Stratospheric ozone depletion: a key driver of recent precipitation trends in South Eastern South America
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- Gonzalez, P.L.M., Polvani, L.M., Seager, R. et al. Clim Dyn (2014) 42: 1775. doi:10.1007/s00382-013-1777-x
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On a hemispheric scale, it is now well established that stratospheric ozone depletion has been the principal driver of externally forced atmospheric circulation changes south of the Equator in the last decades of the 20th Century. The impact of ozone depletion has been felt over the entire hemisphere, as reflected in the poleward drift of the midlatitude jet, the southward expansion of the summertime Hadley cell and accompanying precipitation trends deep into the subtropics. On a regional scale, however, surface impacts directly attributable to ozone depletion have yet to be identified. In this paper we focus on South Eastern South America (SESA), a region that has exhibited one of the largest wetting trends during the 20th Century. We study the impact of ozone depletion on SESA precipitation using output from 6 different climate models, spanning a wide range of complexity. In all cases we contrast pairs of model integrations with and without ozone depletion, but with all other forcings identically specified. This allows for unambiguous attribution of the computed precipitation trends. All 6 climate models consistently reveal that stratospheric ozone depletion results in a significant wetting of SESA over the period 1960–1999. Taken as a whole, these model results strongly suggest that the impact of ozone depletion on SESA precipitation has been as large as, and quite possibly larger than, the one caused by increasing greenhouse gases over the same period.
KeywordsPrecipitationOzone depletionSouth America
The depletion of ozone in the polar Antarctic stratosphere (i.e. ‘the ozone hole’) is now widely recognized to have been a major cause of observed changes in the atmospheric circulation of the Southern Hemisphere (SH) over the last several decades. Thompson and Solomon (2002) originally noted that the ozone hole-induced lower stratospheric temperature trends over the South Pole could be traced all the way to the surface, and suggested that accompanying trends in the geopotential height would result in trends in the surface winds. Modeling evidence (Gillett and Thompson 2003; Perlwitz et al. 2008; Son et al. 2008) has since shown that the wind response to the formation of the ozone hole consists of a southward shift of the eddy-driven, midlatitude jet; in much of the literature, this shift is often referred to as a positive trend of the Southern Annular Mode (Thompson et al. 2000).
More recently, using highly-controlled modeling experiments with single forcings, two independent studies have shown that the impact of ozone depletion on the SH in the second half of the 20th Century has actually been considerably larger than the impact associated with increasing greenhouse gases (GHGs) over the same period (McLandress et al. 2011; Polvani et al. 2011a). These modeling results have now received observational confirmation (Lee et al. 2013). Furthermore, the formation of the ozone hole is now believed to have impacts well beyond the middle and high latitudes. As first shown by Son et al. (2009), the ozone hole induced a widening of the summertime Hadley circulation. Accompanying this, summer precipitation increased considerably in the SH subtropics, with the modeled patterns closely resembling those observed over the period 1979–2000, as demonstrated by Kang et al. (2011).
Within the SH subtropics, South Eastern South America (SESA) stands out as a region of great interest: it is now well documented that SESA is one of the areas with the strongest observed 20th Century regional positive precipitation trends in the entire world (Liebmann et al. 2004; Haylock et al. 2006; Barros et al. 2008; Seager et al. 2010). The strong wetting in this region has had a significant economic impact, owing to the subsequent expansion of its agricultural frontiers (Viglizzo et al. 2006; Barros et al. 2008). Understanding the causes of the recent wetting, therefore, is a question of major importance.
In Fig. 1b, we show the linear precipitation trends from 1960 to 1999. SESA stands out as a region of substantial wetting over the second half of the 20th Century, with increases as large as 50 mm/month over the 1960–1999 period. Most of the observed annual mean trend is actually explained by the DJF season.
In particular, it is immediately clear that the DJF and JJA time series in Fig. 2 are noticeably different after, approximately, 1960. To bring this out we use a flat, dashed, black line in each panel to indicate the 1901–1960 mean. In spite of the large year-to-year variability, SESA precipitation in DJF appears to start rising in the last few decades of the 20th Century, whereas the JJA time series shows no such trend.
Given that (1) the formation of the ozone hole is a major driver of atmospheric circulation changes in the SH over that same period and that (2) the ozone hole effects are largely confined to DJF, Fig. 2 offers the intriguing possibility that stratospheric ozone depletion might have played a major role in the observed SESA precipitation trends. If the recent wetting of SESA were primarily caused by increasing greenhouse gases, it would be difficult to explain why JJA and DJF show different trends.
