Water production rates in Comet P/Halley from IUE observations of H I Lyman-alpha

Details Water production rates in Comet P/Halley from IUE observations of H I Lyman-alpha Water production rates in Comet P/Halley from IUE observations of H I Lyman-alpha

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993icar..105..557c&link_type=abstract

Icarus, vol. 105, p. 557

Computer Science

11

Iue, Halley'S Comet, Water Resources, Lyman Alpha Radiation, Cometary Atmospheres, Radiative Transfer, Monte Carlo Method, Optical Thickness, Computerized Simulation

Scientific paper

IUE observations of Comet Halley's H characteristics with short-wavelength spectrographs encompass nucleus-centered and serendipitously offset cases. A comparison of water production rates with a self-consistent analysis already performed for the IUE observations of OH yields good agreement. These results imply that, in order to bring the H and OH observations into agreement at all heliocentric distances, the OH model must account for coma outflow speed variations with distance.

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