Table 1: Overview of model parameters. From left to right, the columns indicate: planet mass in ${{M}_\oplus }$, value of the adiabatic exponent ($\Gamma =1$means a locally isothermal equation of state), viscosity parameter $\alpha $, radiation flag, accretion flag and the number of refinement levels. When $n_{\rm lev}$ levels of refinement are used, the local resolution within a distance of 2H from the planet is a factor  $2^{n_{\rm lev}}$ higher than the base resolution of $\Delta r=0.0082~r_{\rm p}$. For the local models, the indicated resolution is valid for the whole computational domain.
$M_{\rm p}$ ( ${{M}_\oplus }$) $\Gamma$ $\alpha $ FLD Acc $n_{\rm lev}$ $\mathcal{S}$ Comments
0.6 1 0.004 n y 5 0  
5 1 0.004 n y 4 0  
5 1 0.004 n y 3 0  
5 1 0.004 n y 2 0  
40 1 0.004 n y 3 0  
320 1 0.004 n y 2 0  
5 1.005 0 n y 4 -0.9925  
5 1.01 0 n y 4 -0.9850  
5 1.005 0 n y 3 -0.9925  
5 1.01 0 n y 3 -0.9850  
0.6 1.4 0 y n 5 -0.4  
0.6 1.4 0 y y 5 -0.4  
0.6 1.4 0 y n 4 -0.4  
0.6 1.4 0 y y 4 -0.4  
5 1.4 0 y n 4 -0.4  
5 1.4 0 y y 4 -0.4  
5 1.4 0 y n 3 -0.4  
5 1.4 0 y y 3 -0.4  
5 1.4 0 y n 2 -0.4  
5 1.4 0 y y 2 -0.4  
5 1.4 0 y n 4 -0.4 10 times lower density
5 1.4 0 y n 4 -0.4 100 times lower density
5 1.4 0 n n 4 -0.4 local model
5 1 0 n n 4 0 local model
5 1.4 0 n n 4 -0.2 local model
5 1.4 0 n n 4 0.2 local model
5 1.4 0 n n 4 0.4 local model

Source LaTeX | All tables | In the text