OH prompt emission in Comet IRAS-Araki-Alcock (1983 VII)

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Cometary Atmospheres, Hydroxyl Emission, Iras-Araki-Alcock Comet, Photodissociation, Water Vapor, Comet Nuclei, Resonance Fluorescence, Solar Radiation, Ultraviolet Spectra, Comets, Iras-Araki-Alcock, 1983Vii, Oh Radical, Emissions, Resonance, Spectra, Photodissociation, Fluorescence, Water, Density, Distribution, Ultraviolet, Wavelengths, Spectra, Satellite Observations, Comparisons, Iue Satellite, Tuttle, 1980Xiii, Production Rate, Comet Nuclei, Calculations, Data Reduction

Scientific paper

Following Bertaux's (1986) suggestion that photodissociative OH fluorescence can furnish a direct measure of water-density distribution within about 100 km of the cometary nucleus, if sufficiently high spatial resolution is available, attention is presently given to IUE-obtained UV spectra of two comets which differ only as to effective spatial resolution, in order to search for OH prompt emission. IRAS-Araki-Alcock (1983 VII) and Tuttle (1980 XIII) spectra are compared at comparable heliocentric, but differing geocentric, distances; evidence is thereby obtained for OH prompt emission in Comet IRAS-Araki-Alcock, whose implied water-production rate reflects an instantaneous value which may be compared with that derived from OH solar resonance fluorescence.

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