On the solar abundance of iron

dc.contributor.author	Sinha, K
dc.contributor.author	Sanwal, B. B
dc.date.accessioned	2007-03-22T05:20:38Z
dc.date.available	2007-03-22T05:20:38Z
dc.date.issued	1992
dc.identifier.citation	BASI, Vol. 20, pp. 283-285	en
dc.identifier.uri	http://hdl.handle.net/2248/1466
dc.description.abstract	The MACKKL photospheric model and the latest oscillator strengths are used to obtain a solar abundance of iron close to the meteoritic value N(Fe) = 7.51 +/- 0.01. This helps to eliminate the discrepancy between photospheric and meteoritic abundances of iron	en
dc.format.extent	237193 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Solar atmosphere	en
dc.title	On the solar abundance of iron	en
dc.type	Article	en