Atomic data and spectral line intensities for O VIII and Fe XVII resonance lines as well as their O VII and Fe XVI satellite lines

Details Atomic data and spectral line intensities for O VIII and Fe XVII resonance lines as well as their O VII and Fe XVI satellite lines Atomic data and spectral line intensities for O VIII and Fe XVII resonance lines as well as their O VII and Fe XVI satellite lines

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26as..105...77c&link_type=abstract

Astronomy and Astrophysics Suppl. 105, 77-90 (1994)

Astronomy and Astrophysics

Astrophysics

27

Atomic Data, Lines: Identification, Sun: Corona, Sun: X-Rays, X-Rays: General

Scientific paper

The atomic data required to analyse low density coronal plasmas have
been calculated and used to interpret X-ray spectra observed by the Flat
Crystal Spectrometer of the SMM/NASA satellite in the 14-19 A wavelength
range. The emission lines correspond mainly to Fe XVI, Fe XVII, Fe XVIII
and some ones to O VII, O VIII.

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