On the green-to-red line intensity ratio in the solar corona

Details On the green-to-red line intensity ratio in the solar corona On the green-to-red line intensity ratio in the solar corona

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978znata..33..786m&link_type=abstract

Zeitschrift für Naturforschung, Teil a, vol. 33a, July 1978, p. 786-788. Research supported by the University Grants Commission

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Line Spectra, Solar Corona, Solar Temperature, Abundance, Autoionization, Collision Parameters, Luminous Intensity, Radiative Recombination, Solar Spectra

Scientific paper

Green-to-red line intensity ratios have been investigated by including
various processes, like radiative recombination via bound levels,
autoionization, dielectronic recombination, etc. An improvement in the
value of coronal temperature is found.

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