Characteristics of turbulent nonpremixed jet flames under normal- and low-gravity conditions

• Published in: Combustion and flame 2004-09, Vol.138 (4), p.384-400
• Main Authors: Idicheria, Cherian A., Boxx, Isaac G., Clemens, Noel T.
• Format: Article
• Language: English
• Subjects: Applied sciences; Buoyancy; Combustion. Flame; Energy; Energy. Thermal use of fuels; Exact sciences and technology; Microgravity; Theoretical studies. Data and constants. Metering; Turbulent nonpremixed flames
• ISSN: 0010-2180; 1556-2921
• DOI: 10.1016/j.combustflame.2004.07.002

An experimental study was performed with the aim of investigating the structure of transitional and turbulent nonpremixed jet flames under different gravity conditions. Experiments were conducted under three gravity levels, viz., 1 g, 20 mg, and 100 μg. The milligravity and microgravity conditions were achieved by dropping a jet-flame rig in the University of Texas at Austin 1.25-s and NASA-Glenn Research Center 2.2-s drop towers, respectively. The flames studied were piloted nonpremixed propane, ethylene, and methane jet flames at source Reynolds numbers ranging from 2000 to 10,500. The principal diagnostic employed was time-resolved cinematographic imaging of the visible soot luminosity. Mean and root-mean-square (RMS) images were computed, and volume rendering of the image sequences was used to investigate the large-scale structure evolution and flame tip dynamics. The relative importance of buoyancy was quantified with the parameter, ξ L , as defined by Becker and Yamazaki (Combust. Flame 33 (1978) 123–149). The results showed, in contrast to some previous microgravity studies, that the high-Reynolds-number flames have the same flame length irrespective of the gravity level. The mean and RMS luminosity images and the volume renderings indicate that the large-scale structure and flame tip dynamics are essentially identical to those of purely momentum-driven flames provided ξ L is less than approximately 2–3. The volume renderings show that the luminous structure velocities (i.e., celerities) normalized by the jet exit velocity are approximately constant for ξ L < 6 , but scale as ξ L 3 / 2 for ξ L > 8 . The flame length fluctuation measurements and volume renderings also indicate that the luminous structures are more organized in low gravity than in normal gravity. Finally, taken as a whole, this study shows that ξ L is a sufficient parameter for quantifying the effects of buoyancy on the fluctuating and mean characteristics of turbulent jet flames.