Abstract

Abstract. Within the framework of the second SPARC (Stratosphere-troposphere Processes And their Role in Climate) water vapour assessment (WAVAS-II), profile-to-profile comparisons of stratospheric and lower mesospheric water vapour were performed by considering 33 data sets derived from satellite observations of 15 different instruments. These comparisons aimed to provide a picture of the typical biases and drifts in the observational database and to identify data-set-specific problems. The observational database typically exhibits the largest biases below 70 hPa, both in absolute and relative terms. The smallest biases are often found between 50 and 5 hPa. Typically, they range from 0.25 to 0.5 ppmv (5 % to 10 %) in this altitude region, based on the 50 % percentile over the different comparison results. Higher up, the biases increase with altitude overall but this general behaviour is accompanied by considerable variations. Characteristic values vary between 0.3 and 1 ppmv (4 % to 20 %). Obvious data-set-specific bias issues are found for a number of data sets. In our work we performed a drift analysis for data sets overlapping for a period of at least 36 months. This assessment shows a wide range of drifts among the different data sets that are statistically significant at the 2σ uncertainty level. In general, the smallest drifts are found in the altitude range between about 30 and 10 hPa. Histograms considering results from all altitudes indicate the largest occurrence for drifts between 0.05 and 0.3 ppmv decade−1. Comparisons of our drift estimates to those derived from comparisons of zonal mean time series only exhibit statistically significant differences in slightly more than 3 % of the comparisons. Hence, drift estimates from profile-to-profile and zonal mean time series comparisons are largely interchangeable. As for the biases, a number of data sets exhibit prominent drift issues. In our analyses we found that the large number of MIPAS data sets included in the assessment affects our general results as well as the bias summaries we provide for the individual data sets. This is because these data sets exhibit a relative similarity with respect to the remaining data sets, despite the fact that they are based on different measurement modes and different processors implementing different retrieval choices. Because of that, we have by default considered an aggregation of the comparison results obtained from MIPAS data sets. Results without this aggregation are provided on multiple occasions to characterise the effects due to the numerous MIPAS data sets. Among other effects, they cause a reduction of the typical biases in the observational database.

Highlights

  • Water vapour in the stratosphere and lower mesosphere is important for a number of reasons

  • In our analyses we found that the large number of MIPAS data sets included in the assessment affects our general results as well as the bias summaries we provide for the individual data sets

  • This is because these data sets exhibit a relative similarity with respect to the remaining data sets, despite the fact that they are based on different measurement modes and different processors implementing different retrieval choices

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Summary

Introduction

Water vapour in the stratosphere and lower mesosphere is important for a number of reasons. Water vapour is the most important greenhouse gas. As such, it strongly affects global warming at the Earth’s surface (Riese et al, 2012; Dessler et al, 2013). Water vapour is the primary source of hydrogen radicals (i.e. OH, H, HO2). These radicals destroy ozone within autocatalytic cycles and dominate the ozone budget in the lower stratosphere and above about 1 hPa. Beyond that, water vapour is a suitable trace gas to diagnose dynamical processes in the stratosphere such as the Brewer–Dobson circulation and the overturning circulation in the mesosphere Water vapour is a suitable trace gas to diagnose dynamical processes in the stratosphere such as the Brewer–Dobson circulation and the overturning circulation in the mesosphere (e.g. Brewer, 1949; Remsberg et al, 1984; Mote et al, 1996; Pumphrey and Harwood, 1997; Seele and Hartogh, 1999)

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