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The effects of numerical resolution on hydrodynamical surface convection simulations and spectral line formation
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- Asplund, M (author)
- Uppsala universitet,Institutionen för astronomi och rymdfysik
- Ludwig, HG (author)
- Nordlund, A (author)
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- Stein, RF (author)
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- (creator_code:org_t)
- SPRINGER-VERLAG, 2000
- 2000
- English.
- In: ASTRONOMY AND ASTROPHYSICS. - : SPRINGER-VERLAG. - 0004-6361. ; 359:2, s. 669-681
- Journal article (peer-reviewed)
Abstract
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- 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
Keyword
- 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
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- ref (subject category)
- art (subject category)
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