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The effects of numerical resolution on hydrodynamical surface convection simulations and spectral line formation
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
2000 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 359, no 2, 669-681 p.Article in journal (Refereed) Published
Abstract [en]

The computationally demanding nature of radiative-hydrodynamical simulations of stellar surface convection warrants an investigation of the sensitivity of the convective structure and spectral synthesis to the numerical resolution and dimension of the sim

Place, publisher, year, edition, pages
SPRINGER-VERLAG , 2000. Vol. 359, no 2, 669-681 p.
Keyword [en]
convection; hydrodynamics; line : formation; Sun : abundances; Sun : granulation; Sun : photosphere; NEUTRAL HYDROGEN-ATOMS; FE-I LINES; MODEL ATMOSPHERES; SOLAR GRANULATION; ABUNDANCE; TRANSITIONS; STARS; IRON; COLLISIONS
URN: urn:nbn:se:uu:diva-36617OAI: oai:DiVA.org:uu-36617DiVA: diva2:64516
Addresses: Asplund M, Astron Observ, Box 515, S-75120 Uppsala, Sweden. NORDITA, DK-2100 Copenhagen O, Denmark. NBIFAFG, Astron Observ, DK-2100 Copenhagen, Denmark. Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48823 USA.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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