Infrared measurements of atmospheric CH_3CN

For the first time CH_3CN has been measured in the Earth's atmosphere by means of infrared remote sensing. Vertical profiles of volume mixing ratio were retrieved from 12 solar occultation measurements by the balloon-borne JPL MkIV interferometer between 1993 and 2004. Profile retrieval is poss...

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Bibliographic Details
Published in:Geophysical Research Letters
Main Authors: Kleinböhl, Armin, Toon, Geoffrey C., Sen, Bhaswar, Blavier, Jean-François L., Weisenstein, Debra K., Wennberg, Paul O.
Format: Article in Journal/Newspaper
Language:English
Published: American Geophysical Union 2005
Subjects:
Online Access:https://authors.library.caltech.edu/46620/
https://authors.library.caltech.edu/46620/1/grl20563.pdf
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Description
Summary:For the first time CH_3CN has been measured in the Earth's atmosphere by means of infrared remote sensing. Vertical profiles of volume mixing ratio were retrieved from 12 solar occultation measurements by the balloon-borne JPL MkIV interferometer between 1993 and 2004. Profile retrieval is possible in an altitude range between 12 and 30 km with a precision of ∼20 ppt in the Arctic and ∼30 ppt at mid-latitudes. The retrieved CH_3CN profiles show mixing ratios of 100–150 ppt a few kilometers above the tropopause that decrease to values below 40 ppt at altitudes between 22 and 30 km. The CH_3CN mixing ratios show a reasonably compact correlation with the stratospheric tracers CH_3Cl and CH_4. The CH_3CN altitude profiles and tracer correlations are well reproduced by a 2-dimensional model, suggesting that CH_3CN is long-lived in the lower stratosphere and that previously-proposed ion-molecule reactions do not play a major role as loss processes of CH_3CN.