Abstract
JOURNAL OF GEOPHYSICAL RESEARCH,
VOL. 109,
D06105,
10 PP., 2004
doi:10.1029/2003JD004099
CO as an important high-altitude tracer of dynamics in the polar stratosphere and mesosphere
Institute for Terrestrial and Planetary Atmospheres, State University of New York, Stony Brook, New York, USA
Physics Department, University of Rome, “La Sapienza,” Rome, Italy
We present new ground-based measurements of polar stratospheric and mesospheric CO, made with a millimeter-wave spectrometer
at Thule, Greenland (76.5°N, 68.7°W). Almost daily measurements were made between 17 January and 4 March 2002 and again between
5 January and 22 February 2003. We stress here the retrieval and analysis of CO mixing ratios in the 50–80 km altitude range,
though it can be monitored at lower altitudes as well. Since CO exhibits a strong positive latitude gradient from the summer
to the winter pole, it is an excellent tracer for poleward transport from lower latitudes. Moreover, the mixing ratio of CO
increases rapidly from ∼40 km to at least 100 km at midlatitudes, providing a good tracer for high-altitude vertical transport
as well. Our profiles indicate that in winter near the poles the CO mixing ratio decreases above ∼70 km because of subsidence
of air and minimal high-altitude photoproduction at high latitudes. Our data also show large variations in mixing ratio and
vertical distribution, yielding a good picture of stratospheric and mesospheric dynamics-induced changes on a scale of hours
to days. These observations verify that CO serves as an excellent tracer of vortex-related dynamics in the 30–80 km altitude
range, where other information, particularly above ∼40 km, may be sparse, unreliable, or nonexistent. Our results are in general
agreement with analyses of 1991–1992 Improved Stratospheric and Mesospheric Sounder (ISAMS) satellite data by
Received 22 August 2003; accepted 16 January 2004; published 20 March 2004.
Citation: (2004), CO as an important high-altitude tracer of dynamics in the polar stratosphere and mesosphere, J. Geophys. Res., 109, D06105, doi:10.1029/2003JD004099.
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