Consequently, the objective of this paper is to document, using numerical modeling experiments with uniquely specified forcings, whether stratospheric ozone depletion is able to cause substantial wetting over SESA in DJF. Because modeling of precipitation is a difficult matter, we have opted for a multi-model approach. Our strategy is to gather a relatively large number of models, spanning a wide range of complexity, and to document the response of SESA precipitation to ozone depletion in every case. For each model we have analyzed, at least one pair of integrations with and without ozone depletion is available, with all other forcings unchanged. This allows for clear attribution of any modeled SESA precipitation changes to ozone depletion. In several cases, we are actually able to contrast the changes caused by ozone depletion to those caused by increasing greenhouse gases, given that the two forcings were independently specified in some of the models.
As we describe below, we find that all models are in agreement: they show a clear wetting of SESA in response to ozone depletion. Furthermore, while current generation models are unable to quantitatively simulate the magnitudes of the observed SESA trends, they consistently show that the response of SESA precipitation to ozone depletion is larger than the one accompanying GHG increases. And, finally, we demonstrate that SESA precipitation changes related to the formation of the ozone hole can, in the models we have analyzed, be almost entirely attributed to atmospheric circulations changes, in accordance with previous work (Kang et al. 2011).
In the remainder of the paper, these results will be discussed as follows. In Sect. 2, we present in detail the modeling output we have analyzed in this study, documenting both the model characteristics and the forcing configurations used. The main results, i.e., the response of SESA precipitation to ozone depletion in each model, are represented in Sect. 3, and the dynamical mechanism for this response is illustrated in Sect. 4. A brief summary closes the paper.
2 Data and methods
For simplicity and reproducibility of our work, we define SESA as the land area comprised between 40° S and 20° S in latitude and between 65° W and 45° W in longitude. We apply this definition uniformly across all observational and model datasets analyzed in this paper.
Since the primary objective of this study is assessing the impact of stratospheric ozone depletion on SESA precipitation, we will focus on the period 1960–1999, when most of the ozone hole formation occurred and during which a strong and statistically significant precipitation trend is observed. For the same reason, we limit our analysis to the summer months from December to February (DJF); it is well documented that, while the ozone minimum occurs in October, a lag is needed for the signal to reach the surface (e.g., Polvani et al. 2011a). Models show no response to ozone depletion during JJA, consistent with the lack of an ozone hole in that season. In addition, the largest precipitation trends in SESA have been observed in DJF.
We use observed precipitation data from WMO/DWD Global Precipitation Climatology Centre monthly dataset, version 4 (hereafter GPCCv4, Schneider et al. 2008). This dataset covers the period 1901–2007, and is available at spatial resolutions of 0.5, 1.0 and 2.5 degrees. Its main advantage rests in having been shown to reproduce SESA summer precipitation variability in good agreement with long station-based records over that region (Gonzalez et al. 2012). Throughout this study, we will use the 2.5° resolution dataset only, which is closer to the resolution of most of the model output analyzed here.
2.2 Model integrations
In order to build a strong case for the impact of ozone depletion on SESA precipitation, and given the intrinsic difficulty of modeling rainfall, we have opted to show a maximum of modeling evidence. To this end, we have taken the somewhat unusual approach of assembling into one paper nearly all currently available, pertinent, model output from a number of relevant studies that have recently appeared in the literature, and some additional, unpublished experiments. Specifically, we have included here all recent models for which integrations with and without ozone depletion are available, with forcings typical of the late 20th Century.
The advantage of this approach is that the evidence presented will come from a very wide range of models, from ‘low-top’ atmospheric general circulation models (AGCMs) with specified sea surface temperatures (SSTs) to ‘high-top’ (i.e. stratosphere resolving) coupled atmosphere-ocean models (CGCMs) with fully interactive stratospheric chemistry.
