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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/946
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dc.contributor.authorZhukov, V. I-
dc.contributor.authorEfremov, V. I-
dc.date.accessioned2006-04-11T08:27:27Z-
dc.date.available2006-04-11T08:27:27Z-
dc.date.issued1988-12-
dc.identifier.citationBASI, Vol. 16, No. 4, pp. 145-158en
dc.identifier.urihttp://hdl.handle.net/2248/946-
dc.description.abstractNumerical calculations are given for the propagation of Alfven p-waves in the solar atmosphere for Geronicolas' (1977) sunspot model. It is shown that Alfven p-waves with a period greater than 400s do not, in fact, penetrate into upper layers of a sunspot. This is due to the reflection of Alfven p-waves from the upper layers and to coupling with magnetogravity waves trapped at a particular layer of a sunspot. Proper resonance periods for magnetogravity waves in a sunspot are calculateden
dc.format.extent978211 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indianen
dc.subjectOscillationsen
dc.subjectSunspotsen
dc.subjectMHD wavesen
dc.titlePropagation of magnetohydrodynamic waves in the solar atmosphere - Alfven p-waves in sunspotsen
dc.typeArticleen
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