Extreme Ultraviolet Line Intensities from the Sun

Details Extreme Ultraviolet Line Intensities from the Sun Extreme Ultraviolet Line Intensities from the Sun

Mar 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973rspsa.332..291w&link_type=abstract

Proceedings of the Royal Society of London. Series A, Mathematical and Physical Sciences, Volume 332, Issue 1590, pp. 291-309

Physics

2

Scientific paper

An extreme ultraviolet spectrometer experiment by University College London for observation of whole-Sun spectrum-line fluxes, and flown on Orbiting Solar Observatory-6, is described. Results for the four lines with absolute calibration, are shown for the first 6 months of flight, from August 1969 to February 1970. The mean fluxes for the 30.4, 53.7, 58.4 and 121.6 nm lines are 8.1× 109± 35% ph cm-2 s-1, 3.2× 108\ ± 40% ph cm-2 s-1, 2.5× 109\ ± 40% ph cm-2 s-1, and 3× 1011\ ± 50% ph cm-2 s-1 respectively. Relations between these fluxes and the 10.7 cm radio flux and Zurich sunspot number are presented.

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