\begin{table}%t1
  \caption{\label{tab:SpotSolutions}Parameters of characteristic spot solutions discussed in the text; longitudes and colatitudes are given for the spot center.}
%\centerline
{                  
\begin{tabular}{lcccccc}
\hline \hline
Model$^a$
       & Long.   
       & Colat.
       & Radius
       & Flux$^b$     
       & $\chi^2$
       & Area$^c$ \\
      \hline 
    BC & $216.4\degr$  &  $75.0\degr$  &  $7.8\degr$  & $0.75$  &  0.8 & 0.45\%  \\   
    BN & $216.5\degr$  &  $70.0\degr$  &  $9.5\degr$  & $0.75$  &  1.4 & 0.55\%  \\
    BS & $216.2\degr$  &  $80.0\degr$  &  $8.5\degr$  & $0.75$  &  1.2 & 0.47\%  \\
    DN  & $216.7\degr$  &  $71.0\degr$  &  $4.8\degr$  & $0.3$  &  1.7 & 0.18\%  \\
    DS  & $216.2\degr$  &  $81.0\degr$  &  $4.8\degr$  & $0.3$  &  1.9 & 0.18\%  \\
    DEQ  & $216.3\degr$  &  $94.0\degr$  &  $15.3\degr$  & $0.3$  &  1.6 & 0.72\%  \\
      \hline
    \end{tabular}}
    \medskip
 $^a$ BC, BN and BS stand for ``bright central'', ``bright north'' and ``bright south'', respectively. They describe spots with colatitudes close to 
the center of the planetary disk.
DN and DS stand for ``north'' and ``south'' dark spot solutions, respectively;
DEQ represents a ``dark'' spot centered below the equator.   $^b$ Relative to the photosphere.    $^c$ Fraction of total stellar surface.              
\end{table}