The thermal structure of sunspots

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5189

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DC Field	Value	Language
dc.contributor.author	Hiremath, K. M	-
dc.contributor.author	Akshatha, B. B	-
dc.date.accessioned	2010-07-15T10:28:38Z	-
dc.date.available	2010-07-15T10:28:38Z	-
dc.date.issued	2010	-
dc.identifier.citation	Hasan, 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. 421 – 423	en
dc.identifier.isbn	978-3-642-02858-8	-
dc.identifier.uri	http://hdl.handle.net/2248/5189	-
dc.description	Restricted Access	-
dc.description	The original publication is available at springerlink.com	-
dc.description.abstract	We use SOHO/MDI continuum images to measure the average thermal structure of bipolar spots during their initial appearance. Although the average thermal structure of penumbrae is independent of sunspot size and life span, the thermal structure of umbrae depends on the life span. This suggests that penumbrae are a shallower phenomenon and that umbrae with different life spans have different anchoring depths in the convection zone.	en
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.ispartofseries	Astrophysics and Space Science Proceedings;	-
dc.relation.uri	http://www.springerlink.com/content/lj8182525475h028/	en
dc.rights	© Springer	en
dc.title	The thermal structure of sunspots	en
dc.type	Article	en
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