Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-24T23:43:04.763Z Has data issue: false hasContentIssue false
  • English
  • Français

The Solar Cycle in the heliospheric parameters and galactic cosmic ray intensity

Published online by Cambridge University Press:  14 March 2005

M. B. Krainev  and
W. R. Webber
M. B. Krainev
Affiliation:
Lebedev Physical Institute RAS, Leninsky Prospect, 53, 119991 Moscow, Russia email: [email protected]
W. R. Webber
Affiliation:
New-Mexico State University, Las-Cruces, NM, USA 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.

We consider the Solar Cycle - the variation in any solar, heliospheric or cosmic ray parameter, related to the well-known 22-year dynamo-like process on the Sun - and discuss how it is influenced by the inner (the transformation of the solar activity in the basement of the heliosphere) and the external (the interaction between the solar and interstellar winds) factors. The corresponding approaches to the description of the long-term variations (the Solar Cycle, secular and longer ones) in the galactic cosmic ray intensity are outlined.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. 81 - 84
Copyright
© 2004 International Astronomical Union