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The CH 4 structure in Titan's upper atmosphere revisited

✍ Scribed by Cui, J.; Yelle, R. V.; Strobel, D. F.; Müller-Wodarg, I. C. F.; Snowden, D. S.; Koskinen, T. T.; Galand, M.

Book ID
119683459
Publisher
American Geophysical Union
Year
2012
Tongue
English
Weight
775 KB
Volume
117
Category
Article
ISSN
0148-0227

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✍ L.M. Lara; M. Banaszkiewicz; R. Rodrigo; J.J. Lopez-Moreno 📂 Article 📅 2002 🏛 Elsevier Science 🌐 English ⚖ 171 KB

## Previous modeling by Banaszkiewicz et al. (2000a,b) showed that the CH 4 thermospheric mixing ratio on Titan could vary as much as 35-40% due to ion-neutral chemical reactions. A new vertical methane profile has been computed by simultaneously modifying the stratospheric methane mixing ratio an