The solar spectrum of O IV, including photoexcitation by Fe IX 171.07 A

Details The solar spectrum of O IV, including photoexcitation by Fe IX 171.07 A The solar spectrum of O IV, including photoexcitation by Fe IX 171.07 A

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...108..361k&link_type=abstract

Astronomy and Astrophysics, vol. 108, no. 2, Apr. 1982, p. 361-368.

Astronomy and Astrophysics

Astrophysics

2

Atomic Excitations, Fine Structure, Fluorescence, Iron, Oxygen Spectra, Solar Spectra, Atomic Energy Levels, Collision Rates, Electron Transitions, Line Spectra, Solar Radiation, Transition Probabilities

Scientific paper

The extreme and far ultraviolet doublet spectrum of O IV, emitted from the solar transition region, is calculated taking account of expected photo-excitation by Fe IX at the wavelength 171.07 A. Four multiplets are shown to be sensitive to such photoexcitation, of which two in particular are potentially observable and could provide an estimate of the local Fe IX radiation field.

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