NASA NTRS · 19750051496
Solar X-ray spectroscopy with spatial resolution
Abstract
Preliminary results from a solar X-ray spectroscopic experiment are presented. The data emphasize the nonhomogeneous and multithermal nature of the corona. The oxygen-to-neon abundance ratio in the corona is found to be about 4.7, as derived from the O VIII-to-Ne IX resonance-line photon flux ratio.
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Acton, L. W., Catura, R. C., Joki, E. G.. 1975-01-01. Solar X-ray spectroscopy with spatial resolution. https://ntrs.nasa.gov/citations/19750051496
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