![\begin{figure}
\par\includegraphics[width=7.7cm,clip]{Gb091_f1a.eps}\par\vspace*...
...\par\vspace*{3mm}
\includegraphics[width=7.7cm,clip]{Gb091_f1c.eps}
\end{figure}](/articles/aa/full/2004/23/aagb091/img57.gif) |
Figure 1: The solar wind flow around the Earth in the z=0-plane at t=30 s ( upper plot), t=60 s ( middle plot) and t=600 s ( lower plot). |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[width=8.2cm,clip]{Gb091_f2.ps}
\end{figure}](/articles/aa/full/2004/23/aagb091/img58.gif) |
Figure 2: The draping of the magnetic field lines of the solar wind around the Earth at t=600 s. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[width=7.2cm,clip]{Gb091_f3.eps}
\end{figure}](/articles/aa/full/2004/23/aagb091/img61.gif) |
Figure 3: The strength of the induced magnetic field in the Earth's ionosphere at t=500 s. |
| Open with DEXTER | |
In the text