High-resolution observations of the solar photosphere, chromosphere, and transition region
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 FeI lines and spectrally resolved imaging in the chromospheric CaII 8542 angstrom, H alpha, and CaII 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 a variety of targets including active regions, sunspots, plages, the quiet Sun, and coronal holes.
document
https://n2t.org/ark:/85065/d7pr8090
eng
geoscientificInformation
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publication
2016-01-01T00:00:00Z
publication
2020-09-01T00:00:00Z
Copyright 2020 ESO.
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2025-07-11T19:15:51.473765