High-resolution observations of the solar photosphere, chromosphere, and transition region. A database of coordinated IRIS and SST observations
- Rouppe van Der Voort, L.
- de Pontieu, B.
- Carlsson, M.
- de La Cruz Rodríguez, J.
- Bose, S.
- Chintzoglou, G.
- Drews, A.
- Froment, C.
- Gošić, M.
- Graham, D.
- Hansteen, V.
- Henriques, V.
- Jafarzadeh, S.
- Joshi, J.
- Kleint, L.
- Kohutova, P.
- Leifsen, T.
- Martínez-Sykora, J.
- Nóbrega-Siverio, D.
- Ortiz, A.
- Pereira, T.
- Popovas, A.
- Quintero Noda, C.
- Sainz Dalda, A.
- Scharmer, G.
- Schmit, D.
- Scullion, E.
- Skogsrud, H.
- Szydlarski, M.
- Timmons, R.
- Vissers, G.
- Woods, M.
- Zacharias, P.
DOIAbstract
International audienceNASA’s Interface Region Imaging Spectrograph (IRIS) provides high-resolution observations of the solar atmosphere through ultraviolet spectroscopy and imaging. Since the launch of IRIS in June 2013, we have conducted systematic observation campaigns in coordination with the Swedish 1 m Solar Telescope (SST) on La Palma. The SST provides complementary high-resolution observations of the photosphere and chromosphere. The SST observations include spectropolarimetric imaging in photospheric Fe I lines and spectrally resolved imaging in the chromospheric Ca II 8542 Å, H α , and Ca II K lines. We present a database of co-aligned IRIS and SST datasets that is open for analysis to the scientific community. The database covers ...
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