Solar abundance corrections derived through three-dimensional magnetoconvection simulations

Astrophysical Journal

Volumn 724, Issue 2, 2010, Pages 1536-1541

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

^a INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^b UNIVERSITY OF COPENHAGEN   (Denmark)

^c UNIVERSIDAD DE LA LAGUNA   (Spain)

Author keywords

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

Indexed keywords

EID: 78650118389     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/724/2/1536     Document Type: Article

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