Solar Abundance Corrections Derived Through Three-dimensional Magnetoconvection Simulations

We explore the effect of the magnetic field when using realistic three-dimensional convection experiments to determine solar element abundances. By carrying out magnetoconvection simulations with a radiation-hydro code (the Copenhagen stagger code) and through a posteriori spectral synthesis of thre...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	The Astrophysical journal 2010-12, Vol.724 (2), p.1536-1541
Hauptverfasser:	Fabbian, D, Khomenko, E, Moreno-Insertis, F, Nordlund, Å
Format:	Artikel
Sprache:	eng
Schlagworte:	ABUNDANCE Astronomy ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ATMOSPHERES Earth, ocean, space ELEMENT ABUNDANCE ELEMENTS ENERGY TRANSFER Exact sciences and technology FLUID MECHANICS HEAT TRANSFER HYDRODYNAMICS IRON MAGNETIC FLUX MAGNETOHYDRODYNAMICS MAIN SEQUENCE STARS MECHANICS METALS PHOTOSPHERE RADIANT HEAT TRANSFER SOLAR ATMOSPHERE STARS STELLAR ATMOSPHERES SUN THREE-DIMENSIONAL CALCULATIONS TRANSITION ELEMENTS ZEEMAN EFFECT
Online-Zugang:	Volltext bestellen
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!