Bolgiano scale in confined Rayleigh-Taylor turbulence

被引:53
作者
Boffetta, G. [1 ,2 ]
De Lillo, F. [1 ,2 ]
Mazzino, A. [3 ,4 ]
Musacchio, S. [5 ]
机构
[1] Univ Turin, Dipartimento Fis Gen, I-10125 Turin, Italy
[2] Univ Turin, INFN, I-10125 Turin, Italy
[3] Univ Genoa, Dipartimento Fis, INFN, I-16146 Genoa, Italy
[4] CNISM, I-16146 Genoa, Italy
[5] CNRS, Lab JA Dieudonne, UMR 6621, F-06108 Nice, France
关键词
turbulence simulation; turbulent convection; 3-DIMENSIONAL TURBULENCE; STRATIFIED TURBULENCE; NUMBER CONVECTION; BENARD CONVECTION; INSTABILITY; SIMULATIONS; ENERGY;
D O I
10.1017/jfm.2011.446
中图分类号
O3 [力学];
学科分类号
08 ; 0801 ;
摘要
We investigate the statistical properties of Rayleigh Taylor turbulence in a three-dimensional convective cell of high aspect ratio, in which one transverse side is much smaller that the others. By means of high-resolution numerical simulation we study the development of the turbulent mixing layer and the scaling properties of the velocity and temperature fields. We show that the system undergoes a transition from a three- to two-dimensional turbulent regime when the width of the turbulent mixing layer becomes larger than the scale of confinement. In the late stage of the evolution the convective flow is characterized by the coexistence of Kolmogorov-Obukhov and Bolgiano-Obukhov scaling at small and large scales, respectively. These regimes are separated by the Bolgiano scale, which is determined by the scale of confinement of the flow. Our results show that the emergence of the Bolgiano-Obukhov scaling in Rayleigh Taylor turbulence is connected to the onset of an upscale energy transfer induced by the geometrical constraint of the flow.
引用
收藏
页码:426 / 440
页数:15
相关论文
共 39 条
[11]   Rayleigh-Taylor turbulence in two dimensions [J].
Celani, A ;
Mazzino, A ;
Vozella, L .
PHYSICAL REVIEW LETTERS, 2006, 96 (13)
[12]   Turbulence in More than Two and Less than Three Dimensions [J].
Celani, Antonio ;
Musacchio, Stefano ;
Vincenzi, Dario .
PHYSICAL REVIEW LETTERS, 2010, 104 (18)
[13]   Resonant interactions in rotating homogeneous three-dimensional turbulence [J].
Chen, QN ;
Chen, SY ;
Eyink, GL ;
Holm, DD .
JOURNAL OF FLUID MECHANICS, 2005, 542 :139-164
[14]   Phenomenology of Rayleigh-Taylor turbulence [J].
Chertkov, M .
PHYSICAL REVIEW LETTERS, 2003, 91 (11)
[16]   Self-similarity and internal structure of turbulence induced by Rayleigh-Taylor instability [J].
Dalziel, SB ;
Linden, PF ;
Youngs, DL .
JOURNAL OF FLUID MECHANICS, 1999, 399 :1-48
[17]  
Frisch U., 1995, Turbulence: The Legacy of A
[18]   Filamentary structure on the Sun from the magnetic Rayleigh-Taylor instability [J].
Isobe, H ;
Miyagoshi, T ;
Shibata, K ;
Yokoyama, T .
NATURE, 2005, 434 (7032) :478-481
[19]   TWO-DIMENSIONAL TURBULENCE [J].
KRAICHNAN, RH ;
MONTGOMERY, D .
REPORTS ON PROGRESS IN PHYSICS, 1980, 43 (05) :547-619
[20]   Small-Scale Properties of Turbulent Rayleigh-Benard Convection [J].
Lohse, Detlef ;
Xia, Ke-Qing .
ANNUAL REVIEW OF FLUID MECHANICS, 2010, 42 :335-364