The solar cycle

dc.contributor.author	Javaraiah, J
dc.contributor.author	Rozelot, J. P
dc.contributor.author	Bertello, L
dc.date.accessioned	2012-09-03T13:31:39Z
dc.date.available	2012-09-03T13:31:39Z
dc.date.issued	2012-06
dc.identifier.citation	Advances in Astronomy, Vol. 2012, Article ID 470631, pp. 1-2	en
dc.identifier.issn	1687-7969
dc.identifier.uri	http://hdl.handle.net/2248/5876
dc.description	Open Access	en
dc.description.abstract	The Sun provides variable energetic and magnetic field input to the conditions in the heliosphere which directly affect the magnetosphere. In particular, the Sun's variable magnetic fields constitute a rich source for processes that influence the Earth's upper atmosphere and geomagnetism.
dc.language.iso	en	en
dc.publisher	Hindawi Publishing Corporation	en
dc.relation.uri	http://dx.doi.org/10.1155/2012/470631	en
dc.rights	© J. Javaraiah et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited	en
dc.subject	Solar Physics	en
dc.subject	Sunspot
dc.subject	Helioseismology
dc.title	The solar cycle	en
dc.type	Article	en