High-resolution observations of the solar photosphere, chromosphere, and transition region - A database of coordinated IRIS and SST observations

L. H. M. Rouppe van der Voort; B. De Pontieu; M. Carlsson; J. de la Cruz Rodríguez; S. Bose; G. Chintzoglou; A. Drews; C. Froment; M. Gošić; D. R. Graham; V. H. Hansteen; V. M. J. Henriques; S. Jafarzadeh; J. Joshi; L. Kleint; P. Kohutova; T. Leifsen; J. Martínez-Sykora; D. Nóbrega-Siverio; A. Ortiz; T. M. D. Pereira; A. Popovas; C. Quintero Noda; A. Sainz Dalda; G. B. Scharmer; D. Schmit; E. Scullion; H. Skogsrud; M. Szydlarski; R. Timmons; G. J. M. Vissers; M. M. Woods; P. Zacharias

doi:10.1051/0004-6361/202038732

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Volume 641 (September 2020)

A&A, 641 (2020) A146

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Table 1.

Overview of the datasets available in the database.

Date ^(a)	Time ^(b)	OBSID ^(c)	Raster ^(d)				Target ^(e)	Pointing ^(f)	μ^(g)	SST			Ref. ^(k)
			n	type	FOV [″]	Cad. [s]		(solar X, Y) [″]		Overlap ^(h)	diagnostics ⁽ⁱ⁾	Cad. ^(j) [s]
20130906	081104	4003004168	4	Sparse	3 × 50	11.5	AR, S	773, 128	0.57	00:45:30	Hα	5.5	6
20130910	080943	4003007165	2	Sparse	1 × 50	10.0	AR	−173, −189	0.96	01:12:54	Hα	5.5	1, 2
20130922	073430	4004007147	1	s&s	0.3 × 60	4.2	CH	551, 295	0.77	02:02:16	Hα, Ca 8542, Fe 6302	10.9	1, 2, 3
20140611	073631	3820256197	96	Dense	31 × 175	516	AR	573, −202	0.77	02:50:38	Hα, Ca 8542, Fe 6302	11.4	4, 8
20140614	072931	3820256197	96	Dense	31 × 175	516	AR	235, 277	0.92	00:51:32	Hα, Ca 8542, Fe 6302	11.4	6
20140615	072931	3820256197	96	Dense	31 × 175	516	AR	425, 278	0.84	01:02:36	Hα, Ca 8542, Fe 6302	11.4	6
20140621	073138	3820259497	96	Dense	31 × 175	908	QS	−201, 258	0.94	01:43:41	Hα, Ca 8542, Fe 6302	11.5	9
20140905	080604	3820255167	4	Sparse	3 × 60	13.2	AR, S	702, −304	0.59	01:53:00	Hα, Ca 8542, Fe 6302	11.6	5
20140906	080537	3820255167	4	Sparse	3 × 60	13.2	AR, S	819, −281	0.41	02:01:02	Hα, Ca 8542, Fe 6302	11.6	5
										02:00:53	Ca II H	11.6	5
20140909	075943	3860256865	4	Dense	1 × 60	21	AR	−230, −366	0.89	01:50:46	Hα, Ca 8542, Fe 6302	11.6	8
20140915	074941	3860256865	4	Dense	1 × 60	21	AR	743, 164	0.60	01:16:21	Hα, Ca 8542, Fe 6302	11.6	8
20150626	070915	3630105426	8	Dense	2.3 × 60	25	QS	−422, −260	0.85	02:31:06	Hα, Ca 8542, Fe 6173	16.1	10
20150917	073915	3630104144	32	Dense	10.2 × 60	99	QS	725, 38	0.65	00:24:46	Hα, Ca 8542, Fe 6173	24.1	7
20160429	074917	3620106129	8	Sparse	7 × 60	41	AR, S	634, 18	0.74	01:30:09	Hα, Ca 8542	20	14, 16
20160903	074446	3625503135	16	Dense	5 × 60	21	AR	−561, 44	0.81	02:14:30	Hα, Ca 8542	20	11, 15
										00:34:20	Ca II K	13	12, 13
20160904	074446	3625503135	16	Dense	5 × 60	21	AR	−374, 27	0.91	01:09:36	Hα, Ca 8542	20	15
										00:34:04	Ca II K	22	12

Notes.

^(a)

Observing date in format year, month, day.

^(b)

Starting time (UT) of observations in format hour, min, s.

^(c)

The OBSID number encodes the IRIS observing configuration in a unique number (see Tables 12–14 in De Pontieu et al. 2014a). The combination ⟨Date⟩_⟨Time⟩_⟨OBSID⟩ constitutes a unique identifier to the dataset.

^(d)

The IRIS spectrograph slit covers a region on the Sun through a raster of n slit positions, with a separation of type: dense (035), sparse (1″), or coarse (2″). Raster type s&s is the “sit-and-stare” mode for which the slit remains fixed at one location. The area covered is shown in the FOV column, and the temporal cadence in the Cad. column.

^(e)

Target: AR: active region, QS: quiet Sun, CH: coronal hole, S: sunspot.

^(f)

Pointing coordinates at the beginning of the time series, the target is followed by tracking solar rotation.

^(g)

μ = cos θ with θ the observing angle.

^(h)

Duration of overlap of SST observations with IRIS in format hh:mm:ss.

⁽ⁱ⁾

Spectral lines observed with SST. CRISP is operated independently from the instruments on the blue beam; with fixed interference filters (Ca II H) or CHROMIS (Ca II K). The instruments have their own cadences and overlap times and are separated in rows in the table.

^(j)

Cadence of the SST observations.

^(k)

References to publications based on these data sets: 1: De Pontieu et al. (2014b), 2: Rouppe van der Voort et al. (2015), 3: Martínez-Sykora et al. (2015), 4: Carlsson et al. (2015) 5: Vissers et al. (2015a), 6: Vissers et al. (2015b), 7: Rouppe van der Voort et al. (2016) 8: Skogsrud et al. (2016) 9: Rutten & Rouppe van der Voort (2017), 10: Martínez-Sykora et al. (2017), 11: Nóbrega-Siverio et al. (2017), 12: Rouppe van der Voort et al. (2017), 13: Vissers et al. (2019), 14: Bose et al. (2019b), 15: Ortiz et al. (2020) 16: Drews & Rouppe van der Voort (2020).

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