Coronal hole boundaries evolution at small scales - II. XRT view. Can small-scale outflows at CHBs be a source of the slow solar wind?

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Table 2:

Number of events over 24 h per 100 $\times$ 100 arcsec² identified inside the coronal holes (CH), in coronal hole boundary regions (CHBR) and in the quiet Sun (QS).
	No of events identified			No of unresolved events
Date	with plasma outflows			identified with no plasma outflows
	CH	CHBR	QS	CH	CHBR	QS
09/11/07	29	40	6	6	26	8
12/11/07	16	57	6	2	17	7
14/11/07	10	51	1	16	41	7
16/11/07	56	32	-	44	33	12
16/12/08	99	86	6	31	14	33
20/09/07	57	72	4	5	7	9
10/01/09	-	-	6	-	-	17
13/01/09	-	-	9	-	-	14
29/11/07	-	64	7	-	62	14

Source LaTeX | All tables | In the text

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