Oxygen lines in solar granulation

Astronomy and Astrophysics

Volumn 507, Issue 1, 2009, Pages 417-432

  Pereira, T M D ^a,b   Kiselman, D ^b   Asplund, M ^c  

^a AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^b ALBANOVA UNIVERSITY CENTER   (Sweden)

^c MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Line: formation; Sun: granulation; Sun: photosphere; Techniques: high angular resolution; Techniques: spectroscopic

Indexed keywords

3D MODELS; ATOMIC OXYGEN; BEST MATCH; HIGH ANGULAR RESOLUTIONS; HIGH SPATIAL RESOLUTION; LINE PROFILES; LINE SHIFTS; LINE: FORMATION; NEUTRAL HYDROGEN; OXYGEN LINE; QUANTITATIVE COMPARISON; SCALING FACTORS; SOLAR DISK; SOLAR PHOTOSPHERE; SOLAR TELESCOPE; SUN: GRANULATION; SUN: PHOTOSPHERE; VIEWING ANGLE;

DISKS (STRUCTURAL COMPONENTS); GRANULATION; OXYGEN; SOLAR POWER GENERATION; SUN; TELESCOPES;

THREE DIMENSIONAL;

EID: 70449630321     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912829     Document Type: Article

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