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In this paper, the traveling crossflow instability in the boundary layer on the windward side of a delta wing is studied. The experiments are carried out in a Mach 6 low-noise wind tunnel, with the angles of attack of the model being 5° and 10°, and the Reynolds number being in a range of 2.43 × 106–14.21 × 106 m–1. The wall fluctuation pressure is measured by fast-response Kulite pressure transducers. The power spectrum density (PSD) analysis is conducted to obtain the disturbance waves' development process in the boundary layer. The temperature-sensitive paints (TSPs) and nano-tracer based planar laser scattering (NPLS) technique are also used. From the TSP results, the boundary layer transition near the leading edge of the delta wing is smooth and parallel to the leading edge. A peak around 10 kHz in power spectrum density is detected by the fast-response pressure sensor, which may be caused by the traveling crossflow waves. To verify this dominant mode, an NPLS image in the plane of n = 36 mm is obtained. The shapes of vortex structures correspond to the shapes of the crossflow vortices from the numerical simulation. Only when the boundary layer is laminar can the traveling crossflow wave signal be observed from the PSD curves. When the boundary layer is at a transitional or turbulent phase, the low-frequency component is dominant in the PSD curve. With the increase of Reynolds number, the characteristic frequency of the crossflow wave increases, and the wave’s amplitude first increases and then decreases. Moreover, the angle of attack effect is obtained. The increasing of the angle of attack can make the traveling crossflow wave grow faster and saturate, attenuate at the position closer to the leading edge of the delta wing or at a lower Reynolds number. By sensor pairs composed of three Kulite transducers, the phase velocity and the propagation angle of the traveling crossflow wave are investigated. The dimensionless phase velocities of the traveling wave are in ranges of 0.24–0.26 and 0.26–0.32 at 5° and 10° angles of attack, respectively. The propagation angles are at 50°–60° and 40°–55° at the angles of attack of 5° and 10°, respectively. At a larger angle of attack, the traveling wave’s propagation angel is smaller, but the phase velocity is bigger. It may be because the spanwise pressure gradient is higher at a larger angle of attack, and then the crossflow velocity is stronger.
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Keywords:
- crossflow instability /
- hypersonic flow /
- delta wing /
- power spectrum density
[1] Schneider S P 2004 Prog. Aerosp. Sci. 40 1Google Scholar
[2] Mack L M 1975 AIAA J. 13 278Google Scholar
[3] Saric W S, Reed H L, White E B 2003 Annu. Rev. Fluid Mech. 35 413Google Scholar
[4] Deyhle H, Bippes H 1996 J. Fluid Mech. 316 73Google Scholar
[5] Poll D I A 1985 J. Fluid Mech. 150 329Google Scholar
[6] Malik M R, Li F, Choudhari M, Chang C L 1999 J. Fluid Mech. 399 85Google Scholar
[7] Edelman J B, Schneider S P 2018 AIAA J. 56 182Google Scholar
[8] Craig S A, Saric W S 2016 J. Fluid Mech. 808 224Google Scholar
[9] Corke T, Arndt A, Matlis E, Semper M 2018 J. Fluid Mech. 856 822Google Scholar
[10] Arndt A, Corke T, Matlis E, Semper M 2020 J. Fluid Mech. 887 A30Google Scholar
[11] Moyes A J, Paredes P, Kocian T S, Reed H L 2017 J. Fluid Mech. 812 370Google Scholar
[12] Xu G, Chen J, Liu G, Dong S, Fu S 2019 J. Fluid Mech. 873 914Google Scholar
[13] Ward C A C 2014 Ph. D. Dissertation (Indiana: Pudue University)
[14] Borg M P, Kimmel R L, Stanfield S 2013 43rd Fluid Dynamics Conference San Diego, CA, June 24−27, 2013 p2737
[15] Borg M P, Kimmel R L, Stanfield S 2015 J. Spacecraft Rockets 52 664Google Scholar
[16] Li F, Choudhari M, Chang C L, White J 2010 10th AIAA/ASME Joint Thermophysics and Heat Transfer Conference Chicago, Illinois, June 28−July 1, 2010 p4643
[17] Niu H B, Yi S H, Liu X L, Lu X G, He L 2019 AIAA J. 57 5566Google Scholar
[18] 刘小林, 易仕和, 牛海波, 陆小革, 赵鑫海 2018 物理学报 67 174701Google Scholar
Liu X L, Yi S H, Niu H B, Lu X G, Zhao X H 2018 Acta Phys. Sin. 67 174701Google Scholar
[19] 刘小林, 易仕和, 牛海波, 陆小革 2018 物理学报 67 214701Google Scholar
Liu X L, Yi S H, Niu H B, Lu X G 2018 Acta Phys. Sin. 67 214701Google Scholar
[20] Niu H, Yi S, Liu X, Lu X, Gang D 2020 Chin. J. Aeronaut. 33 1889Google Scholar
[21] Niu H, Yi S, Liu X, Huo J, Jin L 2020 Int. J. Heat Fluid Flow 86 108746Google Scholar
[22] Lu X, Yi S, He L, Liu X, Niu H 2020 Fluid Dyn. 55 111Google Scholar
[23] Cook W J, Felderman E J 1970 AIAA J. 8 1366Google Scholar
[24] Zhao Y X, Yi S H, Tian L F, He L, Cheng Z Y 2009 Sci. China 52 3640Google Scholar
[25] He L, Yi S H, Zhao Y X, Tian L F, Chen Z 2011 Chin. Sci. Bull. 56 489Google Scholar
[26] Liu X L, Yi S H, Xu X W, Shi Y, Ouyang T C, Xiong H 2019 Phys. Fluids 31 074108Google Scholar
[27] 陆昌根, 朱晓清, 沈露予 2017 物理学报 66 204702Google Scholar
Lu C G, Zhu X Q, Shen L Y 2017 Acta Phys. Sin. 66 204702Google Scholar
[28] 沈露予陆昌根 2017 物理学报 66 014703Google Scholar
Shen L Y, Lu C G 2017 Acta Phys. Sin. 66 014703Google Scholar
[29] Tian L, Yi S, Zhao Y, He L, Cheng Z 2009 Sci. China, Ser. G 52 1357Google Scholar
[30] 赵磊 2016 博士学位论文 (天津: 天津大学)
Zhao L 2016 Ph. D. Dissertation (Tianjin: Tianjin University) (in Chinese)
[31] Poggie J, Kimmel R L, Schwoerke S N 2000 AIAA J. 38 251Google Scholar
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表 1 Kulite阵列的坐标
Table 1. Coordinate of the two Kulite arrays.
