Hostname: page-component-54dcc4c588-nx7b4 Total loading time: 0 Render date: 2025-10-05T20:07:40.323Z Has data issue: false hasContentIssue false
  • English
  • Français

Direct Simulations of Radiative and Convective Zones

Published online by Cambridge University Press:  13 January 2006

G. Alecian ,
O. Richard ,
S. Vauclair  and
F. Kupka
F. Kupka*
Affiliation:
Max-Planck-Institute for Astrophysics, Karl-Schwarzschild Str. 1, 85741 Garching, Germany
*
fk@mpa-garching.mpg.de
Get access

Abstract

Numerical simulations have become one of the main tools in the researchon stellar convection zones and they can be expected to become veryimportant for the study of the convection-diffusion interaction as well.In this review, I will first provide some historical background andthen select a few sample problems where numerical simulations of stellarconvection have provided useful results or are expected to do so inthe near future: solar granulation, interacting convection zones, andsemi-convection.

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

Article purchase

Temporarily unavailable