| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10705196 | Planetary and Space Science | 2012 | 17 Pages |
Abstract
⺠Cassini/CIRS far-infrared observations are used to study the distribution of NH3 on Saturn. ⺠Measurements from February 2005 to December 2010. ⺠Comparison using MIRMAP and COMPSIT observations. ⺠Generally little latitudinal dependence in UTLS, but broad maxima at ±25° latitudes. ⺠These maxima are attributed to condensation and/or photolytic processes.
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Authors
J. Hurley, L.N. Fletcher, P.G.J. Irwin, S.B. Calcutt, J.A. Sinclair, C. Merlet,