1LATMOS-IPSL, CNRS/INSU, UMR 8190, UVSQ, UPMC, Guyancourt, France
2ACRI-ST, Sophia Antipolis, Sophia Antipolis, France
3Institute of Applied Physics, University of Bern, Bern, Switzerland
4Oeschger Centre for Climate Change Research, University of Bern, Bern, Switzerland
5FMI, Helsinki, Finland
6RIVM, Bilthoven, The Netherlands
Received: 28 Jan 2010 – Discussion started: 15 Jun 2010
Abstract. The GOMOS ozone profiles have been analysed to evaluate the GOMOS ability to capture the long-term ozone evolution at mid-latitudes during the expected recovery phase of the ozone layer. Version 5 of the operational GOMOS ozone data has been compared with data from two of the longest ground-based instruments based on different techniques and already involved with many other previous space instrument validations. Comparisons between ground-based and GOMOS data confirm the occurrence of spurious retrievals mainly occurring since 2006. Using a selected set of data it is shown that some bad retrievals are induced by the increasing dark charge of the detectors combined with an inadequate method for its correction. This effect does not only induce a continuous bias, but is rather exhibiting a bimodal distribution including the correct profiles and the bad retrievals. For long-term analyses it is recommended filtering the data according to background light conditions and star temperature (spectrum shape). The new method of the dark charge estimate proposed to be implemented in the version 6 of the ESA algorithm seems to significantly reduce the occurrence of such effects and should allow to monitor stratospheric ozone using GOMOS data with greater confidence.
Revised: 27 Oct 2010 – Accepted: 03 Nov 2010 – Published: 13 Dec 2010
Keckhut, P., Hauchecorne, A., Blanot, L., Hocke, K., Godin-Beekmann, S., Bertaux, J.-L., Barrot, G., Kyrölä, E., van Gijsel, J. A. E., and Pazmino, A.: Mid-latitude ozone monitoring with the GOMOS-ENVISAT experiment version 5: the noise issue, Atmos. Chem. Phys., 10, 11839-11849, doi:10.5194/acp-10-11839-2010, 2010.