Storm track sensitivity to sea surface temperature resolution in a regional atmosphere model
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A high resolution regional atmosphere model is used to investigate the sensitivity of the North Atlantic storm track to the spatial and temporal resolution of the sea surface temperature (SST) data used as a lower boundary condition. The model is run over an unusually large domain covering all of the North Atlantic and Europe, and is shown to produce a very good simulation of the observed storm track structure. The model is forced at the lateral boundaries with 15–20 years of data from the ERA-40 reanalysis, and at the lower boundary by SST data of differing resolution. The impacts of increasing spatial and temporal resolution are assessed separately, and in both cases increasing the resolution leads to subtle, but significant changes in the storm track. In some, but not all cases these changes act to reduce the small storm track biases seen in the model when it is forced with low-resolution SSTs. In addition there are several clear mesoscale responses to increased spatial SST resolution, with surface heat fluxes and convective precipitation increasing by 10–20% along the Gulf Stream SST gradient.
KeywordsAtmosphere ocean interaction Gulf Stream
The North Atlantic storm track begins over the east coast of North America where strong surface temperature gradients contribute to high baroclinicity, making the region favourable for cyclogenesis. In winter in particular, a large component of the temperature gradient is due to the contrast between the cold land and the relatively warm ocean. In addition, the sea surface temperatures (SSTs) just off the coast are characterised by very large gradients associated with the Gulf Stream, which can frequently be of the order of a few degrees Kelvin per 100 km, and also by unusually large temporal variability. It is often assumed that these strong SST gradients are important contributions to the overall baroclinicity and hence storm growth, and some recent studies have indeed supported this (e.g. Inatsu et al. 2002; Nakamura et al. 2004; Brayshaw et al. 2008; Nakamura et al. 2008). There has been much speculation that SST variations in the Gulf Stream region may lead to variations in baroclinicity which could affect storm growth and so influence the whole of the storm track (e.g. Xie 2004; Minobe et al. 2008).
It has been known for some time that in the Gulf Stream region temperature variations occur on much finer scales than those represented on coarse grids with resolutions of a few degrees, such as those used in current general circulation models (GCMs) and reanalyses. The low resolution of these models compared to those used for numerical weather prediction is often cited as one of the major sources of structural uncertainty inherent in climate projections. A key question is whether the storm track shows any sensitivity to the fine-scale structure of the SSTs, and the associated large local gradients. Is the large-scale SST distribution sufficient to represent the storm track well, or are current GCMs missing a vital link between the ocean and the atmosphere?
Doyle and Warner (1993) first presented a case study of a midlatitude storm for which a numerical forecast was indeed sensitive to the resolution of the SSTs used. Increasing the SST resolution improved both the position and intensity of the storm when compared to observations. Similar cases have since been noted by Xie et al. (2002) and Thiébaux et al. (2003). Yamamoto and Hirose (2007) found that the use of eddy-resolving SST data improved the simulation of a storm in their case study, though interestingly this was attributed to unrealistically strong SST gradients in the optimum interpolation SSTs which lacked mesoscale ocean eddies.
Regional atmosphere models are most successfully used when there is strong high-resolution forcing within the domain which is absent in the lower resolution GCM, as is often true in the presence of detailed orography. The fine-scale structure of SST fronts such as the Gulf Stream is another potential example of important high-resolution forcing. The assessment of the importance of this forcing on climate timescales has been made possible by recent developments in historical SST datasets. For some years the best historical SST dataset for many climate applications has been that of Reynolds et al. (2002), R02 hereafter. This dataset was generated by combining AVHRR 1 satellite and in situ SST observations using optimal interpolation to fill data gaps, providing a full gridded field on a 1° grid. Within the last 10 years the development of microwave satellite sensors has provided SST observations of much higher effective resolution than previously available (Wentz et al. 2000). These have confirmed the dominance of fine-scale structure in regions such as the Gulf Stream (Chelton and Wentz 2005), and show that SST gradients in these regions are generally significantly stronger than those seen in the R02 data.
