On the EUV Line Diagnostics From N III Solar Ion

dc.contributor.author	Gupta, A. K
dc.contributor.author	Mohan, A
dc.contributor.author	Dwivedi, B. N
dc.date.accessioned	2008-04-21T11:18:52Z
dc.date.available	2008-04-21T11:18:52Z
dc.date.issued	1997
dc.identifier.citation	BASI, Vol. 25, No. 2, pp. 247 - 251	en
dc.identifier.uri	http://hdl.handle.net/2248/2240
dc.description.abstract	We present new calculations for N III ion for diagnostics of solar plasma. The atomic model comprising the first 15 energy levels is considered for evaluating the line emissivities as a function of electron density and temperature, taking account of various physical processes. EUV line ratios, hitherto unexplored for diagnostic study, from this ion are presented as a function of electron density at its temperature of peak ionic concentration and their diagnostic applications in the solar atmosphere are discussed.	en
dc.format.extent	342759 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1997BASI...25..247G	en
dc.subject	Line diagnostics	en
dc.subject	EUV Emission Lines	en
dc.subject	Optically Thin Plasmas	en
dc.subject	Extreme Ultraviolet Radiation	en
dc.title	On the EUV Line Diagnostics From N III Solar Ion	en
dc.type	Article	en