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Intensities and identifications of solar emission lines observed at the center of the quiet Sun are presented for the wavelength range 304-1394 A. The spectra were obtained during 1967 October by the Harvard scanning spectrometer on OSO-ly. This instrument has a spatial resolution of 1 arc minute and a spectral resolution of approximately 2 A.
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Dupree et al. (1971) studied this question.
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