\begin{table}%T1
      \caption{Results of calculations.}\label{t1}
%\centerline
{
\begin{tabular}{llllll}
\hline\hline
Model &$\Delta {\it SW}^{a}$ &$\Delta$ TS (upwind)$^b$ &  $\Delta$ TS
(downwind) & $\Delta$ HP (upwind)
& $R(BS)_{\rm time} -R(BS)_{\rm stationary}^c$ \\
\hline
This paper             &2&14 AU & 25 AU&  4 AU & 3 AU  \\
Zank \& Muller (\cite{Zank03}) &2& 7 AU & 50 AU & 6 AU & n/a  \\
Scherer \& Fahr (2003)& 2.67$^{d}$ &$\sim$16 AU & n/a$^e$ & n/a & $>$15 AU  \\
\hline
\end{tabular}}
\par
\medskip
$^{{a}}$  $\Delta {\it SW}$ notes the ratio of maximum to
minimum the solar wind dynamic pressure.\\
$^{{b}}$ 
$\Delta = R_{\max} - R_{\min}$ is the difference between maximum and
minimum distances of the TS, HP and BS during the solar cycle.\\
$^{{c}}$  $R(BS)_{\rm time} -R(BS)_{\rm stationary}$  is the
difference between mean location of the BS during the
time-dependent calculations and the stationary solution.\\
$^{{d}}$  Model "Sin~800'' in Fig.~4a in Scherer \&
Fahr (\cite{Scherer03b}).\\
$^{{e}}$  n/a means that we
were unable to find the corresponding value from the results
presented in the cited paper.
\end{table}