$\begin{figure} { \epsfig{file=0454fig1.ps,width = 7.6cm} } \end{figure}$ Figure 1: SSNSA of the international sunspot number time series versus the number of days per bin for the binomial distribution (dash-dot line); Excess (dashed line); normal approximation to the binomial distribution (solid line); and Pearson's chi-square test (dotted line).
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In the text

$\begin{figure} { \epsfig{file=0454fig2.ps, width = 7.8cm} } \end{figure}$ Figure 2: SSNSA of the number of X-ray flare time series versus the number of days per bin for the binomial distribution (dash-dot line); Excess (dashed line); normal approximation to the binomial distribution (solid line); and Pearson's chi-square test (dotted line).
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In the text

$\begin{figure} { \epsfig{file=0454fig3.ps, width = 7.5cm} } \end{figure}$ Figure 3: Student's t-test: SSNSA of sunspot area (solid line), H $_{\alpha }$ flare index (dotted line), Mount Wilson total magnetic flux (dash - dot line), and Kitt Peak averaged magnetic flux density (dashed line), versus the number (n) of elements in each group.
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In the text

$\begin{figure} { \epsfig{file=0454fig4.ps, width = 7.5cm} } \end{figure}$ Figure 4: SSNSA of the daily hemispheric sunspot numbers versus solar cycle. Triangles denote the SSNSA around the maximum of solar activity. Squares denote the SSNSA around the minimum of solar activity.
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In the text

$\begin{figure} { \epsfig{file=0454fig1.ps,width = 7.6cm} } \end{figure}$	Figure 1: SSNSA of the international sunspot number time series versus the number of days per bin for the binomial distribution (dash-dot line); Excess (dashed line); normal approximation to the binomial distribution (solid line); and Pearson's chi-square test (dotted line).
Open with DEXTER

$\begin{figure} { \epsfig{file=0454fig2.ps, width = 7.8cm} } \end{figure}$	Figure 2: SSNSA of the number of X-ray flare time series versus the number of days per bin for the binomial distribution (dash-dot line); Excess (dashed line); normal approximation to the binomial distribution (solid line); and Pearson's chi-square test (dotted line).
Open with DEXTER

$\begin{figure} { \epsfig{file=0454fig3.ps, width = 7.5cm} } \end{figure}$	Figure 3: Student's t-test: SSNSA of sunspot area (solid line), H $_{\alpha }$ flare index (dotted line), Mount Wilson total magnetic flux (dash - dot line), and Kitt Peak averaged magnetic flux density (dashed line), versus the number (n) of elements in each group.
Open with DEXTER

$\begin{figure} { \epsfig{file=0454fig4.ps, width = 7.5cm} } \end{figure}$	Figure 4: SSNSA of the daily hemispheric sunspot numbers versus solar cycle. Triangles denote the SSNSA around the maximum of solar activity. Squares denote the SSNSA around the minimum of solar activity.
Open with DEXTER