Numerical Analysis of Nonlocal Convection-Comparison with Three-dimensional Numerical Simulations of Efficient Turbulent Convection

被引:6
|
作者
Cai, Tao [1 ,2 ]
机构
[1] Macau Univ Sci & Technol, Lunar & Planetary Sci Lab, Macau, Peoples R China
[2] Sun Yat Sen Univ, Sch Math, 135 Xingang Xi Rd, Guangzhou 510275, Guangdong, Peoples R China
来源
ASTROPHYSICAL JOURNAL | 2018年 / 868卷 / 01期
关键词
convection; methods: numerical; stars: interiors; turbulence; QUASI-NORMALITY HYPOTHESIS; MIXING-LENGTH CONVECTION; REYNOLDS STRESS APPROACH; COMPRESSIBLE CONVECTION; INHOMOGENEOUS FLOWS; DEEP CONVECTION; CORE OVERSHOOT; MODELS; CLOSURE; APPROXIMATION;
D O I
10.3847/1538-4357/aae1b3
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We compare 1D nonlocal turbulent convection models with 3D hydrodynamic numerical simulations. We study the validity of closure models and turbulent coefficients by varying the Prandtl number, the Peclet number, and the depth of the convection zone. Four closure models of the fourth-order moments are evaluated with the 3D simulation data. The performance of the closure models varies among different cases and different fourth-order moments. We solve the dynamic equations of moments together with equations of the thermal structure. Unfortunately, we cannot obtain steady-state solutions when these closure models of fourth-order moments are adopted. In contrast, the numerical solutions of the down-gradient approximations of the third-order moments are robust. We calibrate the coefficients of the 1D down-gradient model from the 3D simulation data. The calibrated coefficients are more robust in cases of deep convection zones. Finally, we have compared the 1D steady-state solutions with the 3D simulation results. The 1D model has captured many features that appear in the 3D simulations: (1) del - del(a) has a U-shape with a minimum value at the lower part of the convection zone; (2) there exists a bump for del - del(a) near the top of the convection zone when the Peclet number is large; and (3) the temperature gradient can be sub-adiabatic due to the nonlocal effect. However, aside from these similarities, the prediction on the kinetic energy flux is unsatisfactory.
引用
收藏
页数:29
相关论文
共 50 条
  • [1] Numerical Investigation of Spectrums of Three-Dimensional Turbulent Convection
    Palymskiy, I. B.
    IZVESTIYA SARATOVSKOGO UNIVERSITETA NOVAYA SERIYA-MATEMATIKA MEKHANIKA INFORMATIKA, 2010, 10 (01): : 62 - 71
  • [2] Three-dimensional numerical MHD simulations of solar convection
    Ustyugov, S. D.
    HYPERBOLIC PROBLEMS: THEORY, NUMERICS, APPLICATIONS: PROCEEDINGS OF THE 11TH INTERNATIONAL CONFERENCE ON HYPERBOLIC PROBLEMS, 2008, : 1061 - 1068
  • [3] NUMERICAL SIMULATIONS OF NONLOCAL CONVECTION
    XIONG, DR
    ASTRONOMY & ASTROPHYSICS, 1989, 213 (1-2) : 176 - 182
  • [4] Three-dimensional simulations of turbulent compressible convection
    Porter, DH
    Woodward, PR
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2000, 127 (01): : 159 - 187
  • [5] Physical-numerical parameters in turbulent simulations of natural convection on three-dimensional square plates
    Verderio Junior, Silvio Aparecido
    Scalon, Vicente Luiz
    Oliveira, Santiago del Rio
    Ito, Mario Cesar
    INTERNATIONAL JOURNAL OF NUMERICAL METHODS FOR HEAT & FLUID FLOW, 2022, 32 (02) : 761 - 784
  • [6] Three-dimensional numerical simulations of crustal deformation and subcontinental mantle convection
    Moresi, LN
    Lenardic, A
    EARTH AND PLANETARY SCIENCE LETTERS, 1997, 150 (3-4) : 233 - 243
  • [7] Three-dimensional numerical simulations of free convection in a layered porous enclosure
    Guerrero-Martinez, Fernando J.
    Younger, Paul L.
    Karimi, Nader
    Kyriakis, Sotirios
    INTERNATIONAL JOURNAL OF HEAT AND MASS TRANSFER, 2017, 106 : 1005 - 1013
  • [8] Three-dimensional numerical simulations of compressible solar convection in Cartesian geometry
    Elliott, JR
    ASTROPHYSICAL JOURNAL, 2000, 539 (01): : 469 - 479
  • [9] THREE-DIMENSIONAL SPECTRAL SIMULATIONS OF ANELASTIC TURBULENT CONVECTION
    Penev, Kaloyan
    Barranco, Joseph
    Sasselov, Dimitar
    ASTROPHYSICAL JOURNAL, 2011, 734 (02):
  • [10] TURBULENT MIXING AND LAYER FORMATION IN DOUBLE-DIFFUSIVE CONVECTION: THREE-DIMENSIONAL NUMERICAL SIMULATIONS AND THEORY
    Rosenblum, E.
    Garaud, P.
    Traxler, A.
    Stellmach, S.
    ASTROPHYSICAL JOURNAL, 2011, 731 (01):