We have performed three different comparisons. First we assess the importance of spatial resolution in experiments using the R07 data at full resolution and then smoothed to a resolution similar to that of R02. Then we assess the importance of temporal resolution in both of the SST datasets. Using the R02 data, we compare two experiments, one at monthly and the other at weekly frequency. Finally we compare experiments using daily and monthly versions of the R07 data. While the emphasis is on SSTs, especially in the Gulf Stream region, sea-ice is also applied as a lower boundary condition. In the spatial resolution experiment the sea-ice is unchanged, but in the temporal resolution experiments it was treated in the same way as the SST field in order to ensure consistency between sea-ice and SST fields.
2.1 The model
The model used here is HadRM3p. This is the regional version of the Hadley Centre’s third generation atmosphere model HadAM3 (Jones et al. 1995), with modifications to some physical parameterisations as described in Jones et al. (2004). The model uses a regular 0.44° latitude–longitude grid, which is rotated so that the region of interest lies over the grid’s equator, giving a roughly uniform grid size of 50 km. The model has 19 levels in the vertical. The lateral boundary conditions are applied continuously over a four point rim by relaxing the model variables towards the boundary data. The boundary conditions are specified every 6 h, with intervening values obtained by linear interpolation in time. Within the four point rim, the weighting given to the boundary conditions is 1, 0.75, 0.5 and 0.25, with the values decreasing towards the interior of the domain. No relaxation is applied in the subsequent four cells, but the orography is smoothed in these to ensure a gradual transition to higher resolution. In all the experiments described here the lateral boundary conditions are derived from the ERA-40 reanalysis (Uppala et al. 2005). The model is integrated over a large region extending from the east coast of North America to just east of the Mediterranean. The region, excluding both the four point rim and the additional four points with smoothed orography, is that shown in Fig. 1.
2.2 Spatial resolution experiment
This experiment uses the high resolution R07 SSTs which contain length scales of around 100 km in the Gulf Stream region. This data is the AVHRR-only version described by R07 and was obtained from the NOAA National Climatic Data Center. At the time of writing it was available from 1985 onwards. The data were first bilinearly interpolated onto the model grid. Coastal cells could often not be defined by this method, and values for these were chosen by averaging the SST in neighbouring ocean cells. Sea-ice concentrations were also bilinearly interpolated onto the model grid. This version of the R07 data suffers from a small level of noise near the coasts in the sea-ice field (see R07), and this necessitated some further pre-processing. Firstly the coastal cells undefined by the interpolation were defined using the ERA-40 data. Secondly any ice cells adjacent to a coast, but outside of the climatological maximum ice extent derived from ERA-40, were removed. The model was then integrated over the period January 1985–November 2000, using ERA-40 SSTs from 1984 to run the spin-up year. This gives 16 years of model output, but only 15 complete winter seasons. This run will be referred to as HIGH-RES.
The impact of SST resolution is assessed by comparing HIGH-RES to another run, called LOW-RES, which is identical except that a smoothed version of the SST data is used as a boundary condition. The smoothing was achieved by replacing each SST value by an average of the values in a 9 × 9 square of cells (roughly 450 × 450 km) centred on the cell in question. Close to the coastlines this results in unrealistic values, so successively smaller squares were used for averaging, to the point where cells adjacent to the coastline are unchanged. The sea-ice data for this run is identical to that in HIGH-RES, so that this experiment compares the effect of SST resolution in isolation. In both runs the ERA-40 SST and sea-ice values are used in the model’s four point boundary rim, in order to maintain consistency with the lateral boundary conditions. Over the next four cells the high-resolution data is introduced gradually with weightings of 0.25, 0.5, 0.75 and 1.
