Sun-as-a-Star Spectral Line Variability in the 300–2390 nm Wavelength Range

Sun-as-a-Star Spectral Line Variability in the 300–2390 nm Wavelength Range

Combining the near-daily Ozone Monitoring Instrument (OMI) and Tropospheric Monitoring Instrument (TROPOMI) measurements of solar spectra, we construct line indices (line-core to line-flanks ratios) for various transitions (mainly Fe i ) in the 300–2390 nm spectral domain. The indices are supplement...

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Bibliographic Details
Main Authors: Sergey V. Marchenko, Antje Ludewig, Serena Criscuoli, Khaled Al Moulla, Debi P. Choudhary, Matthew T. DeLand, Greg Kopp, Erwin Loots, Emiel van der Plas, Pepijn Veefkind
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Solar activity
Solar cycle
Sunspots
Solar spectral irradiance
Solar active regions
Online Access:https://doi.org/10.3847/1538-4357/ad888f
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https://doi.org/10.3847/1538-4357/ad888f

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