Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-26T00:20:02.787Z Has data issue: false hasContentIssue false
  • English
  • Français

The variations of the solar magnetic field at the fast global reconfigurations periods

Published online by Cambridge University Press:  14 March 2005

S. I. Molodykh ,
G. A. Zherebtsov  and
V. A. Kovalenko
S. I. Molodykh
Affiliation:
Institute of Solar-Terrestrial Physics SB RAS, 664033, Irkutsk, P.O.Box 4026, Russia email: [email protected] Present address: Institute of Solar-Terrestrial Physics, 664033, Irkutsk, P.O.Box 4026, Russia.
G. A. Zherebtsov
Affiliation:
Institute of Solar-Terrestrial Physics SB RAS, 664033, Irkutsk, P.O.Box 4026, Russia email: [email protected]
V. A. Kovalenko
Affiliation:
Institute of Solar-Terrestrial Physics SB RAS, 664033, Irkutsk, P.O.Box 4026, Russia 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.

This paper presents the results of a comprehensive analysis of the dynamics of the sun's global magnetic structure, solar wind parameters, the interplanetary magnetic field and geomagnetic activity during fast global changes of magnetic fields on the Sun.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. 131 - 132
Copyright
© 2004 International Astronomical Union