Patrick Jöckel, Mark G. Lawrence and Carl A.M. Brenninkmeijer
Max Planck Institute for Chemistry, Atmospheric Chemistry Division, Mainz, GermanyJ. Geophys. Res., 104(D9), 11,733-11,743, 1999.
Abstract. Most atmospheric 14CO is produced by cosmic rays in the lowermost stratosphere and upper troposphere. The main removal process for 14CO is oxidation by OH radicals. Assuming that the spatial distribution of OH is well known, 14CO can be useful as a test-tracer for the transport properties of a three-dimensional chemical model. Conversely, if the transport schemes of the model are sufficiently realistic, in particular with respect to stratosphere-troposphere exchange, the OH distribution can be evaluated. In either case, it has to be assumed that the source of 14CO is known in sufficient detail. Two presently available distributions of cosmogenic 14C production are implemented into the Model of Atmospheric Transport and Chemistry (MATCH). The tropospheric 14CO concentrations that are obtained are relatively insensitive to the source differences. The calculations for one source distribution are performed for solar minimum and solar maximum conditions. The spatial distribution of 14CO is almost unaffected by the solar activity, and the absolute concentration levels can be scaled to the actual solar cycle conditions.