Hostname: page-component-78c5997874-s2hrs Total loading time: 0 Render date: 2024-11-13T13:30:14.690Z Has data issue: false hasContentIssue false
  • English
  • Français

Panel discussion section G

Published online by Cambridge University Press:  02 March 2005

H Shibahashi
Rights & Permissions [Opens in a new window]

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

NOELS: How is convection suppressed in model computations?

CUNHA: We do this in two different ways. One is just to make the mixing parameter smaller and smaller. As it approaches zero we are, in e.ect, suppressing convection. The other way is simply to use the equation for radiative energy transport throughout the envelope. The results are very similar.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS224 , July 2004 , pp. 373 - 377
Copyright
© 2004 International Astronomical Union