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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5186
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dc.contributor.authorBagare, S. P-
dc.date.accessioned2010-07-14T16:38:36Z-
dc.date.available2010-07-14T16:38:36Z-
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. 398 – 401en
dc.identifier.isbn978-3-642-02858-8-
dc.identifier.urihttp://hdl.handle.net/2248/5186-
dc.descriptionRestricted Access-
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractWe have examined theWilson effect in 580 epochs of sunspots observed at the Kodaikanal Observatory. Only unipolar spots that are well isolated from opposite polarity spots or pores (49%) exhibit the classic Wilson effect. The larger the isolation, the stronger is the effect. Unipolar spots also show a decrement of the effect that seems to be related to age. However, bipolar spots (45%) do not display theWilson effect, while spots associated with a mixed-polarity magnetic configuration (6%) show an inverse effect. We are now studying dynamic responses of spot penumbrae to their ambient magnetic configuration.en
dc.language.isoenen
dc.publisherSpringeren
dc.relation.ispartofseriesAstrophysics and Space Science Proceedings;-
dc.relation.urihttp://www.springerlink.com/content/m0745475v4802842/en
dc.rights© Springeren
dc.titleRevisit of the classic Wilson effecten
dc.typeArticleen
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