Spatial distributions of extreme-ultraviolet brightenings in the quiet Sun

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Volume 692 (December 2024)

A&A, 692 (2024) A236

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Table A.1.

Statistics of EUV brightenings related to the LoS magnetic field configuration for eight different detection thresholds.

B_th	HMI	Strong bipolar			Weak mixing			Unipolar			Weak field
	FOV	Events	$\bar{Area}$ $\overline{\mathrm{Area}}$	$\bar{Dur}$ $\overline{\mathrm{Dur}}$	Events	$\bar{Area}$ $\overline{\mathrm{Area}}$	$\bar{Dur}$ $\overline{\mathrm{Dur}}$	Events	$\bar{Area}$ $\overline{\mathrm{Area}}$	$\bar{Dur}$ $\overline{\mathrm{Dur}}$	Events	$\bar{Area}$ $\overline{\mathrm{Area}}$	$\bar{Dur}$ $\overline{\mathrm{Dur}}$
G	pixel²	%	Mm²	s	%	Mm²	s	%	Mm²	s	%	Mm²	s
20	5x5	12.4	0.38	27	59.3	0.31	25	9.2	0.25	27	19.1	0.32	25
30	5x5	5.1	0.43	31	46.2	0.30	25	9.2	0.25	27	39.4	0.33	25
40	5x5	3.1	0.45	29	37.8	0.30	25	9.1	0.25	27	50.0	0.33	25
50	5x5	2.1	0.48	34	32.2	0.30	25	9.0	0.25	27	56.7	0.32	25

20	9x9	47.0	0.35	28	49.7	0.27	24	0.4	0.21	32	2.9	0.36	27
30	9x9	22.5	0.40	31	61.5	0.28	24	0.4	0.21	32	15.5	0.31	25
40	9x9	15.1	0.40	30	58.7	0.29	25	0.4	0.21	32	25.8	0.31	24
50	9x9	11.0	0.39	31	56.5	0.30	26	0.4	0.21	32	32.1	0.31	24

Notes. Same as Table 1, but for percentages instead of the number of events.

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