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Cooling Mechanisms of the Planetary Thermospheres: The Key Role of O Atom Vibrational Excitation of CO2 and NO

✍ Scribed by Ramesh D. Sharma; Raymond G. Roble

Publisher
John Wiley and Sons
Year
2002
Tongue
English
Weight
60 KB
Volume
3
Category
Article
ISSN
1439-4235

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πŸ“œ SIMILAR VOLUMES

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The infrared emission observed from Hz0 or Co, when added to discharged oxygen containing Oz(r Zg> and C&(lA ) is shown to arise from their vibrational excitation in the quenching of Oz(\* $'). There was no ev&nce that O$'X> is quenched to the ground state rather than to the ' 4 state.

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The populations of the nascent CO formed in the reactions oi COS with 0(3P~) and O(" Dz) atoms: O? P) + cos s co? + so, O(' D) c COS 4 COi + SO have been determined by a CO laser resonant absorption method. The fraction of the total available energy channelled into CO as vibration ~1s calculated to

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## Abstract Quasiclassical trajectories have been run to study the fundamental one‐quantum vibrational transition formed from collisions of ground‐state nitric oxide with atomic oxygen at temperatures of 500, 750, and 1000 K. Two adiabatic potential energy surfaces of different symmetry (^2^__A__β€²