Accelerated evolution of convective simulations

被引:11
作者
Anders, Evan H. [1 ,2 ]
Brown, Benjamin P. [1 ,2 ]
Oishi, Jeffrey S. [3 ]
机构
[1] Univ Colorado, Dept Astrophys & Planetary Sci, Boulder, CO 80309 USA
[2] Lab Atmospher & Space Phys, Boulder, CO 80303 USA
[3] Bates Coll, Dept Phys & Astron, Lewiston, ME 04240 USA
关键词
RAYLEIGH-BENARD CONVECTION; COMPRESSIBLE CONVECTION; THERMAL-CONVECTION; HEAT-FLUX; NUMBER; TRANSPORT; EQUATIONS; REGIMES; PRANDTL; SCALE;
D O I
10.1103/PhysRevFluids.3.083502
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
High-Peclet-number, turbulent convection is a classic system with a large timescale separation between flow speeds and the thermal relaxation time. In this paper, we present a method of fast-forwarding through the long thermal relaxation of convective simulations, and we test the validity of this method. This accelerated evolution (AE) method involves measuring the dynamics of convection early in a simulation and using its characteristics to adjust the mean thermodynamic profile within the domain toward its evolved state. We study Rayleigh-Benard convection as a test case for AE. Evolved flow properties of AE solutions are measured to be within a few percent of solutions which are reached through standard evolution (SE) over a full thermal diffusion timescale. At the highest values of the Rayleigh number at which we compare SE and AE, we find that AE solutions require roughly an order of magnitude fewer computing hours to evolve than SE solutions.
引用
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页数:16
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