Published December 1983
| public
Journal Article
Computations and Estimates of Rate Coefficients for Hydrocarbon Reactions of Interest to the Atmospheres of the Outer Solar System
Chicago
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Abstract
The rate coefficients, including Arrhenius parameters, have been computed for a number of chemical reactions involving hydrocarbon species for which experimental data are not available and which are important in planetary atmospheric models. The techniques used to calculate the kinetic parameters include the Troe and semiempirical bond energy-bond order (BEBO) or bond strength-bond length (BSBL) methods.
Additional Information
© 1983 Academic Press, Inc. Received May 4, 1983; revised August 8, 1983. This work was supported by the NASA Planetary Atmospheres Program.Additional details
- Eprint ID
- 48369
- Resolver ID
- CaltechAUTHORS:20140812-085131127
- NASA Planetary Atmospheres Program
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2014-08-12Created from EPrint's datestamp field
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2021-11-10Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)