Evershed flow velocities during 100 years

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5191

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DC Field	Value	Language
dc.contributor.author	Hiremath, K. M	-
dc.date.accessioned	2010-07-15T12:25:30Z	-
dc.date.available	2010-07-15T12:25:30Z	-
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. 417 – 420	en
dc.identifier.isbn	978-3-642-02858-8	-
dc.identifier.uri	http://hdl.handle.net/2248/5191	-
dc.description	Restricted Access	-
dc.description	The original publication is available at springerlink.com	-
dc.description.abstract	An extensive literature survey indicates that the peak velocities of the Evershed flows in sunspots at the photospheric level are independent of the strength of the solar activity cycle. This result is discussed in the context of the existing models for the cause of the Evershed flow.	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/v125q80068t328u0/	en
dc.rights	© Springer	en
dc.title	Evershed flow velocities during 100 years	en
dc.type	Article	en
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