Solar Fe abundance and magnetic fields: Towards a consistent reference metallicity

Astronomy and Astrophysics

Volumn 548, Issue , 2012, Pages

  Fabbian, D ^a,b   Moreno Insertis, F ^a,b   Khomenko, E ^a,b   Nordlund, A ^c,d  

^a INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^b UNIVERSIDAD DE LA LAGUNA   (Spain)

^c UNIVERSITY OF COPENHAGEN   (Denmark)

^d UNIVERSITY OF COPENHAGEN   (Denmark)

Author keywords

Line: formation; Magnetohydrodynamics (MHD); Radiative transfer; Sun: abundances; Sun: granulation; Sun: photosphere

Indexed keywords

CONVECTION SIMULATIONS; COPENHAGEN; DIFFERENTIAL APPROACH; EQUIVALENT WIDTH; INDIRECT EFFECTS; LINE: FORMATION; LOCAL THERMODYNAMIC EQUILIBRIUM; MAGNETOCONVECTION; METALLICITIES; OPTICAL DEPTH; OSCILLATOR STRENGTHS; SOLAR ABUNDANCES; SOLAR CONVECTION; SPECTRAL INTENSITY; SPECTRAL LINE; SPECTRAL SYNTHESIS; STAGGER CODES; SUN: ABUNDANCES; SUN: GRANULATION; SUN: PHOTOSPHERE; TEMPERATURE-SENSITIVE;

MAGNETIC FIELDS; MAGNETIC FLUX; RADIATIVE TRANSFER; SPECTROSCOPY; SUN; THREE DIMENSIONAL COMPUTER GRAPHICS;

MAGNETOHYDRODYNAMICS;

EID: 84869173087     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201219335     Document Type: Article

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