Reconnection brightenings in the quiet solar photosphere

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Table 1

Overview of the CRISP datasets analyzed in this study.

Set	Date	Pointing	μ ¹	Time	Duration	Range²	Sampling	Cadence	Other
		(solar X,Y)		(UT)	[h:m:s]	[Å]	[mÅ]	[s]	instruments

1	2013 Jul. 4	−96′′, 931′′	0−0.33	09:20:32	00:21:45	± 1.400	200	3.3
2	2013 Jul. 4	914′′, −127′′	0−0.33	10:13:55	00:53:00	± 2.064	84³	8.6	AIA
3	2014 Jun. 17	24′′,939′′	0−0.30	10:20:03	00:55:49	± 1.200	100	5.5	AIA, IRIS
4	2014 Jun. 19	−11′′, 797′′	0.56	07:27:10	00:53:52	± 1.200	100	5.5
5	2014 Jun. 19	−11′′, 891′′	0−0.38	08:26:24	01:19:30	± 1.200	100	5.5	AIA
6	2014 Sep. 22	378′′, −412′′	0.81	08:37:41	02:16:35	± 1.400 ⁴⁵	200	11.7
7	2015 Sep. 15	652′′, −47′′	0.73	09:24:58	01:21:32	± 1.400 ⁴⁶	200	24.1	AIA, IRIS
8	2015 Sep. 17	728′′, 44′′	0.64	09:02:45	00:24:31	± 1.400 ⁴⁶	200	24.1	AIA, IRIS
9	2015 Oct. 11	−591, 52′′	0.79	08:44:16	01:57:16	± 1.400 ⁴⁶	200	24.1	AIA, IRIS

Notes.

⁽¹⁾

μ = cosθ with θ the observing angle.

⁽²⁾

Extent of spectral coverage of Hα.

⁽³⁾

Regular 84 mÅ sampling over ± 1.376 Å, and further out at ± 1.548, ± 1.806 and ± 2.064 Å.

⁽⁴⁾

In addition to Hα spectral scans of Ca ii 8542 Å were included, with regular 100 mÅ sampling over ± 1.2 Å.

⁽⁵⁾

A single-wavelength polarimetric sampling of Fe i 6302 Å at −48 mÅ was included to yield Stokes I, Q, U, and V maps.

⁽⁶⁾

A 12-wavelength polarimetric sampling of Fe i 6173 Å was included with regular 35 mÅ sampling over ± 0.150 Å, further out at ± 0.240 and + 0.315 Å (continuum).

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