Comparison of water production rates from UV spectroscopy and visual magnitudes for some recent comets

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Cometary Atmospheres, Iue, Ultraviolet Spectroscopy, Visible Spectrum, Water Vapor, Halley'S Comet, Meteoroid Dust Clouds, Perihelions, Tempel 2 Comet, Comets, Water, Production Rate, Comparisons, Ultraviolet, Wavelengths, Spectroscopy, Satellite Observations, Iue Satellite, Optical Properties, Lightcurve, Magnitude, Heliocentric Distance, Gases, Dust, Hydroxyl, Bradfield, 1987Xxix, Tempel 2, 1987G, Wilson, 1987Vii, Halley, 1986Iii

Scientific paper

IUE data on the UV and visible coma emissions of the comets Bradfield, P/Tempel 2, Wilson, and P/Halley, are presently compared with the visual lightcurves from magnitudes reported in the IAU circulars to consider the temporal evolution of these comets. While the water-production rates obtainable from visual magnitudes on the basis of Newburn's (1984) method are consistent with OH-derived rates to first order, they are sometimes either displaced or unable to exhibit the same pre/postperihelion asymmetry. The best agreement is obtained for the relatively dust-free Comet P/Tempel 2. IUE Fine Error Sensor lightcurves are generally in agreement with curves based on total visual magnitude.

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