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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1807
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dc.contributor.authorRoberts, B-
dc.date.accessioned2007-09-19T09:27:23Z-
dc.date.available2007-09-19T09:27:23Z-
dc.date.issued1996-
dc.identifier.citationBASI, Vol.24 No. 2 pp. 199-210en
dc.identifier.urihttp://hdl.handle.net/2248/1807-
dc.description.abstractThe influence of chromospheric magnetism on p- and f-modes is examined. The magnetism is modelled as a horizontal canopy field, embedded in an isothermal atmosphere, overlying a field-free polytropic convection zone. Both low and high frequency modes are considered. The recently detected solar cycle variability of p-modes is explored from the view-point of this model. The dual influence of convective motions and magnetism on the f-mode is discussed.en
dc.format.extent1187144 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996BASI...24..199Ren
dc.subjectMagnetic effectsen
dc.subjectp- and f-mode frequency shiftsen
dc.subjectActivity cycleen
dc.titleThe influence of chromospheric magnetism on oscillation frequenciesen
dc.typeArticleen
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