Free Access

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.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.