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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4923
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dc.contributor.authorMakarov, V. I-
dc.contributor.authorSivaraman, K. R-
dc.date.accessioned2009-12-01T17:29:45Z-
dc.date.available2009-12-01T17:29:45Z-
dc.date.issued1991-
dc.identifier.citationTuominen, I., Moss, D and Rudiger, G eds., Proceedings of Colloquium No.130 of the International Astronomical Union held in Helsinki, Finland, 17 - 20 July 1990, pp 213 - 217en
dc.identifier.isbn978-3-540-53955-1-
dc.identifier.urihttp://hdl.handle.net/2248/4923-
dc.descriptionRestricted Access-
dc.description.abstractThe global solar cycle is considered as an interaction of 3 types of activity: at low-latitude (sunspots), at high-latitude (polar faculae) and the weak magnetic field. The properties of single and 3-fold reversals of the polar magnetic field are considered. The variation spectrum of the large-scale magnetic field of the Sun is analyzed in the range of 1-30 nHz. A dependence between the rate of a poleward meridional flow and phase of the global cycle is discussed.en
dc.language.isoenen
dc.publisherSpringeren
dc.relation.ispartofseriesLecture Notes in Physics;Vol. 380-
dc.relation.ispartofseriesIAU Colloquium;No.130-
dc.relation.urihttp://www.springerlink.com/content/701813t660559u73/en
dc.rights© Springeren
dc.subjectSunen
dc.subjectCool Starsen
dc.subjectSolar Activityen
dc.subjectMagnetismen
dc.subjectDynamosen
dc.subjectLarge scale Magnetic Fielden
dc.titleThe large-scale magnetic field in the global solar cycle: observational aspectsen
dc.typeArticleen
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