Magnetic evolution of superactive regions - Complexity and potentially unstable magnetic discontinuities

S. Criscuoli; P. Romano; F. Giorgi; F. Zuccarello

doi:10.1051/0004-6361/200912044

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Volume 506 / No 3 (November II 2009)

A&A, 506 3 (2009) 1429-1436

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Issue		A&A Volume 506, Number 3, November II 2009


Page(s)		1429 - 1436
Section		The Sun
DOI		https://doi.org/10.1051/0004-6361/200912044
Published online		27 August 2009

Online Material

Appendix A: Parameter evolution

In Figs. A.1-A.14 we report the evolution of the flare activity, total magnetic flux $\Phi _{\rm tot}$ , generalized fractal dimension D₈, contribution diversity $C_{\rm d}$ , dimensional diversity $D_{\rm d}$ and volume occupied by the potentially unstable regions I_v for each of the 14 superactive regions.

$\begin{figure} \par\includegraphics[height=14cm]{12044f29.ps} \end{figure}$	Figure A.1: Flare activity, $\Phi _{\rm tot}$ , D₈, $C_{\rm d}$ , $D_{\rm d}$ and I_v vs. time for NOAA 9026.
Open with DEXTER

$\begin{figure} \par\includegraphics[height=14cm]{12044f28.ps} \end{figure}$	Figure A.2: Flare activity, $\Phi _{\rm tot}$ , D₈, $C_{\rm d}$ , $D_{\rm d}$ and I_v vs. time for NOAA 9236.
Open with DEXTER

$\begin{figure} \par\includegraphics[height=14cm]{12044f31.ps} \end{figure}$	Figure A.3: Flare activity, $\Phi _{\rm tot}$ , D₈, $C_{\rm d}$ , $D_{\rm d}$ and I_v vs. time for NOAA 9690.
Open with DEXTER

$\begin{figure} \par\includegraphics[height=14cm]{12044f32.ps} \end{figure}$	Figure A.4: Flare activity, $\Phi _{\rm tot}$ , D₈, $C_{\rm d}$ , $D_{\rm d}$ and I_v vs. time for NOAA 9733.
Open with DEXTER

$\begin{figure} \par\includegraphics[height=14cm]{12044f33.ps} \end{figure}$	Figure A.5: Flare activity, $\Phi _{\rm tot}$ , D₈, $C_{\rm d}$ , $D_{\rm d}$ and I_v vs. time for NOAA 10030.
Open with DEXTER

$\begin{figure} \par\includegraphics[height=14cm]{12044f34.ps} \end{figure}$	Figure A.6: Flare activity, $\Phi _{\rm tot}$ , D₈, $C_{\rm d}$ , $D_{\rm d}$ and I_v vs. time for NOAA 10039.
Open with DEXTER

$\begin{figure} \par\includegraphics[height=14cm]{12044f35.ps} \end{figure}$	Figure A.7: Flare activity, $\Phi _{\rm tot}$ , D₈, $C_{\rm d}$ , $D_{\rm d}$ and I_v vs. time for NOAA 10314.
Open with DEXTER

$\begin{figure} \par\includegraphics[height=14cm]{12044f36.ps} \end{figure}$	Figure A.8: Flare activity, $\Phi _{\rm tot}$ , D₈, $C_{\rm d}$ , $D_{\rm d}$ and I_v vs. time for NOAA 10365.
Open with DEXTER

$\begin{figure} \par\includegraphics[height=14cm]{12044f37.ps} \end{figure}$	Figure A.9: Flare activity, $\Phi _{\rm tot}$ , D₈, $C_{\rm d}$ , $D_{\rm d}$ and I_v vs. time for NOAA 10375.
Open with DEXTER

$\begin{figure} \par\includegraphics[height=14cm]{12044f38.ps} \end{figure}$	Figure A.10: Flare activity, $\Phi _{\rm tot}$ , D₈, $C_{\rm d}$ , $D_{\rm d}$ and I_v vs. time for NOAA 10486.
Open with DEXTER

$\begin{figure} \par\includegraphics[height=14cm]{12044f39.ps} \end{figure}$	Figure A.11: Flare activity, $\Phi _{\rm tot}$ , D₈, $C_{\rm d}$ , $D_{\rm d}$ and I_v vs. time for NOAA 10656.
Open with DEXTER

$\begin{figure} \par\includegraphics[height=14cm]{12044f40.ps} \end{figure}$	Figure A.12: Flare activity, $\Phi _{\rm tot}$ , D₈, $C_{\rm d}$ , $D_{\rm d}$ and I_v vs. time for NOAA 10696.
Open with DEXTER

$\begin{figure} \par\includegraphics[height=14cm]{12044f41.ps} \end{figure}$	Figure A.13: Flare activity, $\Phi _{\rm tot}$ , D₈, $C_{\rm d}$ , $D_{\rm d}$ and I_v vs. time for NOAA 10720.
Open with DEXTER

$\begin{figure} \par\includegraphics[height=14cm]{12044f42.ps} \end{figure}$	Figure A.14: Flare activity, $\Phi _{\rm tot}$ , D₈, $C_{\rm d}$ , $D_{\rm d}$ and I_v vs. time for NOAA 10786.
Open with DEXTER

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