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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2798
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dc.contributor.authorKrishan, V-
dc.contributor.authorPaniveni, U-
dc.contributor.authorSingh, J-
dc.contributor.authorSrikanth, R-
dc.date.accessioned2008-07-22T10:53:54Z-
dc.date.available2008-07-22T10:53:54Z-
dc.date.issued2002-07-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 334, No. 1, pp. 230 - 232en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2248/2798-
dc.description.abstractA study of 90 supergranular cells obtained from SOHO Dopplergrams was undertaken in order to investigate a possible relation between the sizes and peak horizontal velocities of the cells. For the sample obtained, the two parameters are found to be correlated with a relation: horizontal velocity ~(size)1/3. This is in agreement with the Kolmogorov theory of turbulence as applied to large-scale solar convection.en
dc.format.extent447854 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherRoyal Astronomical Societyen
dc.relation.urihttp://www3.interscience.wiley.com/journal/118945317/abstracten
dc.relation.urihttp://adsabs.harvard.edu/abs/2002MNRAS.334..230Ken
dc.subjectTurbulenceen
dc.subjectSun: Granulationen
dc.titleRelationship between horizontal flow velocity and cell size for supergranulation using SOHO Dopplergramsen
dc.typeArticleen
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