Radiofrequency plasma stabilization of a low-Reynolds-number channel flow

2014 ◽  
Vol 748 ◽  
pp. 663-691 ◽  
Author(s):  
Timothy J. Fuller ◽  
Andrea G. Hsu ◽  
Rodrigo Sanchez-Gonzalez ◽  
Jacob C. Dean ◽  
Simon W. North ◽  
...  

AbstractThe effects of plasma heating and thermal non-equilibrium on the statistical properties of a low-Reynolds-number ($Re_{\tau } = 49$) turbulent channel flow were experimentally quantified using particle image velocimetry, two-line planar laser-induced fluorescence, coherent anti-Stokes Raman spectroscopy and emission spectroscopy. Tests were conducted at two radiofrequency plasma settings. The nitrogen, in air, was vibrationally excited to $T_{vib} \sim 1240\ \mathrm{K}$ and 1550 K for 150 W and 300 W plasma settings, respectively, while the vibrational temperature of the oxygen and the rotational/translational temperatures of all species remained near room temperature. The peak axial turbulence intensities in the shear layers were reduced by 15 and 30 % in moving across the plasma for the 150 and 300 W cases, respectively. The plasma did not alter the transverse intensities. The Reynolds shear stresses were reduced by 30 and 50 % for the 150 and 300 W cases. The corresponding Reynolds shear stress correlation coefficient was also reduced, which indicates that the large-scale structures were diminished. Finally, the plasma enhanced the turbulence decay in the zero-shear regions, where the power law decay $t^{-1/n}$ exponential factor $n$ decreased from 1.0 to 0.8.

2016 ◽  
Vol 62 ◽  
pp. 593-597
Author(s):  
Masaharu Matsubara ◽  
Shun Horii ◽  
Yoshiyuki Sagawa ◽  
Yuta Takahashi ◽  
Daisuke Saito

2017 ◽  
Vol 2017.54 (0) ◽  
pp. A034
Author(s):  
Shun HORII ◽  
Yu Imanishi ◽  
Yoshiyuki SAGAWA ◽  
Masaharu MATSUBARA

2018 ◽  
Vol 101 (2) ◽  
pp. 553-577 ◽  
Author(s):  
Stefano Rolfo ◽  
Konstantinos Kopsidas ◽  
Shahnurriman A. Rahman ◽  
Charles Moulinec ◽  
David R. Emerson

2019 ◽  
Vol 31 (4) ◽  
pp. 042001 ◽  
Author(s):  
A. Terzis ◽  
I. Zarikos ◽  
K. Weishaupt ◽  
G. Yang ◽  
X. Chu ◽  
...  

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