Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4923
Title: The large-scale magnetic field in the global solar cycle: observational aspects
Authors: Makarov, V. I
Sivaraman, K. R
Keywords: Sun;Cool Stars;Solar Activity;Magnetism;Dynamos;Large scale Magnetic Field
Issue Date: 1991
Publisher: Springer
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
Series/Report no.: Lecture Notes in Physics;Vol. 380
IAU Colloquium;No.130
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.
Description: Restricted Access
URI: http://hdl.handle.net/2248/4923
ISBN: 978-3-540-53955-1
???metadata.dc.rights???: © Springer
???metadata.dc.relation.uri???: http://www.springerlink.com/content/701813t660559u73/
Appears in Collections:IIAP Publications

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