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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5184
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dc.contributor.authorSubramanian, K. R-
dc.contributor.authorEbenezer, E-
dc.contributor.authorRaveesha, K. H-
dc.date.accessioned2010-07-14T16:30:30Z-
dc.date.available2010-07-14T16:30:30Z-
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. 482 – 484en
dc.identifier.isbn978-3-642-02858-8-
dc.identifier.urihttp://hdl.handle.net/2248/5184-
dc.descriptionRestricted Access-
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractCoronal magnetic fields at two different heights were estimated using multiple type-II radio bursts observed on 23 January 2003. The strength of the magnetic field was estimated using 1–5 times the Newkirk density value. With these densities the magnetic field varied from 1.47 to 2.16 Gauss for the first type-II burst, and from 1.13 to 1.76 Gauss for the second one. Its strength was found to have power-law variation with height, with the index varying from −3 to −2 for densities 1–5 times Newkirk’s value.en
dc.language.isoenen
dc.publisherSpringeren
dc.relation.ispartofseriesAstrophysics and Space Science Proceedings;-
dc.relation.urihttp://www.springerlink.com/content/p8271480232848j0/en
dc.rights© Springeren
dc.titleCoronal magnetic field estimation using type-II radio burstsen
dc.typeArticleen
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