Semiempirical Models of the Solar Atmosphere. I. The Quiet- and Active Sun Photosphere at Moderate Resolution

By J. Fontenla, E. Avrett, G. Thuillier, J. Harder. 2006

141 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/78e12b1286ea059d60e1365e28fa941cd3014665

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. N. Krivova
2. S. Solanki
3. C. Fröhlich
4. Greg Kopp
5. Martin Asplund
6. N. Grevesse
7. Pat Scott
8. A. Sauval

In Atmospheric Science

1. S. Solanki
2. N. Krivova
3. Greg Kopp
4. J. Fontenla
5. J. Harder
6. M. Haberreiter
7. N. Grevesse
8. U. Langematz

Citations in the corpus

• The chemical composition of the Sun (2009, background): “Indeed it is somewhat surprising that the val3c model or its successors (e.g. Fontenla et al. 2006) have not caught on more within the solar abundance community, since they are built on similar premises but without the LTE restriction.”
• Solar Surface Magnetism and Irradiance on Time Scales from Days to the 11-Year Cycle (2009, methodology): “Besides, first encouraging tests of the models have been carried out in the IR (Fontenla et al. 2006; Platnick and Fontenla 2008; Unruh et al. 2008).”
• HEATING OF THE SOLAR CHROMOSPHERE AND CORONA BY ALFVÉN WAVE TURBULENCE (2011, methodology): “The structure of the lower atmosphere is based on a model of a facular region (i.e., very bright plage region) called model P, which was first developed by Fontenla et al. (1999) and more recently discussed by Fontenla et al. (2006, 2009).”
• Recent variability of the solar spectral irradiance and its impact on climate modelling (2012, result): “These models go back to the ones of Fontenla et al. (1999, and references therein), which have been revised in1215 subsequent studies of Fontenla et al. (2004, 2006, 2009) to account for observational results and for extension of the atmospheric layers.”
• Trends in solar spectral irradiance variability in the visible and infrared (2009, background): “…observed by SIM are consistent with a temperature gradient in the photosphere that, on average, is slightly shallower during the peak of solar activity than it is under quiet conditions as illustrated in Figure 4 [Fontenla et al., 2006, 2007] for quiet sun and facula in the neighborhood of Teff.”