Rayleigh-Darcy convection with hydrodynamic dispersion

被引:30
|
作者
Wen, Baole [1 ,2 ]
Chang, Kyung Won [2 ,3 ]
Hesse, Marc A. [1 ,2 ]
机构
[1] Univ Texas Austin, Inst Computat Engn & Sci, Austin, TX 78712 USA
[2] Univ Texas Austin, Jackson Sch Geosci, Dept Geol Sci, Austin, TX 78712 USA
[3] Sandia Natl Labs, Geomech Dept, Albuquerque, NM 87123 USA
来源
PHYSICAL REVIEW FLUIDS | 2018年 / 3卷 / 12期
关键词
CARBON-DIOXIDE DISSOLUTION; POROUS-MEDIUM; COLUMNAR CONVECTION; SOLUTAL-CONVECTION; NUMBER CONVECTION; CO2; DISSOLUTION; TENSOR FORM; STORAGE; FLOW; FLUID;
D O I
10.1103/PhysRevFluids.3.123801
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
We investigate the effect of hydrodynamic dispersion on convection in porous media by performing direct numerical simulations (DNS) in a two-dimensional Rayleigh-Darcy domain. Scaling analysis of the governing equations shows that the dynamics of this system are not only controlled by the classical Rayleigh-Darcy number based on molecular diffusion, Ra-m, and the domain aspect ratio, but also controlled by two other dimensionless parameters: the dispersive Rayleigh number Ra-d = H/alpha(t) and the dispersivity ratio r = alpha(l)/alpha(t), where H is the domain height and alpha(t )and alpha(l) are the transverse and longitudinal dispersivities, respectively. For Delta = Ra-d/Ra-m > O(1), the influence from the mechanical dispersion is minor; for Delta less than or similar to 0.02, however, the flow pattern is determined by Ra-d while the convective flux is F similar to c(Ra-d)Ra-m for large Ra-m. Our DNS results also show that the increase of mechanical dispersion, i.e., decreasing Ra-d, will coarsen the convective pattern by increasing the plume spacing. Moreover, the inherent anisotropy of mechanical dispersion breaks the columnar structure of the megaplumes at large Ra-m, if Ra-d < 5000. This results in a fan-flow geometry that reduces the convective flux.
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页数:18
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