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\titlerunning{}
\authorrunning{P. Jakab and A. Brandenburg}
\title{The effect of a dynamo-generated field on the Parker wind}
\author{P. Jakab\inst{1,2} and A. Brandenburg\inst{1,3,4,5}
}
\institute{
Nordita, KTH Royal Institute of Technology and Stockholm University,
Roslagstullsbacken 23, 10691 Stockholm, Sweden
\and
Department of Nuclear Physics and Subnuclear Physics,
Pavol Jozef Safarik University in Kosice, 
Jesenna 5, 041 54 Kosice, Slovakia 
\and
Department of Astronomy, AlbaNova University Center,
Stockholm University, 10691 Stockholm, Sweden
\and
JILA and Laboratory for Atmospheric and Space Physics,
University of Colorado, Boulder, CO 80303, USA
\and
McWilliams Center for Cosmology \& Department of Physics,
Carnegie Mellon University, Pittsburgh, PA 15213, USA
}
\date{\today,~ $ $Revision: 1.2 $ $}
\begin{document}

\abstract{
}{
}{
}{
}{
\keywords{Sun: sunspots -- Sun: dynamo -- turbulence --  magnetohydrodynamics (MHD) -- hydrodynamics }
}

\maketitle

\begin{table}[b!]\caption{
Summary of the simulations discussed in this paper.
In all cases we use $w_\alpha=0.02$ and $\dot{M}=1$ is chosen.
We always take $r_{\rm in}=0.1$ and $R=0.2$,
and $\tilde\nu_{\rm t}==8\times10^{-5}$, and $n=6$.
}\vspace{12pt}\centerline{\begin{tabular}{crcccccc}
Run & $\tilde{\alpha}$ & $Q_\alpha$ & $\tilde{\Omega}$ & $P_{\rm cyc}$ &
$\meanB_{\rm sat}$ & $C_\alpha$ & $C_\Omega$ \\
\hline
%     alp       Q
A  &$ 0.05$& $10^{-2}$ &0.2 & 41.0 &$2.4\times10^{-5}$ & 125  & 75 \\%M4096a2_Q001_Om02 (*,osc, om=0.1534, P=41)
B1 &$ 0.05$& $10^{-2}$ & 1  & ---  &$2.4\times10^{-5}$ & & \\%M4096a1_Q001_Om1 (**)
B2 &$ 0.1 $& $ 0     $ & 1  & ---  &$2.4\times10^{-5}$ & & \\%M4096c1_Q001_Om1 (*)
B3 &$ 0.1 $& $10^{-2}$ & 1  & ---  &$2.4\times10^{-5}$ & 250 & 375 \\%M4096b1_Q001_Om1 (*)
C1 &$ 0.05$& $10^{-2}$ & 10 & ---  &$8.0\times10^{-3}$ & & \\%M4096a17_Q001_Om10 (**)
C2 &$ 0.05$& $10^{-1}$ & 10 & ---  &$2.8\times10^{-3}$ & & \\%M4096a17_Q01_Om10
C3 &$-0.05$& $10^{-2}$ & 10 & ---  &$2.4\times10^{-5}$ & & \\%M4096a17_mQ001_Om10
C4 &$ 0.1 $& $10^{-1}$ & 10 & ---  &$2.4\times10^{-2}$ & 250 & 3750 \\%M4096a13_Q01_Om10 (***)
C5 &$-0.1$ & $10^{-2}$ & 10 & ---  &$2.4\times10^{-5}$ & & \\%M4096b17_mQ001_Om10
\label{Tab2}\end{tabular}}\end{table}