The smoothed R07 and ERA-40 SSTs are differenced in Fig. 2d. This shows that there are differences between the two datasets on fairly large scales, even though they are both derived from the same observations. For this reason, model runs driven by R02 and R07 SSTs are not directly comparable, and in order to cleanly assess the effect of resolution this spatial resolution experiment uses only R07 SSTs.
2.3 Temporal resolution experiments
The importance of temporal resolution is assessed using both SST datasets. First we use the low resolution ERA-40 SSTs and assess the effect of upgrading from monthly to weekly resolution. The ERA-40 SSTs are derived from the R02 dataset. The SSTs are given on a 1.125° grid but the effective resolution of the data is much coarser, as described above. These data are at weekly resolution from December 1981 onwards. Model runs were performed for 19 years from December 1981 to November 2000, after a 1 year spin-up period using monthly ERA-40 SSTs. Two runs were performed, one using monthly and the other weekly SSTs, and these will be referred to as MONTHLY and WEEKLY. The monthly data were derived from the weekly data using the AMIP II method of Taylor et al. (2000) which preserves the monthly mean values under linear interpolation. In both cases the SSTs were imposed continuously, using values linearly interpolated in time between the two nearest data points. The sea-ice was also derived from ERA-40 and was treated in exactly the same way as the SST data, so was applied at monthly and weekly frequencies in the two runs, respectively.
The second temporal resolution experiment uses the R07 data, comparing the HIGH-RES run to a run which uses a monthly version of the high-resolution SSTs and sea-ice (referred to as MONTHLY_HI), but which is otherwise identical. The SSTs for this run were created from the daily SSTs using the AMIP II method as above. The sub-monthly variations in the R07 data are characterised in Fig. 4b and d in the same way as for the R02 data. The regression map shows that, as expected, the variations have a much smaller spatial scale than in the R02 data. This confirms that the sub-monthly variations in R02 have an unrealistically large spatial scale, so it is clearly of interest to assess the sensitivity to temporal resolution using both datasets.
2.4 Storm track analysis
The storm track is analysed using the feature tracking software of Hoskins and Hodges (2002) to identify storms as maxima of vorticity at 850 hPa. Model winds are output every 3 h and used to calculate the relative vorticity on the model grid. Since the model resolution is quite high, the vorticity field contains much fine-scale structure such as fronts. In order to reliably identify the synoptic scale systems the vorticity is smoothed to a similar level as in Hoskins and Hodges, who used a T42 spectral truncation on the globe. Standard spectral methods cannot be applied to the regional model output as the domain is not periodic, so a discrete cosine transform was used to transform the vorticity field, following Denis et al. (2002). The filter of Sardeshmukh and Hoskins (1984) was then used to smooth the vorticity, with a power of 0.1 on the 1,000 km wavelength, and the smoothed data were transformed back onto the model grid. Since vorticity is used to identify features, there is no need to remove a background field from the data before tracking. Vorticity maxima were then identified as cyclones and tracked while applying constraints to ensure the tracks are suitably smooth.
The general position and intensity of the storm track in these experiments is described by the track density, defined as the number of individual cyclone tracks per unit area per season, where the area corresponds to a 5° spherical cap. The significance of differences in the track density between runs is estimated using the permutation method of Hodges (2008), in which the two sets of cyclone tracks are pooled and then resampled 2,000 times to provide a distribution of track density differences with which to compare the actual difference. Measures of storm activity are invariably noisy, so it is often hard to determine significance. The model runs used here appear to be just long enough to give some significant results for the winter season, but longer runs may be needed to produce clear results for the other seasons. The length of runs is, of course, limited by the availability of observational data.
