H and K /Ca II/ emissions as observed in coronal spectrum in the July 20, 1963 solar eclipse

Details H and K /Ca II/ emissions as observed in coronal spectrum in the July 20, 1963 solar eclipse H and K /Ca II/ emissions as observed in coronal spectrum in the July 20, 1963 solar eclipse

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...45..291c&link_type=abstract

Solar Physics, vol. 45, Dec. 1975, p. 291-299.

Physics

2

H Lines, K Lines, Solar Corona, Solar Spectra, Emission Spectra, Solar Eclipses, Solar Temperature

Scientific paper

From a detailed analysis of a coronal spectrum taken from a jet aircraft
during the eclipse of July 20, 1963, a rough model of a coronal cold
region (temperature of about 100,000 K) has been obtained. The model
explains the presence of the abnormal H and K (Ca II) emissions and the
large amount of F corona present in the spectrum.

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