\section{Old extra material}

\begin{table}[b!]\caption{
Summary of the simulations discussed in this paper.
In all cases we use $w_\alpha=0.02$
?In all cases, $\dot{M}=1$ is chosen.
}\vspace{12pt}\centerline{\begin{tabular}{rcccccccc}
$r_{\rm in}$ & $R$ & $C_\alpha$ & $Q_\alpha$ & $\tilde\nu_{\rm t}$ & $\tilde{\Omega}$ & $n$ & $P_{\rm cyc}$ & $\meanB_{\rm sat}$\\
\hline
0.2 & 0.4 & 2.83 & $10^{-4}$ & 0.01 & 6 & 0 \\%M128f3
0.2 & 0.4 & 2.00 & $10^{-2}$ & 0.01 & 6 & 0 \\%M128c3k3_movie
0.1 & 0.2 & 3.00 & $10^{-2}$ & 0.01 & 6 & 0 \\%M128d1
0.1 & 0.2 & 4.00 & $10^{-2}$ & 0.01 & 6 & 0 \\%M128d2
%0.1 & 0.2 & 4.00 & $10^{-2}$ & 0.01 &0.2\\%M128d4
%0.1 & 0.2 & 5.00 & $10^{-2}$ & 0.01 &0.0 & 5.78 \\%M128d4
0.1 & 0.2 & 5.00 & $10^{-2}$ & 0.01 &0.2 & 6 & 5.77 & 0.0368  \\%M128h1
0.1 & 0.2 & 5.00 & $10^{-2}$ & 0.01 &0.2 & 0 & 2.39 & 0.399   \\%M128h1_n0
0.1 & 0.2 & 5.00 & $10^{-0}$ & 0.01 &0.2 & 6 &13.6  & 0.000345 \\%M128h1_Q1
0.1 & 0.2 & 5.00 & $10^{-1}$ & 0.01 &0.2 & 6 &11.2  & 0.00357  \\%M128h1_Q01
0.1 & 0.2 & 0.20 & $10^{-1}$ &$2\times10^{-4}$& 10 & 6 & ---  & 0.000309 \\%M1024c3_Q01_Om10
0.1 & 0.2 &$ 0.1 $& $10^{-1}$ &$8\times10^{-5}$& 10 & 6 & ---  &$2.4\times10^{-2}$\\%M4096a13_Q01_Om10 (***)
0.1 & 0.2 &$ 0.05$& $10^{-1}$ &$8\times10^{-5}$& 10 & 6 & ---  &$2.8\times10^{-3}$\\%M4096a17_Q01_Om10
0.1 & 0.2 &$ 0.05$& $10^{-2}$ &$8\times10^{-5}$& 10 & 6 & ---  &$8.0\times10^{-3}$\\%M4096a17_Q001_Om10 (**)
0.1 & 0.2 &$-0.05$& $10^{-2}$ &$8\times10^{-5}$& 10 & 6 & ---  &$2.4\times10^{-5}$\\%M4096a17_mQ001_Om10
0.1 & 0.2 &$-0.1$& $10^{-2}$ &$8\times10^{-5}$& 10 & 6 & ---  &$2.4\times10^{-5}$\\%M4096b17_mQ001_Om10
0.1 & 0.2 &$-0.1$& $10^{-2}$ &$8\times10^{-5}$& 10 & 6 & ---  &$2.4\times10^{-5}$\\%M4096b17_mQ001_Om10
%            alp       Q
0.1 & 0.2 &$0.05$& $10^{-2}$ &$8\times10^{-5}$&0.2 & 6 & 41.0 &$2.4\times10^{-5}$\\%M4096a2_Q001_Om02 (*,osc, om=0.1534, P=41)
0.1 & 0.2 &$0.05$& $10^{-2}$ &$8\times10^{-5}$& 1  & 6 & ---  &$2.4\times10^{-5}$\\%M4096a1_Q001_Om1 (**)
0.1 & 0.2 &$0.1 $& $10^{-2}$ &$8\times10^{-5}$& 1  & 6 & ---  &$2.4\times10^{-5}$\\%M4096b1_Q001_Om1 (*)
0.1 & 0.2 &$0.1 $& $ 0     $ &$8\times10^{-5}$& 1  & 6 & ---  &$2.4\times10^{-5}$\\%M4096c1_Q001_Om1 (*)
%0.1& 0.2 &$0.2 $& $10^{-2}$ &$8\times10^{-5}$& 1  & 6 & ---  &$2.4\times10^{-5}$\\%M4096d3_Q001_Om1 (crashed)
\label{Tab2}\end{tabular}}\end{table}

\begin{figure}[t!]\begin{center}
\includegraphics[width=\columnwidth]{ppprof}
\end{center}\caption[]{
Wind speed versus colatitude for $Q_\alpha=0$ (solid line)
$10^{-4}$ (dashed line), and $1$ (dotted line).
}\label{ppprof}\end{figure}

\begin{figure}[t!]\begin{center}
\includegraphics[width=\columnwidth]{ppprof_M128h1}
\end{center}\caption[]{
Wind speed versus colatitude for Run~M128h1.
}\label{ppprof_M128h1}\end{figure}

\begin{figure}[t!]\begin{center}
\includegraphics[width=\columnwidth]{ppprof_brbphi_0_M128h1}
\includegraphics[width=\columnwidth]{ppprof_brbphi_2_M128h1}
\end{center}\caption[]{
Magnetic field versus colatitude for Run~M128h1 at eight times
in intervals of $0.36$ starting from $t=17.08$.
}\label{ppprof_brbphi}\end{figure}

\begin{figure}[t!]\begin{center}
\includegraphics[width=\columnwidth]{ppprof_M128h1_n0}
\end{center}\caption[]{
Wind speed versus colatitude for Run~M128h1\_n0.
}\label{ppprof_M128h1_n0}\end{figure}

\begin{figure}[t!]\begin{center}
\includegraphics[width=\columnwidth]{ppprof_brbphi_0_M128h1_n0}
\includegraphics[width=\columnwidth]{ppprof_brbphi_2_M128h1_n0}
\end{center}\caption[]{
Magnetic field versus colatitude for Run~M128h1\_n0 at eight times
in intervals of $0.14$ starting from $t=41.46$.
}\label{ppprof_brbphi}\end{figure}

\begin{figure}[t!]\begin{center}
\includegraphics[width=\columnwidth]{ppprof_butter_M128h1_Q01}
\end{center}\caption[]{
Butterfly diagram for the old run.
}\label{ppprof_butter_M128h1_Q01}\end{figure}

\begin{figure}[t!]\begin{center}
\includegraphics[width=\columnwidth]{pvar_M1024c3_Q01_Om10}
\includegraphics[width=\columnwidth]{pvar_M128h1_Q01}
\end{center}\caption[]{
Contours of $\Omega(r,\theta)$ (left) and field lines with
contours of $\meanB_\phi(r,\theta)$ (right) for new (top)
and old (bottom) runs.
}\label{pvar_M1024c3_Q01_Om10}\end{figure}

\end{document}