2.5 Large-scale changes
As described above we deliberately used a large model domain to allow the possibility that the large-scale flow may diverge from that prescribed by the LBCs. This could be envisaged, for example, through modifications to the storm track and its associated mean flow forcing. However, even with a large domain, the lateral boundary conditions do partly constrain the large-scale flow, so it is not entirely free to evolve. To quantify this we use an empirical orthogonal function (EOF) analysis to identify large-scale patterns of variability in the interior flow. The driving reanalysis data are then interpolated onto the model grid to create a matching dataset, and the EOF patterns are projected onto these data to generate time series of these patterns in the reanalysis data. These time series are then correlated with the principal components in order to test the agreement between the model and the driving data. When this is performed using daily wintertime data, for all of the leading EOF patterns the resulting correlations are close to 0.7. This suggests that about 50% of the large-scale variability in the model domain is constrained by the boundary conditions.
In fact, we have found no significant differences in the mean flow, in patterns of variability, or in the occurrence of blocking regimes in any of the experiments presented here. There are, however, significant differences in the storm track, as described below. In general a change in the storm track would be expected to lead to a change in the large-scale flow. In Sect. 4 we give an example of the mean zonal wind field in the model and show that the response to changing SSTs is consistent with the change in the storm track, but that the mean wind response does not pass the significance test. This may be because the storm track changes are subtle, so the lack of any large-scale response simply reflects the weakness of the signal. However, it cannot be ruled out that the lack of a large-scale response is due to the partial control over the large-scale flow by the LBCs.
3 Storm track sensitivity to SST resolution
The storm track differences in the other seasons have also been examined, but the differences are very weak and unclear, so are not shown here. The lack of a significant response in these seasons may be due to the storm track lying further north, so that the interaction with the Gulf Stream SSTs is weaker.
There are two possible mechanisms underlying the storm track sensitivity to SST resolution, and it seems likely that both contribute to the response. Firstly, it is possible that the increased SST gradient leads to an increased temperature gradient at low levels in the atmosphere which provides for enhanced baroclinic growth. This mechanism was demonstrated by Kuo et al. (1991) in a case study of a storm growing over the Gulf Stream in a mesoscale model. Convection over the warm side of the Gulf Stream acted to destabilise the atmospheric boundary layer, leading to a strong low-level atmospheric front oriented along the Gulf Stream. The increase of convection along the warm side of the Gulf Stream in Fig. 7 shows that this process also operates in our experiment, but in this case it is not clear that the atmosphere can respond strongly to the increased baroclinicity. The SST fields used here differ mostly on scales less than 500 km, i.e. on scales which are shorter than the atmospheric radius of deformation, so the ability of baroclinic waves to make use of the increased baroclinicity is expected to be limited. Taguchi et al. (2009) have also demonstrated this mechanism acting over midlatitude ocean fronts in experiments similar to those presented here. However, the SST fields in their experiments were smoothed more strongly than those used here.
Secondly, the increased surface heat fluxes over the Gulf Stream act to warm and moisten low-level air which could provide additional latent heating to storms during their subsequent growth (Kuo et al. 1991; Hoskins and Valdes 1990). Of all the incoming small perturbations, the ones which pass over the Gulf Stream will be enhanced by this heating and this could also explain the shift of the storm track onto the SST gradient.
4 Storm track sensitivity to SST frequency
Storm tracking has been performed for all seasons, though of course the storm track is at its strongest in winter. In the other seasons there are many weak systems which obscure the signal. There are some consistent differences between the two runs in the other seasons, in that they all share the winter signal of an increase in storm activity extending north of the UK and into Scandinavia, but the pattern is very weak and does not pass the significance test. The pattern becomes clearer if the weaker systems are excluded, for example by restricting attention to only the top 50% of storms (by intensity) in each season. However, even then the significance test is not passed, so longer simulations would be required to decide if there is a significant response.
