Solar chlorine abundance from an X-ray flare spectrum

Details Solar chlorine abundance from an X-ray flare spectrum Solar chlorine abundance from an X-ray flare spectrum

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.245p...4p&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 245, July 1, 1990, p. 4P-6P.

Other

3

Abundance, Chlorine, Solar Flares, Solar X-Rays, X Ray Spectra, Solar Corona, Solar Spectra, Sunspots

Scientific paper

The solar coronal chlorine abundance is estimated from a weak X-ray line
seen during a flare. The line intensity is compared with a nearby sulfur
line with very similar contribution function. The chlorine abundance
obtained is very similar to the only other positive determination for
the sun, from HCl lines in a sunspot spectrum.

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