Simulations of the solar near-surface layers with the CO5BOLD, MURaM, and Stagger codes
Context: Radiative hydrodynamic simulations of solar and stellar surface convection have become an important tool for exploring the structure and gas dynamics in the envelopes and atmospheres of late-type stars and for improving our understanding of the formation of stellar spectra. Aims: We quantitatively compare results from three-dimensional, radiative hydrodynamic simulations of convection near the solar surface generated with three numerical codes (CO 5 BOLD, MURaM, and Stagger) and...[Show more]
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics|
|01_Beeck_Simulations_of_the_solar_2012.pdf||2.04 MB||Adobe PDF||Request a copy|
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