about
HelioseismologyMagnetic tornadoes as energy channels into the solar corona.A probable stellar solution to the cosmological lithium discrepancy.Structure of the solar photosphere studied from the radiation hydrodynamics code ANTARES.Detection of convective downflows in a sunspot penumbra.The quiet-Sun photosphere and chromosphere.Magneto-convection.Atmospheric dynamics and the mass loss process in red supergiant starsThe radii and limb darkenings ofαCentauri A and BLarge-Eddy Simulations of Magnetohydrodynamic Turbulence in Heliophysics and Astrophysics3D and Some Other Things Missing from the Theory of Massive Star EvolutionRecent Advances on Solar Global Magnetism and VariabilityUnderstanding the Internal Chemical Composition and Physical Processes of the Solar InteriorTurbulence in the Solar Atmosphere and Solar WindDevelopment of structure in pores and sunspots: flows around axisymmetric magnetic flux tubes
P2860
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P2860
description
1998 nî lūn-bûn
@nan
1998 թուականի Յունիսին հրատարակուած գիտական յօդուած
@hyw
1998 թվականի հունիսին հրատարակված գիտական հոդված
@hy
1998年の論文
@ja
1998年論文
@yue
1998年論文
@zh-hant
1998年論文
@zh-hk
1998年論文
@zh-mo
1998年論文
@zh-tw
1998年论文
@wuu
name
Simulations of Solar Granulation. I. General Properties
@ast
Simulations of Solar Granulation. I. General Properties
@en
type
label
Simulations of Solar Granulation. I. General Properties
@ast
Simulations of Solar Granulation. I. General Properties
@en
prefLabel
Simulations of Solar Granulation. I. General Properties
@ast
Simulations of Solar Granulation. I. General Properties
@en
P356
P1476
Simulations of Solar Granulation. I. General Properties
@en
P2093
A. Nordlund
R. F. Stein
P304
P356
10.1086/305678
P407
P577
1998-06-01T00:00:00Z
P5875
P819
1998ApJ...499..914S