\begin{table}%t1
\par
\caption{\label{table_A}Summary of the different cases studied and the values of $R_{\rm e}$ and $C_\Omega$ used in the 2D Babcock-Leighton models.}  
\small%\centerline
{
\begin{tabular}{cccccc}
 \hline \hline 
  Case    &   $\Omega_{0}/\Omega_{\rm S}$ &   MCKE/$10^4$ & $v_\theta^{\rm scale}$ & $\vec{R}_{\rm e}/10^2$ & $\vec{C}_{\Omega}/10^5$ \\
   \hline
G0.25   &  0.25   &  23.4   &  28.7      &       20.1    &    0.351  \\ 
G0.5   &  0.5    &  16.2    &  23.9      &       16.7    &    0.702  \\  
G0.6   &  0.6   &  12.3     &  20.9      &       14.6    &    0.842  \\ 
G0.75   &  0.75    &  4.75    &  12.9      &       9.06     &    1.05  \\  
G0.9   &  0.9      &  3.09   &  10.4      &       7.29     &    1.26  \\  
G1     &  1   &  2.84       &  10.0      &       7.00     &    1.40  \\  
G1.25    &  1.25    &  2.18    &  8.76       &       6.13     &    1.75  \\  
G1.5    &  1.5   &  1.98      &  8.36    &       5.85     &    2.11  \\  
G1.75    &  1.75      &  1.68  &  7.70       &       5.39     &    2.46  \\  
G2       &  2      &  1.52     &  7.33      &       5.13     &    2.81  \\  
G3       &  3      &  1.11     &  6.25       &       4.38     &    4.21  \\ 
G4       &  4      &  0.767      &  5.20       &       3.64     &    5.62  \\  
G5       &  5      &  0.711      &  5.01       &       3.51     &    7.02  \\ 
G6       &  6      &  0.626      &  4.70       &       3.29     &    8.42  \\ 
G7       &  7     &  0.497       &  4.18       &       2.93     &    9.83  \\ 
G10      &  10    &  0.359       &  3.56       &       2.49     &    14.0  \\ 
\hline
\end{tabular} }
\smallskip
The value of $\eta_{\rm t}$ is fixed to $10^{11} ~~ \rm cm^2~s^{-1}$ and the value of $s_0$ is fixed to $50 ~~ \rm cm~s^{-1}$.
The stellar rotation rate $\Omega_{0}$ is given in terms of the solar rotation rate $\Omega_{\rm S}$.
$v_\theta^{\rm scale}$ represents the amplitude of $v_\theta$ at the surface at $45^{\circ}$ and is imposed equal to $10 ~~ \rm m~s^{-1}$ for case G1,
representing the reference solar mean field dynamo model.\vspace{-2mm}
\end{table}