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Turbulent eddy-time-correlation in the solar convective zone
Solar and Stellar Astrophysics (astro-ph.SR)
2010/12/31
Theoretical modeling of the driving processes of solar-like oscillations is a powerful way of understanding the properties of the convective zones of solar-type stars. In this framework, the descripti...
Differential Rotation and Magnetism in Simulations of Fully Convective Stars
Solar and Stellar Astrophysics (astro-ph.SR) Fluid Dynamics (physics.flu-dyn)
2010/12/29
Stars of sufficiently low mass are convective throughout their interiors, and so do not possess an internal boundary layer akin to the solar tachocline.
On the Modelling of Rotational Effects in the Lower Convective Region of the Sun
Hydrodynamics-Sun general-Sun interior-Sun rotation-Sun fundamental parameters
2010/6/30
The purpose of this work is to study effects of differential rotation in the lower convective region of the Sun. Similar to MHD case; the governing equations are separated in variables, allowing numer...
Convective overshooting in White Dwarf and ZZ Ceti stars
Convective overshooting White Dwarf ZZ Ceti stars
2009/6/10
Convective overshooting in White Dwarf and ZZ Ceti stars。
Chemical Diffusion in Stellar Convective Regions
Chemical Diffusion Stellar Convective Regions
2009/6/10
Chemical Diffusion in Stellar Convective Regions。
An analysis of the influence of the uniform stellar rotation on
masses and radii of convective cores of zero age stars is presented. The study also
shows the dependence of the relative mass of the c...