Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-27T17:42:47.970Z Has data issue: false hasContentIssue false
  • English
  • Français

Basic topology and dynamics of magnetic field leading activity the Sun

Published online by Cambridge University Press:  01 November 2006

Elena Gavryuseva
Elena Gavryuseva
Affiliation:
Istituto Nazionale di Astrofisica – Arcetri Astrophysical Observatory, Largo Enrico Fermi 5, I-50125 Florence, Italy email: [email protected]
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.

Observations of the large scale magnetic field in the photosphere taken at the Wilcox Solar Observatory since 1976 up to 2005 have been analyzed to deduce its latitudinal and longitudinal structures, its differential rotation, and their variability in time. Basic topology of solar magnetic field was reconstructed in coordinate system rotating with different rate.

Keywords

Sun: magnetic fieldsphotosphereactivity
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S233: Solar Activity and its Magnetic Origin , March 2006 , pp. 67 - 68
Copyright
© 2006 International Astronomical Union