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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3584
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dc.contributor.authorHasan, S. S-
dc.contributor.authorUlmschneider, P-
dc.date.accessioned2008-09-12T11:17:50Z-
dc.date.available2008-09-12T11:17:50Z-
dc.date.issued2004-12-
dc.identifier.citationAstronomy and Astrophysics, Vol. 428, No. 3, pp. 1017 -en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/3584-
dc.descriptionErratum-
dc.language.isoenen
dc.publisherEDP Sciencesen
dc.relation.urihttp://dx.doi.org/10.1051/0004-6361:20040200een
dc.subjectSun: Chromosphereen
dc.subjectSun: Magnetic Fieldsen
dc.subjectSun: Oscillationsen
dc.subjectErrataen
dc.subjectAddendaen
dc.titleDynamics and heating of the magnetic network on the Sun. Efficiency of mode transformationen
dc.typeArticleen
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