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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1826
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dc.contributor.authorSchou, J-
dc.contributor.authorTomczyk, S-
dc.contributor.authorThompson, M. J-
dc.date.accessioned2007-09-25T10:10:37Z-
dc.date.available2007-09-25T10:10:37Z-
dc.date.issued1996-
dc.identifier.citationBASI, Vol.24 No. 2 pp. 375-378en
dc.identifier.urihttp://hdl.handle.net/2248/1826-
dc.description.abstractWe present various results from one year of observations with the LOWL instrument, which is designed to observe oscillations with degrees l from 0 to about 100. Among the results shown is an inversion for the solar rotaion rate down to approximately 0.2R, Given the long duration of the observations we have been able to obtain very low errors and good radial and latitude resolution in a substantial part of the solar interior. We will also present results of analyzing different parts of the time-series to look for temporal variations in mode frequencies and show that they seem to be associated with variations in solar activity.en
dc.format.extent353978 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996BASI...24..375Sen
dc.subjectSun:rotationen
dc.subjectActivityen
dc.subjectInversionsen
dc.titleResults from the LOWL instrumenten
dc.typeArticleen
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