Density diagnostics of solar emission lines from nitrogen-like ions

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4805

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DC Field	Value	Language
dc.contributor.author	Dwivedi, B. N	-
dc.contributor.author	Raju, P. K	-
dc.date.accessioned	2009-09-10T10:09:43Z	-
dc.date.available	2009-09-10T10:09:43Z	-
dc.date.issued	1988	-
dc.identifier.citation	Advances in Space Research, Vol. 8, No. 11, pp. 179 - 183	en
dc.identifier.issn	0273-1177	-
dc.identifier.uri	http://hdl.handle.net/2248/4805	-
dc.description.abstract	Steady state level population of 13 levels of nitrogen-like ions; Ne IV, Mg VI, Si VIII, and S X have been computed as a function of electron density and temperature. We have accounted for collisional and spontaneous radiative processes. Photo-excitations among the ground term levels have also been considered. Using the computed level populations line intensities have been obtained as a function of electron density and temperature. This study indicates that line intensity ratios for nitrogen-like ions can be used as a density monitor of the solar plasma. Absolute line fluxes from these ions at earth distance have been computed and compared with values obtained using various satellite and rocket measurements	en
dc.language.iso	en	en
dc.publisher	Elsevier	en
dc.relation.uri	http://dx.doi.org/10.1016/0273-1177(88)90316-X	en
dc.rights	© Elsevier	en
dc.subject	Density Diagnostics	en
dc.subject	Solar Emission Lines	en
dc.subject	Nitrogen-Like Ions	en
dc.title	Density diagnostics of solar emission lines from nitrogen-like ions	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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