On the Origin of Solar Faculae

By C. U. Keller, M. Schüssler, A. Vögler, V. Zakharov. 2004

134 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/eb6f617d6e5d9a4415529850c086c1af03922cba

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Citations in the corpus

Semiempirical Models of the Solar Atmosphere. I. The Quiet- and Active Sun Photosphere at Moderate Resolution (2006, background): “Keller et al. (2004) note, ‘‘Despite the excellent qualitative agreement between simulations and observations, there remain quantitative disagreements. . .’’ Also, these models have not yet been shown to quantitatively account for all the moderateresolution observations that our models discuss, and…”
Solar Irradiance Variability and Climate (2013, background): “Forthermore, photons from these hot walls (which are windows into the hot interior of the Sun) can be directly observed, best when the magnetic element is located at some distance away from solar disc centre (Carlsson et al. 2004, Keller et al. 2004, Spruit 1976).”
Simulations of magneto-convection in the solar photosphere Equations, methods, and results of the MURaM code (2005, methodology): “Early other results already obtained with the MURaM code have been presented by Vögler & Schüssler (2003), Schüssler (2003), Schüssler et al. (2003), and Keller et al. (2004).”
Recent variability of the solar spectral irradiance and its impact on climate modelling (2012, background): “This radiation effi-865 ciently heats features narrower than roughly 250km, making them brighter than the mainly field-free part of the photosphere, especially when seen near the limb where the bright walls are best visible (Spruit, 1976; Keller et al., 2004).”
Solar Surface Emerging Flux Regions: A Comparative Study of Radiative MHD Modeling and Hinode SOT Observations (2008, methodology): “The code has been previously used to investigate various aspects of solar surface magnetism including solar faculae (Keller et al. 2004), magneto-convection in the quiet Sun, plage regions (Vögler 2004; Vögler et al. 2005; Shelyag et al. 2007) and mixed polarity regions (Khomenko et al. 2005),…”
Solar Surface Magnetism and Irradiance on Time Scales from Days to the 11-Year Cycle (2009, background): “D radiative magneto-hydrodynamic simulations of these small magnetic structures (Keller et al. 2004; Carlsson et al. 2004; Steiner 2005).”