Line emission from the quiet sun and the coronal hole regions

dc.contributor.author	Dwivedi, B. N
dc.contributor.author	Raju, P. K
dc.date.accessioned	2005-12-08T05:46:20Z
dc.date.available	2005-12-08T05:46:20Z
dc.date.issued	1985-12
dc.identifier.citation	BASI, Vol. 13, No. 4, pp. 387-393	en
dc.identifier.uri	http://hdl.handle.net/2248/669
dc.description.abstract	Using 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.extent	449555 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	EUV emission lines	en
dc.subject	Chromosphere - corona transition region	en
dc.subject	Coronal holes	en
dc.title	Line emission from the quiet sun and the coronal hole regions	en
dc.type	Article	en