Discriminant analysis of solar bright points and faculae - I. Classification method and center-to-limb distribution

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Table 1:

Dataset specifications.
Date	NOAA	$\left \langle \mu \right \rangle$	$(\mu_{\rm min}, \mu_{\rm max})$	FOV $_{\rm eff}$ [arcsec²]	Number of pairs
07-Sept-2004	0669	$0.97 \pm 0.003$	(0.963, 0.977)	2034	1
07-Sept-2004	0671	$0.78 \pm 0.008$	(0.75, 0.8)	2135	1
08-Sept-2004	0670	$0.97 \pm 0.003$	(0.963, 0.976)	1906	1
08-Sept-2004	0667	$0.937 \pm 0.003$	(0.928, 0.945)	1027	2
08-Sept-2004	-	$0.9 \pm 0.005$	(0.882, 0.916)	2400	1
08-Sept-2004	0671	$0.63 \pm 0.01$	(0.58, 0.67)	1923	3
08-Sept-2004	0671	$0.6 \pm 0.01$	(0.55, 0.64)	1763	2
08-Sept-2004	0671	$0.56 \pm 0.01$	(0.51, 0.6)	1904	1
13-Aug-2006	0671	$0.77 \pm 0.008$	(0.763, 0.776)	566	1

$(\mu_{\rm min}, \mu_{\rm max})$ indicates the $\mu$ coverage of the images, after their rotation along the disk radius vector pointing towards the closest limb. FOV $_{\rm eff}$ is the effective field of view once the spots and pores have been masked out. The number of image pairs selected for processing and analysis are given in the last column.

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