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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4778
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dc.contributor.authorRangarajan, K. E-
dc.contributor.authorRao, D. M-
dc.date.accessioned2009-08-28T15:02:21Z-
dc.date.available2009-08-28T15:02:21Z-
dc.date.issued1991-
dc.identifier.citationUlmschneider, P., Priest, E. R and Rosner, R. eds., Mechanisms of chromospheric and coronal heating: Proceedings of the International Conference, Heidelberg, 5 - 8 June, 1990., pp. 63 - 65en
dc.identifier.isbn0-540-53436-9-
dc.identifier.urihttp://hdl.handle.net/2248/4778-
dc.description.abstractWe have considered the formation of Si II 1816 line in the solar chromosphere. The VAL model has been adopted as the input for the electron density and temperature. These preliminary calculations show that there are measurable changes in the profile shape of this line due to electron scattering.-
dc.language.isoenen
dc.publisherSpringer-Verlagen
dc.subjectEffects of Electron Scatteringen
dc.subjectSi II 1816 Lineen
dc.subjectSolar Chromosphereen
dc.titleThe effects of electron scattering on the Si II 1816 line in the solar chromosphereen
dc.typeArticleen
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