The detection of the 5577.3 A forbidden line of O I in comets

Details The detection of the 5577.3 A forbidden line of O I in comets The detection of the 5577.3 A forbidden line of O I in comets

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984em%26p...30..105k&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 30, Feb. 1984, p. 105-110. Research supported by the University of California, N

Physics

4

Comets, Forbidden Bands, Oxygen Spectra, Swan Bands, Data Simulation, Encke Comet, Kohoutek Comet, Radiant Flux Density

Scientific paper

The spectral synthesis of C2 Swan band sequence Delta V = -1 indicates the intensity of the forbidden green oxygen line of 5577.3 A to be about 3 to 5 percent of the 6300 A line. Therefore, it appears that the green line should be observable in high-resolution spectra of a bright comet. Festou and Feldman suggest red/green greater than or equal to 10 means a water parent origin.

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