Descriptions of the model output analyzed in this paper and the experimental design
# integration name
T42 L26 (low top)
Polvani et al. (2011a)
50 years, steady forcings @ 1960 levels, SSTs from obs
As reference, but all forcings at @ 2000 levels
As reference, but GHGs & SSTs @ 2000 levels
As reference, but O3 @ 2000 levels
T63 L71 (high top)
Sigmond et al. (2010)
1 reference (CGCM)
80 years, steady forcings @1979 levels, coupled model
3 ozone-only (CGCM)
As CGCM reference, but O3 @ 2005 levels
1 reference (AGCM)
As CGCM reference, atmosphere only (SSTs from reference)
1 ozone-only (AGCM)
As AGCM reference, but O3 @ 2005 levels
T42 L26 (low top)
Unpublished, but similar to Polvani et al. (2011a)
1950–2009, all forcings transient, SST from obs
1950–2009, only O3 transient
1950–2009, only GHGs and SSTs transient
∼1° L26 (low top)
Gent et al. (2011)
1850–2005, all forcings transient
Fixed 1850 forcings, but transient GHGs 1850–2005
Fixed 1850 forcings, but transient O3 1850–2005
∼2° L66 (high top)
Garcia et al. (2007)
1960–2100, all forcings transient, modeled SSTs (REF-B2)
As REF-B2, but halogens @ 1960 levels (SCN-B2b)
As REF-B2, but GHGs and SSTs @ 1960 levels (SCN-B2b)
T31 L71 (high top)
McLandress et al. (2010)
1960–2100, all forcings transient, coupled GCM (REF-B2)
As REF-B2, but halogens @ 1960 levels (SCN-B2b)
As REF-B2, but GHGs and SSts @ 1960 levels (SCN-B2c)
2.2.1 Time-slice integrations
The simplest type of model output we have analyzed is in the form of so-called ‘time-slice’ integrations. In this configuration, models are forced with seasonally varying ozone concentrations and sea surface temperatures (if needed), but with no year-to-year trends. To evaluate the response of the climate system to ozone depletion, an initial ‘reference’ integration (many decades long) is performed, with ozone levels typical of conditions before the formation of the ozone hole. The ‘perturbed’ integrations are then carried out (also many decades long) with ozone levels typical of the decade 2000–2010, where a considerable ozone hole is present over Antarctica in SH spring. The response of the climate system to ozone depletion (or other forcings) is then computed as the difference in the climatologies between the perturbed and the reference integrations.
Two sets of previously published time-slice integrations are analyzed here: one from the Community Atmospheric Model, version 3, and the other from the Canadian Middle Atmosphere Model. A brief description of each set follows.
a. CAM3 time-slice integrations. The simplest model integrations we have analyzed were performed with the Community Atmospheric Model, version 3 (CAM3), documented in Collins et al. (2006). For these experiments, CAM3 was run with T42 horizontal resolution and 26 hybrid vertical levels, only 8 of which are located above 100 hPa. The model top being at 2.2 hPa, CAM3 can be referred to as a low-top model, in which the stratospheric circulation is poorly resolved. The SSTs were specified from Rayner et al. (2003), while the ozone fields were taken from Cionni et al. (2011).
In addition to 50-year long ‘reference’ integrations, in which all forcings were specified at year 1960 levels, three perturbed 50-year long runs were analyzed. One with all forcings set at year 2000 levels (‘all-forcings’); one with GHGs and SSTs set at year 2000 levels, but ozone kept at year 1960 levels (‘GHG-only’); and, lastly, one in which all forcings were kept at 1960 levels except for ozone, which was set at the year 2000 levels (‘ozone-only’). Additional details can be found in Polvani et al. (2011a).
b. CMAM time-slice integrations. The second set of model integrations were carried out with the Canadian Middle Atmosphere Model (CMAM), a coupled atmosphere-ocean model that extends so as to encompass the entire middle atmosphere, as detailed in Scinocca et al. (2008). For the integrations analyzed here, the model was run with T63 horizontal resolution and 71 vertical levels, reaching approximately a height of 100 km. This is, therefore, a high-top model, with a good resolution of stratospheric dynamics and its variability. The atmospheric chemical composition is entirely specified in this version of CMAM, with the ozone concentration taken from Randel and Wu (2007). The other main difference from CAM3 is that CMAM is a fully coupled atmosphere-ocean model.
The integrations analyzed here have been presented and discussed in Sigmond et al. (2010). They consist of four 80-year long integrations of the CGCM. The ’reference’ run has monthly varying and zonally symmetric ozone concentrations fixed at the year 1979 (the pre-ozone hole state). Additionally, three ‘ozone-only’ integrations are identical to the ‘reference’, except the ozone concentrations were changed to the severely depleted 2005 levels.
In addition to these coupled integrations, a pair of 80-year integrations (‘reference’ and ‘ozone-only’) were performed with the atmospheric component of the model alone, for which the SSTs were specified from the corresponding coupled integrations above. We label these with ’AGCM’ to distinguish them from the CGCM runs.
