Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mnras.178..611p&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 178, Mar. 1977, p. 611-618. Research supported by the Science Research
Astronomy and Astrophysics
Astronomy
12
Emission Spectra, Line Spectra, Solar Corona, Solar Spectra, Solar X-Rays, X Ray Spectra, Fine Structure, Iron, Monochromators, Rocket-Borne Instruments, Spaceborne Astronomy
Scientific paper
A record of the coronal X-ray emission spectrum between 13.3 and 13.8 A is presented which was obtained with a rocketborne scanning Bragg monochromator. Identification of lines due to the Fe XIX 2p-3d transition array is discussed, and four features still unidentified are noted. Blending of Fe XIX lines in the long-wavelength wing of the Ne IX 13.447-A line and with Ne VIII satellite lines is examined.
Evans K. D.
Hutcheon R. J.
Pye John P.
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