Hostname: page-component-76fb5796d-wq484 Total loading time: 0 Render date: 2024-04-25T13:04:27.609Z Has data issue: false hasContentIssue false
  • English
  • Français

Chromospheric structure and activity in solar analogues

Published online by Cambridge University Press:  14 March 2005

M. C. Vieytes ,
P. J. D. Mauas  and
C. C. Cincunegui
M. C. Vieytes
Affiliation:
Instituto de Astronomía y Física del Espacio, CC. 67 Suc.28 (1428), Buenos Aires, Argentina. email: mariela@iafe.uba.ar
P. J. D. Mauas
Affiliation:
Instituto de Astronomía y Física del Espacio, CC. 67 Suc.28 (1428), Buenos Aires, Argentina. email: mariela@iafe.uba.ar
C. C. Cincunegui
Affiliation:
Instituto de Astronomía y Física del Espacio, CC. 67 Suc.28 (1428), Buenos Aires, Argentina. email: mariela@iafe.uba.ar
Rights & Permissions [Opens in a new window]

Abstract

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.

We computed chromospheric models of the Sun as a star and of nine solar analogues. The stars have a wide variety of magnetic activity levels, which allows us to study the differences in atmospheric structures induced by activity.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 IAUS223 , June 2004 , pp. 691 - 692
Copyright
© 2004 International Astronomical Union