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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/669
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dc.contributor.authorDwivedi, B. N-
dc.contributor.authorRaju, P. K-
dc.date.accessioned2005-12-08T05:46:20Z-
dc.date.available2005-12-08T05:46:20Z-
dc.date.issued1985-12-
dc.identifier.citationBASI, Vol. 13, No. 4, pp. 387-393en
dc.identifier.urihttp://hdl.handle.net/2248/669-
dc.description.abstractUsing Kopp & Orrall (1976) model for the electron density and temperature for the quiet sun and the coronal hole regions, we have computed emission line intensities from Mg VIII, Si X (boron-like); Mg VII, Si IX (Carbon-like) and Si VII, S IX (oxygen-like) ions and compared them with available observational data.en
dc.format.extent449555 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectEUV emission linesen
dc.subjectChromosphere - corona transition regionen
dc.subjectCoronal holesen
dc.titleLine emission from the quiet sun and the coronal hole regionsen
dc.typeArticleen
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