A study reveals that recent warming in the Indian Ocean and in the Pacific 'warm pool' has caused a cooling near the top of the tropical troposphere above, leading to less water vapour entering the stratosphere.
Water vapour in the stratosphere is a greenhouse gas. It is constrained from entering the stratosphere in the tropics by the thermal boundary between the stratosphere and troposphere1 — the tropical tropopause, the coldest point in the lower atmosphere. Cold-point temperatures at the tropical tropopause (Fig. 1a) have important implications for both stratospheric chemistry2 and global climate change3. The importance of the spatial distribution of temperature (Fig. 1b) is well recognized, as the temperature minimum is relevant to cloud formation and subsequent dehydration through atmospheric circulation4. In the boreal winter, for example, the lowest cold-point temperatures over the warm pool in the tropical western Pacific govern the amount of water vapour that enters the stratosphere5. It is thus critically important to understand how the zonal (longitudinal) structure of the tropical cold-point temperature would respond to global warming. Now, reporting in the Journal of Geophysical Research, Garfinkel and co-workers6 find that the warming in the tropical upper troposphere over the past 30 years has been strongest over the Indo-Pacific warm pool, where cooling near the tropopause has been strongest. They suggest that warming in the Indian Ocean and the Pacific warm pool has led to zonal asymmetry in atmospheric temperature trends, and that such trends may continue in the future.
Temperatures near the tropical tropopause are determined by a complex combination of stratospheric (top-down) and tropospheric (bottom-up) processes7. The zonal structures at 100 hPa (Fig. 1b) closely resemble the mean pattern of the equatorial planetary waves — large-scale perturbations of the atmospheric dynamical structure. These are driven by massive convection over the Indo-Pacific warm pool8, with the lowest temperatures and largest cirrus cloud fractions over the western Pacific and Maritime Continent (which includes the islands of Indonesia, New Guinea and Malaysia, and the surrounding shallow seas)9. The signature of the equatorial planetary waves is also evident in the temperature variability over intraseasonal to interannual timescales9. The responses of temperature structures at 100 and 250 hPa are reversed in sign because the maximum amplitude of equatorial planetary waves with opposite phases occurs at these two levels. The temperatures and cloud fraction near the tropical tropopause are also strongly modulated by extra-tropical stratospheric waves. These drive the Brewer–Dobson circulation (BDC) — a large-scale latitudinal circulation in the stratosphere with air rising across the tropical tropopause, moving polewards and sinking towards the extra-tropical troposphere — which is particularly evident in their seasonal cycles9,10,11 (Fig. 1c). In contrast to the equatorial planetary waves, the extra-tropical stratospheric waves are associated with zonally symmetric temperature anomalies in the lower stratosphere.
Temperatures in the lower stratosphere and upper troposphere have been changing during the past few decades. Although many studies have focused on the zonal mean component of temperature trends12, Garfinkel and co-workers concentrate on the zonally asymmetric component, and in particular on trends near the coldest point in the tropopause region. Satellite observations are used to document the zonal structure of the temperature trends, which is strongest in January, February and March. The lower stratosphere over the warm-pool region is found to have cooled more than the zonal mean, whereas the central and eastern Pacific have cooled less. However, the structure of the upper tropospheric trends is opposite in phase, with the largest warming over the warm pool. All atmospheric chemistry–climate models that are driven by observed sea surface temperature (SST) and external forcings are shown to accurately capture the observed zonal variations of these trends.
To understand the cause of the zonal structure of atmospheric temperature trends in January–March, Garfinkel et al. use an atmospheric chemistry–climate model with observed SST as the only forcing that varies over time. The simulated structure of temperature trends is similar to those from more comprehensive model integrations and satellite observations, indicating that the SST changes have driven the zonal asymmetry. An increase in SST over the Indian Ocean and the far western Pacific enhances the deep convection and thus the latent heat release in the upper troposphere that increases the amplitude of the equatorial planetary waves. This leads to warming near 250 hPa, but cooling near 100 hPa, over the Indo-Pacific warm pool. Their study represents the first effort to document and understand the cause of zonal structures in tropical atmospheric temperature trends since 1980.
Changes in the cold-point temperature would be expected to alter the amount of water vapour entering the stratosphere. The model simulation shows that less water vapour enters the stratosphere as a result of the cooling near the cold-point tropopause over the Indo-Pacific warm pool, driven by the increased SST there6. However, their work does not explain the changes in lower-stratospheric water vapour content that have been observed in the past few decades. This could partly be because other factors — such as the change of the BDC13 — would also affect the cold point-temperatures (Fig. 1c). In addition, the impact of the equatorial planetary waves and upward motion associated with the BDC on tropical thin cirrus clouds need to be investigated, and could have a warming feedback to the climate system14.
Past increases in the Indian Ocean SST have been directly linked to the global warming15 and may continue in the future. Garfinkel et al. show that there is a cooling near the tropical tropopause over the Indo-Pacific warm-pool region and thus less water vapour entering the stratosphere. This response to the SST change is due to the enhanced equatorial planetary waves. A decrease in stratospheric water vapour may lead to a slight cooling of global surface temperatures. This study demonstrates that it is of paramount importance to pay attention to, and understand the cause of, the patterns of SST changes that are related to global warming.
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Q.F. is supported by NASA grant NNX13AN49G.
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Fu, Q. Bottom up in the tropics. Nature Clim Change 3, 957–958 (2013). https://doi.org/10.1038/nclimate2039
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