Axial evolution of forced helical flame and flow disturbances

dc.contributor.author

Smith, TE

dc.contributor.author

Douglas, CM

dc.contributor.author

Emerson, BL

dc.contributor.author

Lieuwen, TC

dc.date.accessioned

2025-09-25T01:29:24Z

dc.date.available

2025-09-25T01:29:24Z

dc.date.issued

2018-06-10

dc.description.abstract

This paper presents 5 kHz stereo particle image velocimetry and OH planar laser induced fluorescence measurements of transversely forced swirl flames. The presence of transverse forcing on this naturally unstable flow both influences the natural instabilities, as well as amplifies disturbances that may not necessarily manifest themselves during natural oscillations. By manipulating the structure of the acoustic forcing field, both axisymmetric and helical modes are preferentially excited away from the frequency of natural instability. The paper presents a method for spatially interpolating the phase locked r-z and r-θ planar velocity and flame position data, extracting the full three-dimensional structure of the helical disturbances. These helical disturbances are also decomposed into symmetric and anti-symmetric disturbances about the jet core, showing the subsequent axial evolution (in magnitude and phase) of each of these underlying disturbances. It is shown that out-of-phase acoustic forcing excites m = ±1 modes, but the flow field preferentially amplifies the counter-winding, co-rotating helical disturbance over the co-winding, counter-rotating helical disturbance. This causes the flow and flame to transition from a transverse flapping near the jet exit to a precessing motion further downstream. In contrast, in-phase forcing promotes axisymmetric m = 0 disturbances which dominate the flow field over the entire axial domain. In both cases, the amplitudes of the anti-symmetric disturbances about the jet core grow with downstream distance before saturating and decaying, while the symmetric disturbances appear nearly negligible. It is suggested that this saturation and decay is due to linear effects (e.g. a negative spatial growth rate), rather than nonlinear interactions.

dc.identifier.issn

0022-1120

dc.identifier.issn

1469-7645

dc.identifier.uri

https://hdl.handle.net/10161/33231

dc.language

en

dc.publisher

Cambridge University Press (CUP)

dc.relation.ispartof

Journal of Fluid Mechanics

dc.relation.isversionof

10.1017/jfm.2018.151

dc.rights.uri

https://creativecommons.org/licenses/by-nc/4.0

dc.subject

absolute/convective instability

dc.subject

combustion

dc.subject

reacting flows

dc.title

Axial evolution of forced helical flame and flow disturbances

dc.type

Journal article

duke.contributor.orcid

Douglas, CM|0000-0002-5968-3315

pubs.begin-page

323

pubs.end-page

356

pubs.organisational-group

Duke

pubs.organisational-group

Pratt School of Engineering

pubs.organisational-group

Thomas Lord Department of Mechanical Engineering and Materials Science

pubs.publication-status

Published

pubs.volume

844

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