The large-scale magnetic field in the global solar cycle: observational aspects

dc.contributor.author	Makarov, V. I
dc.contributor.author	Sivaraman, K. R
dc.date.accessioned	2009-12-01T17:29:45Z
dc.date.available	2009-12-01T17:29:45Z
dc.date.issued	1991
dc.identifier.citation	Tuominen, 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 - 217	en
dc.identifier.isbn	978-3-540-53955-1
dc.identifier.uri	http://hdl.handle.net/2248/4923
dc.description	Restricted Access
dc.description.abstract	The 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.iso	en	en
dc.publisher	Springer	en
dc.relation.ispartofseries	Lecture Notes in Physics;Vol. 380
dc.relation.ispartofseries	IAU Colloquium;No.130
dc.relation.uri	http://www.springerlink.com/content/701813t660559u73/	en
dc.rights	© Springer	en
dc.subject	Sun	en
dc.subject	Cool Stars	en
dc.subject	Solar Activity	en
dc.subject	Magnetism	en
dc.subject	Dynamos	en
dc.subject	Large scale Magnetic Field	en
dc.title	The large-scale magnetic field in the global solar cycle: observational aspects	en
dc.type	Article	en