Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-29T15:05:00.509Z Has data issue: false hasContentIssue false
  • English
  • Français

The sensitivity of three lines to AR

Published online by Cambridge University Press:  14 March 2005

V. Penza ,
D. Del Moro  and
B. Caccin
V. Penza
Affiliation:
INAF - Osservatorio Astronomico di Roma, Via Frascati 33, I-00040, Monte Porzio Catone, Rome, Italy email: [email protected]
D. Del Moro
Affiliation:
Dip. di Fisica, Universitá “Tor Vergata”, Via della Ricerca Scientifica 1, I-00133, Rome, Italy
B. Caccin
Affiliation:
Dip. di Fisica, Universitá “Tor Vergata”, Via della Ricerca Scientifica 1, I-00133, Rome, Italy
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 study the sensitivity to AR of three photospheric lines, comparing experimental results, from THEMIS observations, with spectral synthesis, demonstrating the inappropriateness of using these lines as indicators of quiet sun modifications, because their variations in the active regions. We try to reconstruct the cyclic lines behavior.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. 137 - 138
Copyright
© 2004 International Astronomical Union