High-resolution observations of the solar photosphere, chromosphere, and transition region
- 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
DOIAbstract
NASA’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
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