Calibrated fluxes are given for approximately thirty identified resonance lines of coronal ions in the wavelength region 25( 370 A obtained from the rocket spectrum 0! May 10, 1963. Estimated fluxes for thirty coronal lines and multiplets in the wavelength region 33-70 A obtained from the rocket spectrum of September 20,1963, are also given. Data are presented for the solar active centers of September 20,1963, from measurements of rocket spectroheliograms in the 300-A region.
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Austin et al. (1966) studied this question.