Theoretical analysis of the Fe XVIII X-ray spectrum and application to solar coronal observations

Details Theoretical analysis of the Fe XVIII X-ray spectrum and application to solar coronal observations Theoretical analysis of the Fe XVIII X-ray spectrum and application to solar coronal observations

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...259..669c&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 259, no. 2, p. 669-681.

Astronomy and Astrophysics

Astrophysics

25

Iron, Metal Ions, Solar Corona, Solar Flares, Spectrum Analysis, X Ray Spectra, Atomic Energy Levels, Solar Activity, Solar Maximum Mission, Transition Probabilities

Scientific paper

A theoretical study of Fe XVIII X-ray spectrum is presented and a comparison of the corresponding atomic parameters with other calculations is done. Results are used to construct different theoretical spectra which are compared to a solar active-region spectrum in the 13-19 A range. From this analysis, new Fe XVIII line identifications are proposed.

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