Evershed flow velocities during 100 years

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