No CrossRef data available.
Article contents
Comparative Analysis of Physical Conditions in the Solar and Procyon Atmospheres
Published online by Cambridge University Press: 08 February 2017
Abstract
An analysis is made of the velocity field determined from spectral absorption line profiles as well as inhomogeneous element sizes obtained from stochastic theory. The results of three-dimensional simulations of convective motions in the photospheres of the Sun and Procyon are presented. It is concluded that penetrative convection covers a considerable fraction of the Procyon photosphere.
- Type
- VII. Convection and Magnetic Fields in Solar-type Stars
- Information
- Copyright
- Copyright © Kluwer 1990