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