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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5190
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dc.contributor.authorSivaraman, K. R-
dc.contributor.authorSivaraman, H-
dc.contributor.authorGupta, S. S-
dc.contributor.authorHoward, R. F-
dc.date.accessioned2010-07-15T12:22:21Z-
dc.date.available2010-07-15T12:22:21Z-
dc.date.issued2010-
dc.identifier.citationHasan, S. S and Rutten, R. T., eds., Magnetic coupling between the interior and atmosphere of the Sun, Proceedings of the conference "Centenary commemoration of the discovery of the Evershed effect" Dec, 2 - 5, 2008, Indian Institute of Astrophysics, Bangalore, India, pp. 357 – 360en
dc.identifier.isbn978-3-642-02858-8-
dc.identifier.urihttp://hdl.handle.net/2248/5190-
dc.descriptionRestricted Access-
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractWe report velocities of meridional motions derived from the latitude drifts of spot groups measured on photographic images of the Sun in the Kodaikanal observatory archives. They serve to measure different meridional flows for spot groups anchored at different depths. Comparison of spot-group rotation rates with the rotation profile resulting from helioseismic inversions yields estimates of the anchoring depths. The measured latitudinal drifts correspond to meridional flows at these depths. They show evidence of return meridional flows as required in a flux-transport dynamo.en
dc.language.isoenen
dc.publisherSpringeren
dc.relation.ispartofseriesAstrophysics and Space Science Proceedings;-
dc.relation.urihttp://www.springerlink.com/content/q558150145006144/en
dc.rights© Springeren
dc.titleEvidence for return meridional flows in the convection zoneen
dc.typeArticleen
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