For clarity, we point out that these CMAM time-slice integrations, for which no GHG-only experiment is available, are included in the analysis to complement the assessment of stratospheric ozone depletion.
2.2.2 CAM3 transient integrations
The next step in model complexity is given by a low-top AGCM (CAM3) with time-varying forcings over the second half of the 20th Century. These integrations are the only ones analyzed in this paper which have not been presented in prior publications, although they are very similar to the CAM3 time-slices. Specifically, identical CAM3 configuration and forcing dataset were used as in Polvani et al. (2011a), except that the forcings vary continuously from 1960 to 2000.
Since these are transient runs, there is no need for a ’reference’ integration. Three ensembles of integrations were performed in transient mode: their names—‘all-forcings’, ‘GHG-only’ and ‘ozone-only’—are self explanatory. Each ensemble has 40 members, constituting the largest set analyzed in this paper.
2.2.3 CCSM4/CMIP5 transient integrations
From transient runs with an atmosphere-only model (CAM3), we next consider transient runs with a coupled atmosphere-ocean model (with land surface and sea-ice components), the Community Climate System Model, version 4 (CCSM4). This is one of the models used by the National Center for Atmospheric Research (NCAR) to produce simulations for the Climate Model Intercomparison Project, Phase 5 (CMIP5). For the output analyzed here, the resolution of the model atmosphere was 1.25° longitude by 0.9° latitude (called ‘1° version’), with 26 vertical levels (a low-top model); this was coupled to the Parallel Ocean Program version 2 (POP2), as described by Smith et al. (2010). Further details about the CMIP5 configuration of CCSM4 can be found in Gent et al. (2011).
‘all-forcings’: these are CCSM4/CMIP5 historical integrations, which include all the transient forcings. An ensemble of 5 such integrations is available.
‘GHG-only’: only the GHGs concentration are transient, with all other forcings fixed at 1850 levels. An ensemble of 3 such integrations is available.
‘ozone-only’: only the ozone forcing is transient, as described in Lamarque et al. (2010). All other forcings are fixed at 1850 levels. An ensemble of 3 such integrations is available.
2.2.4 CCMVal-2 transient integrations
Last in order of complexity, we analyzed several sets of integrations that were performed as part of the Stratospheric Processes and their Role on Climate (SPARC) Chemistry-Climate Model Validation phase 2 (CCMVal-2) project, described in SPARC (2010). For these integrations, state-of-the-art chemistry-climate models were used. In brief, these are high-top models (with good resolution of the stratospheric circulation) and with interactive stratospheric chemistry (e.g., Morgenstern et al. 2010). Such models are typically used for the scientific assessments of ozone depletion (WMO 2010). Output from two such models was analyzed in this paper: the Whole Atmosphere Community Climate Model (WACCM) and the Canadian Middle Atmosphere Model (CMAM). A brief description of each set follows.
WACCM The version of the Whole Atmosphere Community Climate Model used for the integrations analyzed here is fully described in Garcia et al. (2007). WACCM was run at 1.9° by 2.5° horizontal resolution, with 66 vertical levels, and a model top at about 150 km. In addition to interactive stratospheric chemistry, this version of WACCM also includes many upper atmosphere processes (e.g., ion chemistry in the mesosphere, auroral processes, etc). Finally, we note that this version of WACCM was run with specified SSTs, which were taken from model output from CMIP3 integrations.
CMAM The version of CMAM used here is quite similar to the one described in Sect. 2.2.1 above. There is one key difference: this version was integrated with interactive stratospheric chemistry. Because of the computational cost associated with the chemistry component, the horizontal resolution was reduced to T31, with the model top at 0.00081 hPa. Compared to WACCM, these CMAM integrations have the advantage of being fully coupled to the NCOM 1.3 ocean general circulation model. This model configuration, and the associated integrations described below, are documented in McLandress et al. (2010). The chemistry-coupled version of CMAM is, in terms of complexity, the most comprehensive of the models we have analyzed.
‘all-forcings’: these integrations, over the period 1960–2100, are meant to cover the past and extend into the future, using forcings from the SRES A1B scenario. To insure continuity between the past and future, these integrations do not include solar variability and volcano activity, but they do include all anthropogenic forcings. The SSTs are either specified from another model (in the case of WACCM), or are part of the model itself (in the case of CMAM). For reference, these integrations were labeled ’REF-B2’ in the CCMVal-2 project. Further details can be found in Sect. 2.5 of the SPARC Report (SPARC 2010).
