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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5199
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dc.contributor.authorBanerjee, D-
dc.date.accessioned2010-07-16T09:57:52Z-
dc.date.available2010-07-16T09:57:52Z-
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. 281 – 286en
dc.identifier.isbn978-3-642-02858-8-
dc.identifier.urihttp://hdl.handle.net/2248/5199-
dc.descriptionRestricted Access-
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractThe fast solar wind originates from polar coronal holes. Recent observations from SoHO suggest that the solar wind is flowing from funnel-shaped magnetic fields anchored in the lanes of the magnetic network at the solar surface. Using the spectroscopic diagnostic capability of SUMER on SoHO and of EIS on HINODE, we study waves in polar coronal holes, in particular their origin, nature, and acceleration. The variation of the width of spectral lines with height above the solar surface supplies information on the properties of waves as they propagate out of the Sun.en
dc.language.isoenen
dc.publisherSpringeren
dc.relation.ispartofseriesAstrophysics and Space Science Proceedings;-
dc.relation.urihttp://dx.doi.org/10.1007/978-3-642-02859-5_22en
dc.rights© Springeren
dc.titleWaves in polar coronal holesen
dc.typeArticleen
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