A grid nesting method for large-eddy simulation of planetary boundary-layer flows

被引:152
作者
Sullivan, PP [1 ]
McWilliams, JC [1 ]
Moeng, CH [1 ]
机构
[1] UNIV CALIF LOS ANGELES,DEPT ATMOSPHER SCI,LOS ANGELES,CA 90024
关键词
D O I
10.1007/BF00119016
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
A method for performing nested grid calculations with a large-eddy simulation code is described. A common numerical method is used for all meshes, and the grid architecture consists of a single outer or coarse grid, and nested or fine grids, which overlap in some common region. Inter-grid communication matches the velocity, pressure and potential temperature fields in the overlap region. Resolved and sub-grid scale (SGS) turbulent fluxes and kinetic energy on the fine grid are averaged to the coarse grid using a conservation rule equivalent to Germane's identity used to develop dynamic SGS models. Simulations of a slightly convective, strong shear planetary boundary layer were carried out with varying surface-layer resolutions. Grid refinements in the (x, y, z) directions of up to (5, 5, 2) limes were employed. Two-way interaction solutions on the coarse and fine meshes are successfully matched in the overlap region on an instantaneous basis, and the turbulent motions on the fine grid blend smoothly into the coarse grid across the grid interface. With surface-layer grid nesting, significant increases in resolved eddy fluxes and variances are found. The energy-scale content of the vertical velocity, and hence vertical turbulent fluxes, appear to be most influenced by increased grid resolution. Vertical velocity spectra show that the dominant scale shifts towards higher wavenumbers (smaller scales) and the magnitude of the peak energy is increased by more than a factor of 3 with finer resolution. Outside of the nested region the average heat and momentum fluxes and spectra are slightly influenced by the fine resolution in the surface layer. From these results we conclude that fine resolution is required to resolve the details of the turbulent motions in the surface layer. Al the same time, however, increased resolution in the surface layer does not appreciably alter the ensemble statistics of the resolved and SGS motions outside of the nested region.
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页码:167 / 202
页数:36
相关论文
共 30 条
[1]   LARGE-EDDY SIMULATION OF A NEUTRALLY STRATIFIED BOUNDARY-LAYER - A COMPARISON OF 4 COMPUTER CODES [J].
ANDREN, A ;
BROWN, AR ;
GRAF, J ;
MASON, PJ ;
MOENG, CH ;
NIEUWSTADT, FTM ;
SCHUMANN, U .
QUARTERLY JOURNAL OF THE ROYAL METEOROLOGICAL SOCIETY, 1994, 120 (520) :1457-1484
[2]   MULTIDOMAIN SIMULATIONS OF THE TIME-DEPENDENT NAVIER-STOKES EQUATIONS - BENCHMARK ERROR ANALYSIS OF SOME NESTING PROCEDURES [J].
CLARK, TL ;
HALL, WD .
JOURNAL OF COMPUTATIONAL PHYSICS, 1991, 92 (02) :456-481
[3]  
CLARK TL, 1984, J ATMOS SCI, V41, P327
[4]   APPLICATION OF THE SPECTRAL MULTIDOMAIN METHOD TO THE NAVIER-STOKES EQUATIONS [J].
DANABASOGLU, G ;
BIRINGEN, S ;
STREETT, CL .
JOURNAL OF COMPUTATIONAL PHYSICS, 1994, 113 (02) :155-164
[5]   STRATOCUMULUS-CAPPED MIXED LAYERS DERIVED FROM A 3-DIMENSIONAL MODEL [J].
DEARDORFF, JW .
BOUNDARY-LAYER METEOROLOGY, 1980, 18 (04) :495-527
[6]   A DYNAMIC SUBGRID-SCALE EDDY VISCOSITY MODEL [J].
GERMANO, M ;
PIOMELLI, U ;
MOIN, P ;
CABOT, WH .
PHYSICS OF FLUIDS A-FLUID DYNAMICS, 1991, 3 (07) :1760-1765
[7]  
GERZ T, 1994, PHYS FLUIDS, V3, P1242
[8]  
Grell GA, 1994, NCARTN398 STR
[9]  
Henderson R., 1991, Journal of Scientific Computing, V6, P79, DOI 10.1007/BF01062115
[10]  
KLEMP J, 1983, MON WEA REV, V11, P430