Manganese and carbon lines as temperature indicators.

Details Manganese and carbon lines as temperature indicators. Manganese and carbon lines as temperature indicators.

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..107...47e&link_type=abstract

Solar Physics, Volume 107, Issue 1, pp.47-56

Physics

2

Solar Granulation:Temperatures, Solar Photosphere:Carbon, Solar Photosphere:Manganese, Solar Photosphere:Temperatures

Scientific paper

Selected hyperfine structure broadened lines of various excitations and the carbon line at 5380 Å are tested as temperature diagnostics for photospheric heterogeneities. This is done by comparing the observed center-to-limb variation of the equivalent widths of these lines with predictions by several proposed models of homogeneous type. Model 10 (Elste, 1968), which also explains the limb-darkening of the continuum in the same spectral range, provides a better basis for the analysis of heterogeneities at different photospheric levels than other recent reference models.

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