Comparison of computed fluxes for Fe X and Fe XIV lines with observed values at 1980 eclipse

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3890

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DC Field	Value	Language
dc.contributor.author	Raju, P. K	-
dc.contributor.author	Singh, J	-
dc.date.accessioned	2008-09-25T12:49:04Z	-
dc.date.available	2008-09-25T12:49:04Z	-
dc.date.issued	1987-09	-
dc.identifier.citation	Solar Physics , Vol. 110, No. 2, pp. 271 - 280	en
dc.identifier.issn	0038-0938	-
dc.identifier.uri	http://hdl.handle.net/2248/3890	-
dc.description.abstract	Fluxes have been computed for Fex (6374 Å) and Fe xiv (5303 Å) lines as a function of solar radii and at various coronal tempratures. The electron density derived from the white light corona during the total solar eclipse of 1980 were used in the computations. Fluxes in adjacent continua have also been computed. The computed ratios of line flux to the square of continuum flux at a coronal temperature of 1.6 × 106 K show a good fit with the observed values for Fex line. Further, radiative excitation seems to dominate over collisional excitation beyond 1.3 solar radius.	en
dc.language.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.uri	http://dx.doi.org/10.1007/BF00206423	en
dc.subject	Ion production rates	en
dc.subject	Iron	en
dc.subject	Line spectra	en
dc.subject	Radiant flux density	en
dc.subject	Solar eclipses	en
dc.subject	Solar heating	en
dc.subject	Computational astrophysics	en
dc.subject	Solar corona	en
dc.subject	Solar temperature	en
dc.subject	Stellar spectrophotometry	en
dc.title	Comparison of computed fluxes for Fe X and Fe XIV lines with observed values at 1980 eclipse	en
dc.type	Article	en
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