Relationship between wall pressure and velocity-field sources

被引:58
作者
Chang, PA
Piomelli, U
Blake, WK
机构
[1] Hydromech Directorate, David Taylor Model Basin NSWC CD, W Bethesda, MD 20817 USA
[2] Univ Maryland, Dept Mech Engn, College Pk, MD 20742 USA
[3] Signatures Directorate, David Taylor Model Basin NSWC CD, W Bethesda, MD 20817 USA
关键词
D O I
10.1063/1.870202
中图分类号
O3 [力学];
学科分类号
08 ; 0801 ;
摘要
The objective of this investigation is to study the velocity-field sources for the fluctuating wall pressure, determine their locations in the boundary layer, and investigate their physics. The velocity-field sources and partial wall pressures were computed from a database generated by a direct numerical simulation of a low Reynolds number, fully developed, turbulent channel flow. Results show that the mean-shear (MS) and turbulence-turbulence (TT) partial pressures (pi(MS) and pi(TT), respectively) are the same order of magnitude. The buffer region dominates most of the wave number range; the viscous shear layer is significant at the highest wavenumbers; the buffer and logarithmic regions are important at low wavenumbers. Over most of the wavenumber range, the contribution from the buffer region is the dominant TT component; in the low-wavenumber range, the viscous shear layer, buffer region, and logarithmic region are significant; in the medium and high wavenumbers the viscous shear layer and buffer region dominate. The most important TT partial pressures are pi(23)(TT), pi(13)(TT) and pi(12)(TT) from the buffer region. It is conjectured that pi(23)(TT) and pi(13)(TT) may be generated by quasi-streamwise vortices. pi(12)(TT) may be due to near-wall shear layers and spanwise vortices. pi(23)(TT), pi(22)(TT) and pi(33)(TT) from the viscous shear layer are the dominant high-wavenumber partial pressures. (C) 1999 American Institute of Physics. [S1070-6631(99)02511-8].
引用
收藏
页码:3434 / 3448
页数:15
相关论文
共 50 条
[31]   IS THE VELOCITY-FIELD SUFFICIENT TO PERCEIVE HEADING [J].
WARREN, WH .
BULLETIN OF THE PSYCHONOMIC SOCIETY, 1990, 28 (06) :504-504
[32]   THE PECULIAR VELOCITY-FIELD IN FLATTENED SUPERCLUSTERS [J].
SZALAY, AS ;
SILK, J .
ASTROPHYSICAL JOURNAL, 1983, 264 (02) :L31-L35
[33]   STRUCTURE OF THE VELOCITY-FIELD IN THE VICINITY OF A CAUSTIC [J].
EREMENKO, VA .
PMM JOURNAL OF APPLIED MATHEMATICS AND MECHANICS, 1977, 41 (06) :1147-1151
[34]   VELOCITY-FIELD OF GROWING EAR CARTILAGE [J].
COX, RW ;
PEACOCK, MA .
JOURNAL OF ANATOMY, 1978, 126 (AUG) :555-566
[35]   ON THE VELOCITY-FIELD ASSOCIATED WITH POTENTIAL VORTICITY [J].
STAQUET, C ;
RILEY, JJ .
DYNAMICS OF ATMOSPHERES AND OCEANS, 1989, 14 (1-2) :93-123
[36]   THE VELOCITY-FIELD OF THE VIRGO CLUSTER OF GALAXIES [J].
TANAKA, KI .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 1985, 37 (02) :427-437
[37]   THE LOCAL ANOMALY OF THE EXTRAGALACTIC VELOCITY-FIELD [J].
GIRAUD, E .
ASTRONOMY & ASTROPHYSICS, 1990, 231 (01) :1-12
[38]   THEORY OF THE VELOCITY-FIELD RELATION IN ALGAAS [J].
BRENNAN, KF ;
PARK, DH ;
HESS, K ;
LITTLEJOHN, MA .
JOURNAL OF APPLIED PHYSICS, 1988, 63 (10) :5004-5008
[39]   THE TIDAL VELOCITY-FIELD IN THE LOCAL SUPERCLUSTER [J].
LILJE, PB ;
YAHIL, A ;
JONES, BJT .
ASTROPHYSICAL JOURNAL, 1986, 307 (01) :91-96
[40]   TEMPERATURE AND VELOCITY-FIELD BETWEEN COAXIAL HORIZONTAL CYLINDERS IN FREE CONVECTION [J].
SZOKEFAL.A ;
GAAL, I .
ACTA TECHNICA ACADEMIAE SCIENTIARUM HUNGARICAE, 1974, 78 (3-4) :445-456