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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5876
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dc.contributor.authorJavaraiah, J-
dc.contributor.authorRozelot, J. P-
dc.contributor.authorBertello, L-
dc.date.accessioned2012-09-03T13:31:39Z-
dc.date.available2012-09-03T13:31:39Z-
dc.date.issued2012-06-
dc.identifier.citationAdvances in Astronomy, Vol. 2012, Article ID 470631, pp. 1-2en
dc.identifier.issn1687-7969-
dc.identifier.urihttp://hdl.handle.net/2248/5876-
dc.descriptionOpen Accessen
dc.description.abstractThe 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.isoenen
dc.publisherHindawi Publishing Corporationen
dc.relation.urihttp://dx.doi.org/10.1155/2012/470631en
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 citeden
dc.subjectSolar Physicsen
dc.subjectSunspot-
dc.subjectHelioseismology-
dc.titleThe solar cycleen
dc.typeArticleen
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