The Iron Line Formation Problem in Three-dimensional Hydrodynamic Models of Solar-like Photospheres

By N. Shchukina, J. Trujillo Bueno. 2001

146 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/c351d8a6f853a7c05c68f96778e757959556852c

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. W. Schmutz
4. Y. Unruh
5. Eugene V. Rozanov
6. U. Langematz
7. S. A. K. A. O. O. Odessa
8. C. Soubiran

Citations in the corpus

• Recent variability of the solar spectral irradiance and its impact on climate modelling (2012, background): “This, however, does not imply that only NLTE codes are capable of reproducing the visible solar spectrum as the NLTE effects can be imitated by a slight readjustment of the atmosphere structure (see, e.g. Rutten and Kostik, 1982; Shchukina and Trujillo Bueno, 2001).”
• On the correlation of elemental abundances with kinematics among galactic disk stars (2004, methodology): “…the Sun the abundance deviations due to NLTE effects are generally small and do not exceed 0.1 dex, as established in former calculations: 0.07 dex according to Shchukina & Bueno (2001), 0.10 dex according to Gehren et al (2001a, 2001b) for FeI lines, and -0.01 dex for SiI lines (Wedemeyer 2001).”