All Figures

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0550fig1.ps}\end{figure}$ Figure 1: The daily area-weighted latitude of sunspot groups as a function of time.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0550fig2.ps}\end{figure}$ Figure 2: The daily latitudinal area-weighted extension of activity as a function of time. The vertical dashed lines denote the Schwabe minima.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0550fig3.ps}\end{figure}$ Figure 3: The DFT-based power spectrum for the difference between the ensemble average area of sunspot groups for the two hemispheres, i.e. $(A_{30}/N_{30})_{{\rm North}}-(A_{30}/N_{30})_{{\rm South}}$ .
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0550fig4.ps}\end{figure}$ Figure 4: Difference between the ensemble average area of sunspot groups for the two hemispheres, i.e. $(A_{30}/N_{30})_{{\rm North}}-(A_{30}/N_{30})_{{\rm South}}$ . Each dot denotes a value for a 30-day interval, and the solid line represents the fitted sinusoidal profile prescribed in Eq. (3), with the following parameter values: $\nu=1/48~500$ , a₀=3.283199, a₁=-6.971889 and b₁=-18.475170.
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In the text

$\begin{figure} \par\includegraphics[width=8.7cm,clip]{0550fig5.ps}\hspace*{0.5cm} \includegraphics[width=8.6cm,clip]{0550fig6.ps}\end{figure}$ Figure 5: The mean (solid line) and the standard deviation (dashed line) of the daily latitudinal extension of activity as a function of time. The dotted line represents the results of Garcia & Mouradian (1998), i.e. the secularly smoothed sunspot number of minima $R_{\rm m}^{\ast }$ .
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0550fig1.ps}\end{figure}$	Figure 1: The daily area-weighted latitude of sunspot groups as a function of time.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0550fig2.ps}\end{figure}$	Figure 2: The daily latitudinal area-weighted extension of activity as a function of time. The vertical dashed lines denote the Schwabe minima.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0550fig3.ps}\end{figure}$	Figure 3: The DFT-based power spectrum for the difference between the ensemble average area of sunspot groups for the two hemispheres, i.e. $(A_{30}/N_{30})_{{\rm North}}-(A_{30}/N_{30})_{{\rm South}}$ .
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$\begin{figure} \par\includegraphics[width=8.7cm,clip]{0550fig5.ps}\hspace*{0.5cm} \includegraphics[width=8.6cm,clip]{0550fig6.ps}\end{figure}$	Figure 5: The mean (solid line) and the standard deviation (dashed line) of the daily latitudinal extension of activity as a function of time. The dotted line represents the results of Garcia & Mouradian (1998), i.e. the secularly smoothed sunspot number of minima $R_{\rm m}^{\ast }$ .
Open with DEXTER