‘GHG-only’: these integrations are identical to the all-forcings ones above, but with surface halogen concentrations fixed at the 1960 (i.e.; at pre-ozone hole) levels. In these integrations, no ozone hole forms over the South Pole. These integrations were labeled ’SCN-B2b’ in the CCMVal-2 project.
‘ozone-only’: these integrations are identical to the all-forcings ones, but with GHGs and all other forcings fixed at the 1960 levels; specifically, the SSTs are taken as the 1955–1964 average of the REF-B2. They were labeled ’SCN-B2c’ in the CCMVal-2 project.
2.3 Calculating the change due to ozone depletion and its significance
In summary (see Table 1), we have studied 6 sets of model configurations: two sets of time-slice integrations (a low-top AGCM and a high-top CGCM), and four sets of transient runs (a low-top AGCM, a low-top CGCM, and two with high-top chemistry coupled models).
For every model, we are interested in documenting the response of SESA precipitation to external forcings. In order to quantitatively compare model output from the time-slice and transient integrations, we compute the ‘change’ in precipitation, which we define as follows. For the time-slice integrations, it is simply the difference between the perturbed and reference integrations, pro-rated by the length of the run. For instance, for the CMAM time-slice integrations (see Sect. 2.2.1.b above), the forcing period (in terms of ozone depletion) is somewhat smaller (1979–2005) than in the other models (1960–1999); so we compute the change for 1979–2005, in mm/month for a 27-year period, and then we re-scale it for a 40-year period, to get a precipitation change commensurate with the other models. For all the transient integrations, the ‘change’ is constructed by first computing the linear trend from 1960 to 1999, and then multiplying it by 40 years.
In the case of the time slices, the statistical significance is assessed using a t test as in Kang et al. (2011). When more than one time-slice is available for a same experiment, they are considered as a single concatenated run. For the transient integrations, the statistical significance of the linear trend for the period 1960–1999 is assessed using a Mann-Kendall test (Mann 1945; Kendall 1975). When multiple ensemble members were available, the significance test was applied to the ensemble mean.
3 Modeled SESA precipitation changes
3.1 The CMIP simulations
Each panel presents both the individual and the multi-model mean for 1960–1999 changes over SESA. The values in the top panel are for the CMIP3 models for which we used the ‘20C3M’ simulations (Meehl et al. 2007). In the bottom panel we show the CMIP5 results, for which we have used the ‘historical’ simulations (Taylor et al. 2012).
The key point to be made from this figure is that the CMIP multi-model means (grey bars) severely underestimate the observed precipitation trends (black bars) over SESA. For the CMIP3 models (top panel), this was already noted in Seager et al. (2010), although we are here specifically focusing on the last four decades of the 20th Century, when the largest trends are observed. The lower panel of Fig. 3 confirms that the same remains true for the CMIP5 trends.
There is some indication in Fig. 3 that the CMIP5 models agree better with the observations than the CMIP3 models, although the multi-model mean precipitation trend in the latest CMIP is still smaller than that in the observations—by more than a factor of 5. Closer inspection reveals that just a few models (i.e., GFDL-CM3 and HadGEM2-ES) account for most of the increase in the multi-model trend; note also that 8 of the 26 models in the ensemble still produce negative trends.
The blue bars in Fig. 3a show two subsets of CMIP3 models, with and without ozone depletion specified. As documented in Son et al. (2009), approximately half the models in CMIP3 did not include the formation of the ozone hole as a forcing in the 20C3M simulations. Comparing the two blue bars in Fig. 3a (left: fixed ozone; right: varying ozone) appears to suggest, however, that ozone depletion does not have a significant effect on SESA precipitation. Such a conclusion, however, would be premature, since many other forcings differ between the two sets of simulations. See, as a cautionary example, the recent commentary of Previdi and Polvani (2012) on Hu et al. (2011).
For the CMIP5 historical simulations, all modeling groups were asked to include ozone depletion as part of the 20th Century forcings (Taylor et al. 2012), although the actual ozone forcings were not uniquely specified, and therefore differ greatly (Eyring et al. 2012). Since no CMIP5 models lack ozone depletion, one cannot carry out an exercise similar to the one we have just discussed for CMIP3. We have, however, attempted to see if one may be able to document the importance of a well-resolved stratosphere by segregating the high-top and low-top models in CMIP5, following Gerber et al. (2012). As shown by the blue bars in Fig. 3b, it would appear that the low-top models are slightly closer to the observations. This, however, would be a premature conclusion, since other differences exist between the two sets of models. Difference in SESA precipitation trends cannot be attributed to model top alone from the CMIP5 ensemble.
