Iron opacity predictions under solar interior conditions

Details Iron opacity predictions under solar interior conditions Iron opacity predictions under solar interior conditions

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009mnras.400.1808w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 400, Issue 4, pp. 1808-1813.

Astronomy and Astrophysics

Astronomy

1

Atomic Processes, Radiative Transfer, Stars: Interiors

Scientific paper

Iron opacity predictions over an extended spectral range are obtained with a model using Opacity Project atomic data for conditions within the solar convective zone. These predictions are compared with the published results of a laboratory experiment using a laser-plasma backlighter. The effect of differing line-broadening treatments on monochromatic and the Rosseland mean opacity is also investigated.

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