SEMIEMPIRICAL MODELS OF THE SOLAR ATMOSPHERE. III. SET OF NON-LTE MODELS FOR FAR-ULTRAVIOLET/EXTREME-ULTRAVIOLET IRRADIANCE COMPUTATION

By J. Fontenla, W. Curdt, M. Haberreiter, J. Harder, Hai-Jun Tian. 2009

164 citations recorded by the source corpus.

Subfields: Artificial Intelligence, Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/8fe7a9208281942107a7fd90704da8ac3ef80ae5

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In Artificial Intelligence

1. S. Solanki
2. N. Krivova
3. J. Haigh
4. K. L. Yeo
5. Karl-Heinz Glassmeier
6. W. Schmutz
7. Y. Unruh
8. T. Woods

In Astronomy and Astrophysics

1. N. Krivova
2. S. Solanki
3. J. Haigh
4. Karl-Heinz Glassmeier
5. K. L. Yeo
6. L. Gray
7. W. Schmutz
8. A. A. Ballegooijen

Citations in the corpus

• Recent variability of the solar spectral irradiance and its impact on climate modelling (2012, methodology): “…SSI variability.1035 Presently, a wide range of solar atmospheric models with different degrees of complexity is available (e.g. Kurucz, 1993; Fontenla et al., 1999, 2009, 2011; Unruh et al., 1999; Penza et al., 2004; Uitenbroek, 2001; Kurucz, 2005; Avrett and Loeser, 2008; Shapiro et al.,…”
• HEATING OF THE SOLAR CHROMOSPHERE AND CORONA BY ALFVÉN WAVE TURBULENCE (2011, methodology): “Fontenla et al. (2009) computed radiative loss rates as function of gas pressure (i.e., height) for several different wavelength bands (see their Figure 14).”
• Reconstruction of total and spectral solar irradiance from 1974 to 2013 based on KPVT, SoHO/MDI and SDO/HMI observations (2014, methodology): “The reconstruction of TSI and SSI by Fontenla et al. (2011) based on PSPT observations (Coulter & Kuhn 1994; Ermolli et al. 1998) and the model atmospheres of Fontenla et al. (2009) with certain adjustments does qualitatively reproduce the overall trends in early SIM visible observations.”
• HAZMAT. I. THE EVOLUTION OF FAR-UV AND NEAR-UV EMISSION FROM EARLY M STARS (2014, methodology): “…exoplanets, from Earths to Jupiters (e.g., Segura et al. 2010; Line et al. 2010; Kaltenegger et al. 2011; Hu et al. 2012; Kopparapu et al. 2012; Moses et al. 2013), require realistic input stellar fluxes, and are at the moment limited to using solar data in most cases (e.g., Fontenla et al. 2009).”
• Solar Irradiance Variability and Climate (2013, methodology): “These include the Naval Research Laboratory Solar Spectral Irradiance model (NRLSSI; Lean 2000, Lean et al. 1997), SATIRE-S (Ball 2012; Krivova, Solanki & Floyd 2006; Krivova, Solanki & Unruh 2011; Krivova et al. 2009), the COSI (COde for Solar Irradiance; Shapiro et al. 2011, 2010), SRPM (Solar Rad”