From this discussion we therefore conclude that the CMIP model output is the wrong tool to assess the impact of ozone depletion on SESA precipitation. This is why we have decided to analyze sets of models where a single forcing is changed at a time. We consider this to be a rigorous way to study cause and effect relationships using climate models.
3.2 The time-slice integrations
3.2.1 The CAM3 time-slice integrations
In order to assess the importance of ozone depletion from the simplest to the most complex models, we start by discussing SESA precipitation changes in the low-top, CAM3 time-slice integrations of Polvani et al. (2011a). For this model, three perturbed integrations are available (GHG-only, ozone-only and all forcings), all of which can be contrasted to the reference integration.
The precipitation change for the all-forcings integration shows a clear wetting over most of SESA (Fig. 4b), in agreement with observations. The overall spatial pattern of the change over South America, however, shows significant differences from the observed pattern (Fig. 1b), especially north of 20° S. In particular, the eastern Brazilian coast shows wetting, which is opposite to the observed change. Analogous problems are found to the north of the equator.
The GHG-only integration (Fig. 4c) shows a very similar spatial pattern, in the tropical region, to that in the all-forcings case. This suggests that those patterns are mainly due to the increase in GHGs. Over the SESA box, however, the modeled changes are mainly negative, whereas in the observations they are mostly positive (see Fig. 1b). We conclude that GHGs are unable to produce the observed wetting of SESA in this model.
In contrast, the ozone-only integration (Fig. 4d) shows a spatially-coherent—albeit small—wetting over SESA. Since the prominent dipolar feature over eastern Brazil (which one can see in the all-forcings case, Fig. 1b) is absent in the ozone-only integration, we conclude that observed changes in the tropical sector of South America are due to increased GHGs in this model. The wetting of SESA, however, appears to be mainly caused by ozone depletion.
3.2.2 The CMAM time-slice integrations
The lower panels of Fig 6 show the changes resulting from ozone depletion, as obtained from the ozone-only integrations, for the coupled and uncoupled versions of the model (left and right, respectively). It is clear that in CMAM, SESA exhibits mostly wetting under ozone depletion in both versions of the model, but with some differences. In the uncoupled version (Fig. 6d) the changes are closer to the observations, due to the fact that a dipolar pattern with NW-SE orientation is seen in the model between SESA and eastern Brazil, together with a wetting in the northwestern Andes (cf. with Fig. 1b).
In order to directly compare the results from CMAM and CAM3, we show the CMAM precipitation change due to ozone depletion with dark green bars in Fig. 5. Note that the CMAM changes are larger than the CAM3 changes, for both the coupled and uncoupled integrations, though they are not significant at the 90 % level, and they amount to about one quarter of the observed change. For the CGCM, the superimposed black line shows the scatter among the 3 available integrations, which is smaller than the change itself. In fact, all three coupled integrations show positive precipitation changes over SESA. Therefore, the CMAM results corroborate the above CAM3 results, and show that ozone depletion alone is able to cause modeled wetting over SESA.
3.3 The CAM3 transient integrations
Similarly, contrasting Figs. 7b and Fig. 4b, one can see that the precipitation changes over 1960–1999 in the all-forcings ensemble are also similar to the time-slice ones, with wetting over SESA as observed, but with changes in eastern Brazil and tropical South America opposite in sign to the observations. Unlike the time-slice integrations, however, in the case of the GHG-only ensemble (Fig. 7c), wetting is observed over SESA, although less generalized than in the ozone-only ensemble (Fig. 7d). In this last case, the dipolar structure in the change between SESA and eastern Brazil is also present, though somewhat weaker than in the observations (Fig. 1b).
These transient CAM3 results are summarized by the orange bars in Fig. 5, which show wetting over SESA for the 1960–1999 period in all three ensembles, although weaker than the observations. Note that the GHG-only ensemble (central orange bar), explains a smaller positive change than the ozone-only ensemble (rightmost bar). Note also that while the spread among the 40 members is quite large in all cases (black lines), the interquartile range (gray lines)—containing the central 50 % of the ensemble members— encompasses only positive values for the all-forcings and ozone-only ensembles, whereas it includes both negative and positive values in the GHG-only case. Furthermore, we find that the ozone-only ensemble mean alone is significant at the 90 and 95 % levels. This would suggest that ozone-depletion might be a more important forcing for SESA precipitation changes than GHG increases.
