Weak Fe XVII transitions in the coronal X-ray spectrum

Details Weak Fe XVII transitions in the coronal X-ray spectrum Weak Fe XVII transitions in the coronal X-ray spectrum

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....51..451h&link_type=abstract

Astronomy and Astrophysics, vol. 51, no. 3, Sept. 1976, p. 451-460.

Astronomy and Astrophysics

Astrophysics

21

Electron Transitions, Iron, Solar Corona, Solar X-Rays, X Ray Spectra, Atomic Energy Levels, High Resolution, Ionization Potentials, Luminous Intensity, Spectral Resolution, Wavelengths

Scientific paper

Wavelengths and relative intensities are calculated for previously unknown higher members of all Rydberg series of Fe XVII known to be significantly radiated by coronal active regions. High-resolution coronal-active-region X-ray-spectrum measurements are analyzed to find these transitions. The measured wavelengths and intensities are given along with a revised value of the Fe XVII ionization potential. The work is compared with that of others, and a critical examination of the risk of erroneous identification in the present work is included

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