Zonal velocity bands and the solar activity cycle

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3268

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DC Field	Value	Language
dc.contributor.author	Sivaraman, K. R	-
dc.contributor.author	Antia, H. M	-
dc.contributor.author	Chitre, S. M	-
dc.contributor.author	Makarova, V. V	-
dc.date.accessioned	2008-08-27T15:29:09Z	-
dc.date.available	2008-08-27T15:29:09Z	-
dc.date.issued	2008-09	-
dc.identifier.citation	Solar Physics, Vol. 251, No. 1 - 2, pp. 149 - 156	en
dc.identifier.issn	0038-0938 (Print) 1573-093X (Online)	-
dc.identifier.uri	http://hdl.handle.net/2248/3268	-
dc.description	The original publication is available at springerlink.com	en
dc.description.abstract	We compare the zonal-flow pattern in subsurface layers of the Sun with the distribution of surface magnetic features such as sunspots and polar faculae. We demonstrate that, in the activity belt, the butterfly pattern of sunspots coincides with the fast stream of zonal flows, although part of the sunspot distribution does spill over to the slow stream. At high latitudes, the polar faculae and zonal-flow bands have similar distributions in the spatial and temporal domains.	en
dc.language.iso	en	en
dc.publisher	Springer Netherlands	en
dc.relation.uri	http://arxiv.org/abs/0802.0907	en
dc.relation.uri	http://www.springerlink.com/content/w5q27660733385r1/	en
dc.rights	© Springer	en
dc.subject	Solar activity	en
dc.subject	Helioseismology	en
dc.subject	Rotation - Magnetic fields	en
dc.title	Zonal velocity bands and the solar activity cycle	en
dc.type	Article	en
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