3.4 The CCSM4/CMIP5 transient integrations
This conclusion is greatly reinforced by the next set of transient model integrations we analyzed. These were performed as part of the CMIP5 project with CCSM4. This low-top, atmosphere-ocean-land-sea-ice model is a very recent version of NCAR’s coupled climate model and, as such, can be thought of as a state-of-the-art IPCC-class CGCM. Three ensembles are available: all-forcings, GHG-only and ozone-only. Unfortunately, these ensembles are relatively small (only a few members each), but still allow us to get a sense of the magnitude of the internal variability (Deser et al. 2012).
The corresponding changes are shown in Fig. 8b. These patterns are quite similar to the observations (Fig. 1b), though apparently shifted south, which might be due to an overall model bias. Nevertheless, more than half of the SESA box exhibits clear wetting, and the eastern coast of Brazil shows drying. For the GHG-only ensemble (Fig. 8c), the signal over SESA is highly mixed, with large cancellation suggesting a very small overall SESA change. In contrast, the ozone-only ensemble (Fig. 8d) shows a very clear wetting over all of SESA.
The precipitation changes for these integrations, averaged over the SESA box, are indicated by the red bars in Fig. 5. While the changes are positive for all three ensembles, they are much larger in the ozone-only case. In fact, the changes for the ozone-only ensemble are positive for each member, whereas for the GHG ensemble they are negative in some cases. We acknowledge that these single-forcing integrations have small ensembles (only 3 members each), which probably explains the small spread in comparison with the all-forcings ensemble. While none of the ensemble mean changes are statistically significant at the 90 % level, these results are in agreement with the ones obtained from the previous analysis, and together provide compelling evidence that ozone depletion has been an important forcing of the SESA precipitation trend.
3.5 The CCMVal-2 transient integrations
The high-top models discussed in this and the next section further corroborate this possibility. These models include, in addition to a full representation of stratospheric dynamics, interactive stratospheric chemistry. Therefore, only surface concentrations of ozone-depleting substances are specified in these model, instead of the entire latitude-height ozone fields. We analyze here two such models, whose ensembles were performed for the CCMVal-2 project.
3.5.1 The WACCM transient integrations
The key point of the figure comes from comparing the changes in the GHG-only (Fig. 9c) and ozone-only (Fig. 9d) sets. These suggest that most of the simulated precipitation increase in the subtropics (and hence SESA) in the all-forcings integrations are due to the ozone forcing, whereas the changes observed in the more tropical sector are due to a combination of both forcings.
The light blue bars in Fig. 5 summarize these findings. Note that the mean SESA change in the all-forcings ensemble is slightly negative, due to this model’s bias in the positioning of the wetting band. However, the spread among the members is very large, and does encompass large positive changes. Unfortunately only a single member is available for the single-forcing integrations. In addition, none of the ensemble mean changes are statistically significant at the 90 % level. With those caveats, we nonetheless observe that precipitation changes are larger in the ozone-only than in the GHG-only integrations for this model as well.
3.5.2 The CMAM transient integrations
The last piece of evidence implicating ozone depletion on SESA precipitation changes comes from the most complex model in this study. The version of CMAM analyzed here consist of a stratosphere resolving (high-top) atmospheric model, with interactive stratospheric chemistry, and coupled to an interactive ocean model. The integrations discussed here have been carefully documented in the literature (McLandress et al. 2010, 2011), and we focus uniquely on SESA precipitation changes over the period 1960–1999.
Nonetheless, the all-forcings ensemble mean (Fig. 10b) shows a clear precipitation increase over SESA, also found in every member of the ensemble (not shown). In fact, as one can see from the dark blue bars in Fig. 5, these CMAM integrations show the largest computed SESA precipitation changes of all the models we have analyzed.
From the single-forcing experiments, it is clear that a large precipitation increase occurs in the ozone-only ensemble (Fig. 10d), whereas the GHG-only (Fig. 10c) ensemble exhibits mostly negative changes over SESA, albeit with a very large spread among its integrations (Fig. 5). Notice, in contrast, that the mean precipitation changes are positive for the ozone-only set, with only one member showing slight drying over SESA. Only the all-forcings ensemble mean change is significant at the 90 % level.
In this model, as in others examined above, the evidence for the role of ozone depletion is not conclusive. It is, however, the accumulation of such evidence over a large array of models (with very different complexity) that imparts robustness to the key result of this paper.
