Computer Science
Scientific paper
Oct 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icar...56..184s&link_type=abstract
Icarus (ISSN 0019-1035), vol. 56, Oct. 1983, p. 184-189. Research supported by the Nederlandse Organisatie voor Zuiver-Wetenscha
Computer Science
17
Cometary Atmospheres, Deuterium Compounds, Hydroxyl Radicals, Photodissociation, Radiation Absorption, Solar Radiation, Electron Transitions, Hydrogen Atoms, Reaction Kinetics, Comets, Radicals, Photodissociation, Absorption, Solar Radiation, Data, Calculations, Velocity, Atmosphere, Analysis
Scientific paper
The rates of photodissociation of the OH and OD molecules from absorption of solar radiation in the X2Π-A2Σ+ electronic transition are calculated to lie between 3.5 and 6.7×10-6 sec-1 for OH for heliocentric velocities between -60 and +60 km sec-1 and to be about 4.7×10-7 sec-1 for OD at 1 AU from the Sun. The corresponding lifetimes, which are upper bounds to the actual lifetimes, are generally consistent with the observational cometary data.
Dalgarno Alexander
Singh Patan D.
van Dishoeck Ewine F.
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