Formation of chromospheric Fe I lines in the near-ultraviolet in 1D atmospheres
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A1 Alkuperäisartikkeli tieteellisessä aikakauslehdessä
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en
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8
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Astronomy & Astrophysics, Volume 704
Abstract
In the near-ultraviolet part of the solar spectrum lie several Fe I lines with very broad profiles that are typical of chromospheric lines. These lines are largely unexplored because high-resolution data in this region were lacking. This changed with the successful SUNRISE III flight in 2024, when spectropolarimetric data were recorded with high spatial, spectral, and temporal resolution covering a large variety of solar targets.Description
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Harnes, E, Smitha, H N, Lagg, A, Przybylski, D & Solanki, S K 2025, 'Formation of chromospheric Fe I lines in the near-ultraviolet in 1D atmospheres', Astronomy & Astrophysics, vol. 704, A60. https://doi.org/10.1051/0004-6361/202555319