ-toulouse.fr/10660

Weller, Jessie and Joly, Laurent and Fontane, Jérôme Stability of coaxial swirling jets. (2013) In: 66th Annual Meeting of the American Physical Society's Division of Fluid Dynamics (DFD), 24 November 2013 - 26 November 2013 (Pittsburgh, United States).

(2)

Stability of coaxial swirling jets

Jessie Weller-Calvo, Laurent Joly and J´erˆome Fontane

Universit´e de Toulouse, ISAE, 10 Av. ´Edouard Belin, 31055 Toulouse, France

In order to improve the mixing properties of injectors, we investigate the potential synergy between azimuthal and axial shear. For this purpose, we examine the linear modal stability of a simplified analytical model which consists of a temporally evolving swirling jet surrounded by an annular jet with a different axial velocity. We denote Λ = V2/V1 the ratio between the

axial velocity of the non-swirling annular jet V2 and the axial velocity of the

central jet V1; and q = Ωcr1/V1 the swirl number of the central jet where Ωc

is the rotation rate on the jet axis and r1 the radius of the central jet. The

present study extends the results of Gallaire & Chomaz (2003) where a single swirling jet was considered. For all values of the swirl number up to q = 2, adding the outer non-swirling jet increases substantially the growth rate of the most amplified mode, which can be more than doubled when Λ > 1. This is the result of the collaborative axial and azimuthal shear instabilities localised in between the two jets. The mode selection of larger azimuthal wavenumbers with increasing q, identified by Gallaire & Chomaz (2003), is no longer observed when the outer jet is at least as fast as the central jet Λ > 1, the axisymmetric m = 0 mode being the most amplified.

References

Gallaire, F. & Chomaz, J-M. 2003 Mode selection in swirling jet experi-ments : a linear stability analysis. J. Fluid Mech. 494, 223–253.

Références

Documents relatifs

There exists a constant c > 0 such that, for any real number , there are infinitely many integers D for which there exists a tuple of algebraic numbers

The existence of spiral breakdown states is shown to proceed from a global instability of the axisymmetric breakdown solution to helical disturbances with azimuthal

to encode Turing machines in these non-intersecting squares in a stable way (with two colours Red and Black but only one kind of 1-macro-tiles) but such that an unstable structure

Viewed as a Markovian Stochastic Approximation (SA) recursive procedure, it appears as the simplest example of an algorithm having two possible limits – its target and a trap –

of four genomic groups of Borrelia burgdorferi sensu lato in Ixodes ricinus ticks collected in a Lyme borreliosis endemic region of northern Croatia. Contribution a`

Despite gigantic efforts one has also always failed to observe indisputably a hypothetical microscopic process revealing either the violation of baryonic number A (no evidence

The large super-solar values we measure for [Ba /Fe] and [Ba/Y], which can be interpreted as the result of pollution by metal-poor AGB stars over time-scales of few 100s Myr to

The differences in the short- and long-term cumulated response observed with these methods of selection were related to the weight given in the selection index to the