Modal dynamics of high-frequency transverse combustion instabilities

被引:17
|
作者
Kim, Jeong-won [1 ]
Gillman, Wesley [1 ]
Emerson, Benjamin [1 ]
Wu, David [1 ]
John, Tony [1 ]
Acharya, Vishal [1 ]
Isono, Mitsunori [2 ]
Saitoh, Toshihiko [2 ]
Lieuwen, Timothy [1 ]
机构
[1] Georgia Inst Technol, Atlanta, GA 30332 USA
[2] Mitsubishi Heavy Ind Co Ltd, Tokyo, Japan
关键词
Combustion instability; Transverse modes; Dynamical systems; Acoustics; Premixed flames; EXCITED AZIMUTHAL MODES; LARGE-EDDY SIMULATION;
D O I
10.1016/j.proci.2020.06.237
中图分类号
O414.1 [热力学];
学科分类号
摘要
This paper investigates the modal dynamics of self-excited high frequency transverse instabilities in a multi-nozzle, swirl-stabilized can combustor. It utilizes results from multiple pressure sensors to decompose the disturbance into clockwise (CW) and counter-clockwise (CCW) waves, enabling a reconstruction of the pressure amplitude, phase, anti-nodal line location, and spin ratio. While these types of decompositions have been demonstrated on small scale combustors, particularly annular combustors, this is the first study to analyze these results for a high power, multi-nozzle can combustor. Its particular focus is in characterizing the system evolution in phase space and the nature of the system attractors under linearly unstable conditions; results are presented in spin ratio-phase difference space, so that limit cycle oscillations appear as fixed points. Results are shown for conditions where three different attractors dominate (standing, CW, and CCW) but are taken for very long time periods (similar to 50,000 cycles) so that the system's interaction with these attractors can be observed. For the standing mode-dominated case, the phase portrait shows spiral trajectories converging to a single fixed point. For the spinning mode dominated cases, however, multiple fixed points and saddle points were observed, and the trajectories showed a more complicated structure. It was also shown that even though the CW mode is dominant, this mode intermittently switches to standing or CCW modes for short period. These results suggest that the strength of each attractor depends on test conditions and that random noise stochastically perturbs the system so that large regions of the phase space are explored. Finally, one interesting observation is that the angular velocity of the anti-nodal line linearly varies with the spin ratio under standing-mode dominant conditions. (c) 2020 The Combustion Institute. Published by Elsevier Inc. All rights reserved.
引用
收藏
页码:6155 / 6163
页数:9
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