Limb-brightening observations from the OSO-7 satellite. III - Comparison of EUV line intensities of Fe XII, Fe XI, Fe XV, SI X and S XII, SI IX and S XI with predictions

Details Limb-brightening observations from the OSO-7 satellite. III - Comparison of EUV line intensities of Fe XII, Fe XI, Fe XV, SI X and S XII, SI IX and S XI with predictions Limb-brightening observations from the OSO-7 satellite. III - Comparison of EUV line intensities of Fe XII, Fe XI, Fe XV, SI X and S XII, SI IX and S XI with predictions

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....67..119k&link_type=abstract

Astronomy and Astrophysics, vol. 67, no. 1, June 1978, p. 119-127.

Astronomy and Astrophysics

Astronomy

25

Iron, Oso-7, Silicon, Solar Corona, Spectroheliographs, Sulfur, Ultraviolet Astronomy, Ultraviolet Spectra, Emission Spectra, Far Ultraviolet Radiation, Line Spectra

Scientific paper

Continuing a study of heliocentric dependence of EUV emission line intensities observed by the Goddard OSO-7 spectroheliograph in 1972, the variation of lines of the ions Fe XII, Fe XI, Fe XV, Si X and S XII, Si IX and S XI is compared with the results of individual calculations for these ions, including theoretical intensities presented for Fe XII and Fe XI. Agreement is found to be good for Fe XII and reasonable for some of the lines of the other ions which in general are weaker in intensity. Several apparent anomalies are found however which may be due to unknown line components near the wavelengths observed.

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