Diagnostics of solar plasma using emission lines

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/190

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DC Field	Value	Language
dc.contributor.author	Dwivedi, B. N	-
dc.date.accessioned	2005-01-08T05:45:03Z	-
dc.date.available	2005-01-08T05:45:03Z	-
dc.date.issued	1988	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 9, pp. 99-110	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/190	-
dc.description.abstract	The spectroscopic techniques in the X- and EUV region to determine electron density and temperature of solar plasma have been presented. The line intensity ratios as a diagnostic probe of solar plasma from berrylium, boron, nitrogen and oxygen - like ions have been discussed with a detailed investigation of carbon-like ions. Absolute line fluxes from these ions at earth distance have also been discussed.	en
dc.format.extent	391098 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Solar plasma	en
dc.subject	Emission lines	en
dc.subject	Spectral formation	en
dc.title	Diagnostics of solar plasma using emission lines	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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