2002
DOI: 10.1002/1439-7641(20021018)3:10<841::aid-cphc841>3.0.co;2-4
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Cooling Mechanisms of the Planetary Thermospheres: The Key Role of O Atom Vibrational Excitation of CO2 and NO
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Cited by 20 publications
(20 citation statements)
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Abstract
Smart CitationsHow this paper cites the one you are viewing
“…Calculated state-to-all rate constants for room temperature were also found to be in good agreement with the reported experimental values, − albeit a factor of nearly 3 or so smaller than the recommended values of Fernando and Smith . Such data may bear important implications on the thermospheric temperature modeling as referred to in ref .…”
Section: Discussion
supporting
confidence: 80%
Abstract
Smart CitationsHow this paper cites the one you are viewing
“…Calculated state-to-all rate constants for room temperature were also found to be in good agreement with the reported experimental values, − albeit a factor of nearly 3 or so smaller than the recommended values of Fernando and Smith . Such data may bear important implications on the thermospheric temperature modeling as referred to in ref .…”
Section: Discussion
supporting
confidence: 80%
Abstract
Smart CitationsHow this paper cites the one you are viewing
“…Recently, at least two aeronomic models have been developed or extended, taking account of the newer data on the NO( v )‐O quenching rate coefficients. Sharma and Roble [2001, 2002] found that when the value of k O ( v = 1) = 2.4 × 10 −11 cm 3 s −1 was input into the global mean model, the predicted temperature and density structure of the upper atmosphere was unrealistic using the MSIS model as a benchmark. For instance, the neutral temperature in the 100–500 km altitude range was predicted to be up to 70 K higher as compared to that predicted using the previously determined value of k O ( v = 1) = 6.5 × 10 −11 cm 3 s −1 [ Fernando and Smith , 1979], while the neutral species densities were predicted to increase by up to a factor of 2.…”
Section: Results
mentioning
confidence: 99%
Abstract
Smart CitationsHow this paper cites the one you are viewing
“…While the TIE-GCM is one of the best models in its category, it is not a perfect representation of the true upper atmosphere and there are uncertainties associated with any model simulation. For instance, there are limited constraints available on the CO 2 -O relaxation rate coefficient, which determines in part how efficiently CO 2 cools the upper atmosphere (Sharma & Roble 2002). This means that a reasonable choice has to be made, and this choice will have an influence on the effect the model predicts for an increase in the CO 2 concentration.…”
Section: Discussion
mentioning
confidence: 99%
Abstract
Smart CitationsHow this paper cites the one you are viewing
“…Calculated state-to-all rate constants for room temperature were also found to be in good agreement with the reported experimental values, − albeit a factor of nearly 3 or so smaller than the recommended values of Fernando and Smith . Such data may bear important implications on the thermospheric temperature modeling as referred to in ref .…”
Section: Discussion
supporting
confidence: 80%
Abstract
Smart CitationsHow this paper cites the one you are viewing
“…Recently, at least two aeronomic models have been developed or extended, taking account of the newer data on the NO( v )‐O quenching rate coefficients. Sharma and Roble [2001, 2002] found that when the value of k O ( v = 1) = 2.4 × 10 −11 cm 3 s −1 was input into the global mean model, the predicted temperature and density structure of the upper atmosphere was unrealistic using the MSIS model as a benchmark. For instance, the neutral temperature in the 100–500 km altitude range was predicted to be up to 70 K higher as compared to that predicted using the previously determined value of k O ( v = 1) = 6.5 × 10 −11 cm 3 s −1 [ Fernando and Smith , 1979], while the neutral species densities were predicted to increase by up to a factor of 2.…”
Section: Results
mentioning
confidence: 99%
Abstract
Smart CitationsHow this paper cites the one you are viewing
“…While the TIE-GCM is one of the best models in its category, it is not a perfect representation of the true upper atmosphere and there are uncertainties associated with any model simulation. For instance, there are limited constraints available on the CO 2 -O relaxation rate coefficient, which determines in part how efficiently CO 2 cools the upper atmosphere (Sharma & Roble 2002). This means that a reasonable choice has to be made, and this choice will have an influence on the effect the model predicts for an increase in the CO 2 concentration.…”
Section: Discussion
mentioning
confidence: 99%
Abstract
Smart CitationsHow this paper cites the one you are viewing
“…Calculated state-to-all rate constants for room temperature were also found to be in good agreement with the reported experimental values, − albeit a factor of nearly 3 or so smaller than the recommended values of Fernando and Smith . Such data may bear important implications on the thermospheric temperature modeling as referred to in ref .…”
Section: Discussion
supporting
confidence: 80%
Abstract
Smart CitationsHow this paper cites the one you are viewing
“…Recently, at least two aeronomic models have been developed or extended, taking account of the newer data on the NO( v )‐O quenching rate coefficients. Sharma and Roble [2001, 2002] found that when the value of k O ( v = 1) = 2.4 × 10 −11 cm 3 s −1 was input into the global mean model, the predicted temperature and density structure of the upper atmosphere was unrealistic using the MSIS model as a benchmark. For instance, the neutral temperature in the 100–500 km altitude range was predicted to be up to 70 K higher as compared to that predicted using the previously determined value of k O ( v = 1) = 6.5 × 10 −11 cm 3 s −1 [ Fernando and Smith , 1979], while the neutral species densities were predicted to increase by up to a factor of 2.…”
Section: Results
mentioning
confidence: 99%
Abstract
Smart CitationsHow this paper cites the one you are viewing
“…While the TIE-GCM is one of the best models in its category, it is not a perfect representation of the true upper atmosphere and there are uncertainties associated with any model simulation. For instance, there are limited constraints available on the CO 2 -O relaxation rate coefficient, which determines in part how efficiently CO 2 cools the upper atmosphere (Sharma & Roble 2002). This means that a reasonable choice has to be made, and this choice will have an influence on the effect the model predicts for an increase in the CO 2 concentration.…”
Section: Discussion
mentioning
confidence: 99%