Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3890
Title: Comparison of computed fluxes for Fe X and Fe XIV lines with observed values at 1980 eclipse
Authors: Raju, P. K
Singh, J
Keywords: Ion production rates;Iron;Line spectra;Radiant flux density;Solar eclipses;Solar heating;Computational astrophysics;Solar corona;Solar temperature;Stellar spectrophotometry
Issue Date: Sep-1987
Publisher: Kluwer Academic Publishers
Citation: Solar Physics , Vol. 110, No. 2, pp. 271 - 280
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.
URI: http://hdl.handle.net/2248/3890
ISSN: 0038-0938
???metadata.dc.relation.uri???: http://dx.doi.org/10.1007/BF00206423
Appears in Collections:IIAP Publications

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