\begin{table}%T1
\caption{Parameters used for the calculations performed in this article. The values should be appropriate for the solar wind at 1 AU 
heliocentric distance.}
\label{tab1}
%\centering
\par
\begin{tabular}{lll}
\hline\hline
\vphantom{$1 \over 2$} $ \textnormal{Parameter}						$ & $ \textnormal{Symbol}	$ & $ \textnormal{Value}	$ \\ 
\hline
\vphantom{$1 \over 2$} $ \textnormal{Inertial range spectral index}		$ & $ 2 \nu				$ & $ 5/3					$ \\
\vphantom{$1 \over 2$} $ \textnormal{Dissipation range spectral index}	$ & $ p					$ & $ 3 						$ \\
\vphantom{$1 \over 2$} $ \textnormal{Energy range spectral index}	$ & $ q					$ & $ 1.07 					$ \\
\vphantom{$1 \over 2$} $ \textnormal{Alfv\'en speed}					$ & $ v_{\rm A}			$ & $ 33.5 \;$km~s$^{-1}$				 \\
\vphantom{$1 \over 2$} $ \textnormal{Cut-off wavenumber}			$ & $ k_{\min}			$ & $ 10^{-4} \; l_{\rm slab}			$ \\
\vphantom{$1 \over 2$} $ \textnormal{Bendover scale}				$ & $ l_{\rm slab}			$ &  0.030~AU				 \\
\vphantom{$1 \over 2$} $ \textnormal{Dissipation wavenumber}		$ & $ k_{\rm d}			$ & $ 3 \times 10^{6} $~(AU)$^{-1}	$ \\
\vphantom{$1 \over 2$} $ \textnormal{Mean field}					$ & $ B_0				$ & $ 4.12 \; nT				$ \\
\vphantom{$1 \over 2$} $ \textnormal{Turbulence strength}			$ & $ \delta B / B_0		$ & $ 1						$ \\
\hline
\end{tabular}
\end{table}