Sensor No. x/mm y/mm K3 403.88 59.14 K5 406.88 56.14 K6 409.88 56.14 K7 300 50.84 K8 300 46.84 K9 302 52.84 -
[1] Schneider S P 2004 Prog. Aerosp. Sci. 40 1Google Scholar
[2] Mack L M 1975 AIAA J. 13 278Google Scholar
[3] Saric W S, Reed H L, White E B 2003 Annu. Rev. Fluid Mech. 35 413Google Scholar
[4] Deyhle H, Bippes H 1996 J. Fluid Mech. 316 73Google Scholar
[5] Poll D I A 1985 J. Fluid Mech. 150 329Google Scholar
[6] Malik M R, Li F, Choudhari M, Chang C L 1999 J. Fluid Mech. 399 85Google Scholar
[7] Edelman J B, Schneider S P 2018 AIAA J. 56 182Google Scholar
[8] Craig S A, Saric W S 2016 J. Fluid Mech. 808 224Google Scholar
[9] Corke T, Arndt A, Matlis E, Semper M 2018 J. Fluid Mech. 856 822Google Scholar
[10] Arndt A, Corke T, Matlis E, Semper M 2020 J. Fluid Mech. 887 A30Google Scholar
[11] Moyes A J, Paredes P, Kocian T S, Reed H L 2017 J. Fluid Mech. 812 370Google Scholar
[12] Xu G, Chen J, Liu G, Dong S, Fu S 2019 J. Fluid Mech. 873 914Google Scholar
[13] Ward C A C 2014 Ph. D. Dissertation (Indiana: Pudue University)
[14] Borg M P, Kimmel R L, Stanfield S 2013 43rd Fluid Dynamics Conference San Diego, CA, June 24−27, 2013 p2737
[15] Borg M P, Kimmel R L, Stanfield S 2015 J. Spacecraft Rockets 52 664Google Scholar
[16] Li F, Choudhari M, Chang C L, White J 2010 10th AIAA/ASME Joint Thermophysics and Heat Transfer Conference Chicago, Illinois, June 28−July 1, 2010 p4643
[17] Niu H B, Yi S H, Liu X L, Lu X G, He L 2019 AIAA J. 57 5566Google Scholar
[18] 刘小林, 易仕和, 牛海波, 陆小革, 赵鑫海 2018 物理学报 67 174701Google Scholar
Liu X L, Yi S H, Niu H B, Lu X G, Zhao X H 2018 Acta Phys. Sin. 67 174701Google Scholar
[19] 刘小林, 易仕和, 牛海波, 陆小革 2018 物理学报 67 214701Google Scholar
Liu X L, Yi S H, Niu H B, Lu X G 2018 Acta Phys. Sin. 67 214701Google Scholar
[20] Niu H, Yi S, Liu X, Lu X, Gang D 2020 Chin. J. Aeronaut. 33 1889Google Scholar
[21] Niu H, Yi S, Liu X, Huo J, Jin L 2020 Int. J. Heat Fluid Flow 86 108746Google Scholar
[22] Lu X, Yi S, He L, Liu X, Niu H 2020 Fluid Dyn. 55 111Google Scholar
[23] Cook W J, Felderman E J 1970 AIAA J. 8 1366Google Scholar
[24] Zhao Y X, Yi S H, Tian L F, He L, Cheng Z Y 2009 Sci. China 52 3640Google Scholar
[25] He L, Yi S H, Zhao Y X, Tian L F, Chen Z 2011 Chin. Sci. Bull. 56 489Google Scholar
[26] Liu X L, Yi S H, Xu X W, Shi Y, Ouyang T C, Xiong H 2019 Phys. Fluids 31 074108Google Scholar
[27] 陆昌根, 朱晓清, 沈露予 2017 物理学报 66 204702Google Scholar
Lu C G, Zhu X Q, Shen L Y 2017 Acta Phys. Sin. 66 204702Google Scholar
[28] 沈露予陆昌根 2017 物理学报 66 014703Google Scholar
Shen L Y, Lu C G 2017 Acta Phys. Sin. 66 014703Google Scholar
[29] Tian L, Yi S, Zhao Y, He L, Cheng Z 2009 Sci. China, Ser. G 52 1357Google Scholar
[30] 赵磊 2016 博士学位论文 (天津: 天津大学)
Zhao L 2016 Ph. D. Dissertation (Tianjin: Tianjin University) (in Chinese)
[31] Poggie J, Kimmel R L, Schwoerke S N 2000 AIAA J. 38 251Google Scholar
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