We investigate the effect of 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, , and the domain aspect ratio, but also controlled by two other dimensionless parameters: the dispersive Rayleigh number and the dispersivity ratio $r = \alpha_l/\alpha_tH\alpha_t\alpha_l\Delta = Ra_d/Ra_m > O(1)\Delta \ll 1Ra_d$ while the convective flux is for large , but with a prefactor that has a non-monotonic dependence on . Our DNS results also show that the increase of mechanical dispersion, i.e. decreasing , will coarsen the convective pattern by increasing the plume spacing. Moreover, the inherent anisotropy of mechanical dispersion breaks the columnar structure of the mega-plumes at large , if . This results in a fan-flow geometry that reduces the convective flux.

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