Density Diagnostics of Solar Emission Lines from the Nitrogen-Like Mgvi Ion

dc.contributor.author	Raju, P. K
dc.contributor.author	Vasundhara, R
dc.date.accessioned	2008-09-12T10:35:53Z
dc.date.available	2008-09-12T10:35:53Z
dc.date.issued	1990
dc.identifier.citation	IAU Symposium, No. 142, pp. 443 - 444	en
dc.identifier.issn	0074-1809
dc.identifier.uri	http://hdl.handle.net/2248/3572
dc.description.abstract	The variation of theoretical line intensity ratios with electron density for Mg VI ion is presented. This study indicates that the line intensity ratios for Mg VI can be used to infer electron density for solar plasma.	en
dc.language.iso	en	en
dc.publisher	International Astronomical Union	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1990IAUS..142..443R	en
dc.subject	Electron density	en
dc.subject	Solar Emission Lines	en
dc.title	Density Diagnostics of Solar Emission Lines from the Nitrogen-Like Mgvi Ion	en
dc.type	Article	en