We cannot identify the mechanism behind the storm track sensitivity to SST frequency, but there are several possibilities. The temporal smoothing implicit in the monthly data will mean there are fewer periods of unusually large SST gradients, and hence baroclinicity. However, this mechanism might be expected to have a smaller influence when using the high-resolution SSTs (Fig. 4). Note that the extreme gradients in the Gulf Stream region do not appear to be affected by the temporal averaging (the analysis of Fig. 3 was repeated using the monthly ERA-40 data, and the distribution is virtually unchanged). Alternatively, with sub-monthly SSTs there will also be an enhanced variance of the air–sea temperature contrast, which could affect the latent and sensible heat fluxes. It is, of course, possible that enhanced sea-ice variance is responsible, although given the location of the storm track signal this seems unlikely.
5 Comparison to ERA-40
The results presented above show that the storm track is sensitive to both the temporal and spatial resolution of SSTs. It is of interest to compare the storm track in these simulations with that in the ERA-40 data. To generate storm track statistics for the ERA-40 data, the winds were first interpolated onto the model grid using linear interpolation. The vorticity was calculated and then this was smoothed using the discrete cosine transform described in Sect. 2.4. This smoothing ensures that features are tracked at the same resolution in both model and reanalysis data, despite the differing resolutions of the original data. The ERA-40 data are only available at six hourly intervals, so for this comparison the model data were sub-sampled to six hourly resolution before tracking.
A regional atmosphere model has been used over a large North Atlantic domain to investigate the sensitivity of the storm track to the spatial and temporal resolution of SST data. Firstly, it is clear that the model reproduces the general structure of the storm track very well when compared to the ERA-40 data, which are used as lateral boundary conditions.
This work has shown that, in general, the storm track is sensitive to the SST data used as a lower boundary condition. Large-scale differences between the low-resolution R02 and high-resolution R07 data motivated the use of separate experiments to assess the impact of improving spatial and temporal resolution within the same dataset. These show that the storm track is sensitive to both the temporal and spatial resolution of the SSTs. Increasing the horizontal resolution acts to shift the storm track partly off the North American coast and onto the Gulf Stream temperature gradients. Increasing the temporal resolution from monthly to weekly (or daily) increases the storm activity over the Gulf Stream and leads to significant changes in activity over Europe. The character of these European changes is similar in experiments with both SST datasets, but the location which is affected most does depend on the dataset used.
This work has shown that the storm track is sensitive to changes in the spatial and temporal resolution of SSTs, though interestingly an improvement in resolution, particularly temporal, does not always lead to an improved simulation when compared to observations. Increasing the temporal resolution of SST data of low spatial resolution can lead to fast SST variations of unrealistically large length scales.
The storm track sensitivity shown here is small, but significant, and while the changes are generally in the detailed structure of the storm track, some of these changes occur over populated regions, and they may be important. For example, since the response of the North Atlantic storm track to increased greenhouse gas forcing is often subtle (Bengtsson et al. 2006), it may be important that the detailed structure of the storm track is represented as well as possible in climate models. Also, since the effect of increased spatial resolution is to pull the start of the storm track off the North American coast and onto the strong SST gradient, this could mean that the storm track is more sensitive to SST variability than is apparent in low-resolution models.
It should also be remembered that, since the lateral boundary conditions constrain roughly 50% of the large-scale variability in the model, the results shown here may be an underestimate of the impact of increasing SST resolution. In addition, Chelton et al. (2006) found that fine-scale wind structure in the atmospheric boundary layer is underestimated even in high resolution models driven by high resolution SSTs, and Song et al. (2009) have shown that this arises due to an underestimate of vertical diffusion in the boundary layer. Although these studies used different models to that used here, it is possible that limitations in the boundary layer scheme could also be leading to an underestimate of the sensitivity of the storm track to SST resolution in our experiments.
Advanced Very High-Resolution Radiometer.
This work was performed as part of the NERC RAPID Climate Change programme and was supported by the Defra and MoD Integrated Climate Programme—(Defra) GA01101, (MoD) CBC/2B/0417_Annex C5. We would like to thank Richard Reynolds for help and advice on the use of the SST data, and Dudley Chelton and the anonymous reviewers for comments which have helped to improve the paper.
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