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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3525
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dc.contributor.authorHoward, R. F-
dc.contributor.authorSivaraman, K. R-
dc.contributor.authorGupta, S. S-
dc.contributor.authorGilman, P. I-
dc.date.accessioned2008-09-10T12:16:17Z-
dc.date.available2008-09-10T12:16:17Z-
dc.date.issued1990-
dc.identifier.citationIAU Symposium, No. 142, pp. 107 - 111en
dc.identifier.issn0074-1809-
dc.identifier.urihttp://hdl.handle.net/2248/3525-
dc.description.abstractResults are presented of a study of the daily motions of individual sunspots and of sunspot groups on the basis of Kodaikanal and Mount Wilson white-light observations. A comparison of the two data sets show a good agreement between them in spot areas and motions. Preliminary rotation and latitude drift reduction from the combined data set confirm earlier results from the Mount Wilson data alone.en
dc.language.isoenen
dc.publisherInternational Astronomical Unionen
dc.relation.urihttp://adsabs.harvard.edu/abs/1990IAUS..142..107Hen
dc.subjectAstronomical photographyen
dc.subjectSolar activity, Sunspotsen
dc.subjectSolar cyclesen
dc.subjectSolar rotationen
dc.titleSunspot motions from a study of Kodaikanal and Mount Wilson observationsen
dc.typeArticleen
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