Center-to-limb variation of solar line profiles as a test of NLTE line formation calculations

Astronomy and Astrophysics

Volumn 423, Issue 3, 2004, Pages 1109-1117

  Prieto, C Allende ^a,b   Asplund, M ^c   Bendicho, P Fabiani ^b,d  

^a The University of Texas at Austin   (United States)

^b INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^c AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^d UNIVERSIDAD DE LA LAGUNA   (Spain)

Author keywords

Line: formation; Line: profiles; Sun: photosphere

Indexed keywords

DAMPING; DATA REDUCTION; FOURIER OPTICS; LIGHT SCATTERING; OXYGEN; SPECTRUM ANALYSIS; SUN; THERMODYNAMICS;

INFRARED TRANSITIONS; LINE:FORMATION; LINE:PROFILES; SUN:PHOTOSPHERE;

ASTROPHYSICS;

EID: 4243175911     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20047050     Document Type: Article

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