4 The dynamics of ozone-depletion induced precipitation changes
Additional evidence can be offered from the dynamical mechanism associated with the precipitation changes that result from imposing ozone depletion in these integrations. We illustrate the mechanism with the 40-member CAM3 transient ensemble, as we have computed these ourselves, and therefore all the variables are easily available to construct a clear picture.
The link between this increased upwelling and the midlatitude jet shift can be seen in the red and blue contours in the top panel of Fig. 11c: these contours represent the changes in the monthly-mean, transient eddy momentum fluxes for a limited longitudinal range in the vicinity of Southern South America. Specifically, the momentum flux divergence centered around 35° S in the upper troposphere is balanced by an anomalous southward upper tropospheric flow, which in turn forces upward motion between 20° S and 35° S (as shown by the vertical velocity changes in green shades). Consistent with this, the bottom panel of Fig. 11d shows that this latitudinal band exhibits increases both in vertically integrated precipitable water (green curve) and in precipitation itself (blue bars). This mechanism is exactly the one proposed in Kang et al. (2011) to explain the ozone-induced average wetting of the SH subtropical band. As in their assessment, these results show that the SESA precipitation changes due to ozone depletion in these integration are driven by circulation changes rather than thermodynamic ones.
5 Summary and conclusions
The impact of stratospheric ozone depletion on precipitation in South Eastern South America was analyzed in a hierarchy of numerical experiments with different general circulation (both AGCMs and CGCMs) and climate-chemistry models. All the GCMs considered in this study underestimate the precipitation change over SESA but, as we have illustrated with the CMIP3 and CMIP5 ensembles, this is a widespread deficiency of all recent-generation climate models.
That said, we have found a unanimous agreement across the ensemble means of all model integrations we analyzed: specifying ozone depletion alone as a forcing agent results in a clear increase in SESA precipitation. Furthermore, the same model integrations show that, for the period 1960–1999, increasing GHGs cause either small or negative changes in SESA precipitation—unlike ozone-depletion, the GHG forcing does not show a consensus among the models. Taken together, these results suggest that stratospheric ozone depletion has significantly contributed to the observed wetting in the region during 1960–1999, and that its impact has been as large as, and possibly larger, than the one caused by increasing GHGs.
The mechanism proposed by Kang et al. (2011), which we have confirmed with the new integrations shown here, only offers an explanation for the zonal mean changes. A more detailed dynamical analysis is needed to understand the zonal asymmetries associated with the ozone-induced precipitation changes over South America and the surrounding oceans. In particular, topographic features in the region and their influence on the mean flow are likely to be important, and this would require the use of higher resolution or regional climate models.
The results of this work are of particular relevance for the coming decades, since the ozone layer is predicted to recover by the second half of the 21st Century (WMO 2010). As the ozone hole closes, the effects of ozone recovery will oppose and possibly overwhelm the effects of increasing GHGs, notably on the position of the midlatitude jet, the extent of the Hadley circulation, and the associated subtropical precipitation, as documented in a number of recent studies (Son et al. 2010; Arblaster et al. 2011; McLandress et al. 2011; Polvani et al. 2011b). Therefore, if the recently observed increase in SESA precipitation changes is partly caused by ozone-induced circulation changes, as we are here suggesting, we might infer that precipitation will stabilize or, possibly, decrease in the coming decades, as a consequence of ozone recovery. Foreseeing such a scenario could have a significant impact in the region’s economic and agricultural strategies, which are of great relevance to the World’s grain and food productions.
PG and RS were supported by NSF EaSM award 1049066 (Multi-scale Climate Information for Agricultural Planning in Southeastern South America for Coming Decades). RS was also supported by NOAA award NA10OAR4310137 (Global Decadal Hydroclimate Change and Variability, GloDecH). LMP is supported by a grant from the NSF to Columbia University. We acknowledge the World Climate Research Programme (WCRP) Working Group on Coupled Modeling; the US Department of Energy’s Program for Climate Model Diagnosis and Intercomparison (CMIP) provides coordinating support and led development of software infrastructure in partnership with the Global Organization for Earth System Science Portals. For the chemistry-coupled models, we thank the Chemistry-Climate Model Validation (CCMVal-2) Activity for the WCRP SPARC (Stratospheric Processes and their Role in Climate) project for organizing and coordinating the model data analysis activity. Special thanks to John Fyfe and Michael Sigmond, for allowing us to use their data for the CMAM time-slice integrations.
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