The effects of electron scattering on the Si II 1816 line in the solar chromosphere

dc.contributor.author	Rangarajan, K. E
dc.contributor.author	Rao, D. M
dc.date.accessioned	2009-08-28T15:02:21Z
dc.date.available	2009-08-28T15:02:21Z
dc.date.issued	1991
dc.identifier.citation	Ulmschneider, 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 - 65	en
dc.identifier.isbn	0-540-53436-9
dc.identifier.uri	http://hdl.handle.net/2248/4778
dc.description.abstract	We 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.iso	en	en
dc.publisher	Springer-Verlag	en
dc.subject	Effects of Electron Scattering	en
dc.subject	Si II 1816 Line	en
dc.subject	Solar Chromosphere	en
dc.title	The effects of electron scattering on the Si II 1816 line in the solar chromosphere	en
dc.type	Article	en