High‐resolution solar spectral irradiance from extreme ultraviolet to far infrared

By J. Fontenla, J. Harder, W. Livingston, M. Snow, T. Woods. 2011

184 citations recorded by the source corpus.

Subfields: Artificial Intelligence, Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/20515a66d4b5d7745741343bbdff3244bb55119c

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Citations in the corpus

THE ULTRAVIOLET RADIATION ENVIRONMENT AROUND M DWARF EXOPLANET HOST STARS (2012, background): “The UV (FUV + NUV) spectra of solar-type stars have been studied extensively, both observationally and theoretically (e.g., Woods et al. 2009; Fontenla et al. 2011; Linsky et al. 2012c).”
The Absolute Magnitude of the Sun in Several Filters (2018, methodology): “The Fontenla et al. (2011) spectrum was scaled by the bi-weight average (Beers et al. 1990) ratio between the Haberreiter et al. (2017) composite and the model for wavelengths between 1.8 µm and 2.0 µm (1.0299 ±0.0074).”
Reconstruction of total and spectral solar irradiance from 1974 to 2013 based on KPVT, SoHO/MDI and SDO/HMI observations (2014, methodology): “Coming at a time where solar activity is declining, this increase in visible flux runs counter to models of solar irradiance (apart from Fontenla et al. 2011, discussed below), which point to visible solar irradiance varying in phase with the solar cycle instead.”
THE MUSCLES TREASURY SURVEY. I. MOTIVATION AND OVERVIEW (2016, methodology): “The Lyα fluxes are combined with models of solar active regions (Fontenla et al. 2011) to estimate the EUV luminosity in the wavelength region 100 – 1170 Å, in 100 Å bins (see Linsky et al. 2014 and Paper II).”
Solar Irradiance Variability and Climate (2013, methodology): “…Solanki & Unruh 2011; Krivova et al. 2009), the COSI (COde for Solar Irradiance; Shapiro et al. 2011, 2010), SRPM (Solar Radiation Physical Modelling; Fontenla et al. 1999, 2009, 2011, 2004) and OAR (Osservatorio Astronomico di Roma; Ermolli, Criscuoli & Giorgi 2011; Ermolli et al. 2012) models.”
Recent variability of the solar spectral irradiance and its impact on climate modelling (2012, methodology): “the calculations of each of these features are presented in Fontenla et al.(2009). These models go back to the ones of Fontenla et al. (1999, and references therein), which have been revised in subsequent studies of F ntenla et al.(2004, 2006, 2009) to account for observational results and for exten”