Center-to-limb variation of solar line profiles as a test of NLTE line formation calculations
Open Access
- 12 August 2004
- journal article
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 423 (3) , 1109-1117
- https://doi.org/10.1051/0004-6361:20047050
Abstract
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysicsKeywords
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This publication has 24 references indexed in Scilit:
- Line formation in solar granulationAstronomy & Astrophysics, 2004
- Inelastic H+Li and H-+Li+collisions and non-LTE Li I line formation in stellar atmospheresAstronomy & Astrophysics, 2003
- Non‐LTE Model Atmospheres for Late‐Type Stars. I. A Collection of Data for Light Neutral and Singly Ionized AtomsThe Astrophysical Journal Supplement Series, 2003
- Non‐LTE Model Atmospheres for Late‐Type Stars. II. Restricted Non‐LTE Calculations for a Solar‐like AtmosphereThe Astrophysical Journal, 2003
- A list of data for the broadening of metallic lines by neutral hydrogen collisionsAstronomy and Astrophysics Supplement Series, 2000
- A catalogue of accurate wavelengths in the optical spectrum of the SunAstronomy and Astrophysics Supplement Series, 1998
- On the Determination of the Quiet-Sun Center-to-Limb Variation in Ca II K SpectroheliogramsSolar Physics, 1998
- Width cross-sections for collisional broadening of s–p and p–s transitions by atomic hydrogenMonthly Notices of the Royal Astronomical Society, 1995
- The center-to-limb variations of four Ca i lines in the photospheric spectrum at ?6500Solar Physics, 1992
- Computed Profiles for Solar MG b- and NA D-LinesThe Astrophysical Journal, 1969