The correlation of fractal structures in the photospheric and the coronal magnetic field

M. Dimitropoulou; M. Georgoulis; H. Isliker; L. Vlahos; A. Anastasiadis; D. Strintzi; X. Moussas

doi:10.1051/0004-6361/200911852

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Volume 505 / No 3 (October III 2009)

A&A, 505 3 (2009) 1245-1253

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Table 5:

HINODE subset: Pearson correlation coefficients between $D_{\rm 2d}$ and $D_{\rm 3d}$ for the potential and the NLFF cases.
Extrapolation	Used 3d	Correlation	Corresponding
Method	criterion	with $D_{\rm 2d}$	Probability
Potential	$G_{\rm av}$	0.919	99%
NLFF with preprocessing	$G_{\rm av}$	-0.5	91%
NLFF with preprocessing	C_n	0.427	85%

Source LaTeX | All tables | In the text

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