Benchmarking atomic data for astrophysics: Fe xi

Details Benchmarking atomic data for astrophysics: Fe xi Benchmarking atomic data for astrophysics: Fe xi

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010a%26a...514a..41d&link_type=abstract

Astronomy and Astrophysics, Volume 514, id.A41

Astronomy and Astrophysics

Astrophysics

10

Atomic Data, Line: Identification, Sun: Corona, Techniques: Spectroscopic

Scientific paper

High-resolution spectroscopic observations of the solar corona and laboratory measurements are used to review all the line identifications for Fe xi, from the EUV to the visible. The results of the atomic structure and scattering calculations are presented elsewhere, while detailed comparisons between observed and predicted wavelengths and intensities are discussed here. All the brightest EUV lines in the solar corona are now finally firmly identified. Several new identifications are proposed, in particular, coronal forbidden lines. The previously-known density-diagnostics are confirmed. New and important temperature diagnostics are presented, and the presence of blends highlighted.

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