Dust devils are generally attributed to the near-surface conditions, usually the composite actions of the surface parameters, such as heat flux, wind shear and surface friction. Dust devil scale (DD-scale) numerical modeling has been developed to simulate the air flow of dust devils (Gu et al., 2006, 2008). In the DD-scale model, local vorticity is imposed on the boundary domain (the outer dust devil), as described by Lewellen et al. (2000). The computational domain is close to the size of convective plumes. The predicted physical parameters of Arizona-type dust devil, such as the maximum tangential velocity, the updraft velocity, the pressure drop in the inner core region and even the inverse flow at the top of the core region, approach the observation results, testifying the validity of the DD-scale modeling. The effects of buoyancy (ground temperature) and surface friction (surface momentum impact height) on the fine scale structure of dust devils are further examined in this paper. The results indicate that even with small temperature difference (weak buoyancy), severe dust devils may be formed by strong local vorticity, and that different surface momentum impact heights may result in different conic angles of corner flow.