Recent Near-surface Temperature Trends in the Antarctic Peninsula from Observed, Reanalysis and Regional Climate Model Data

This study investigates the recent near-surface temperature trends over the Antarctic Peninsula. We make use of available surface observations, ECMWF’s ERA5 and its predecessor ERA-Interim, as well as numerical simulations, allowing us to contrast different data sources. We use hindcast simulations performed with Polar-WRF over the Antarctic Peninsula on a nested domain configuration at 45 km (PWRF-45) and 15 km (PWRF-15) spatial resolutions for the period 1991−2015. In addition, we include hindcast simulations of KNMI-RACMO21P obtained from the CORDEX-Antarctica domain (~50 km) for further comparisons. Results show that there is a marked windward warming trend except during summer. This windward warming trend is particularly notable in the autumn season and likely to be associated with the recent deepening of the Amundsen/Bellingshausen Sea low and warm advection towards the Antarctic Peninsula. On the other hand, an overall summer cooling is characterized by the strengthening of the Weddell Sea low as well as an anticyclonic trend over the Amundsen Sea accompanied by northward winds. The persistent cooling trend observed at the Larsen Ice Shelf station is not captured by ERA-Interim, whereas hindcast simulations indicate that there is a clear pattern of windward warming and leeward cooling. Furthermore, larger temporal correlations and lower differences exhibited by PWRF-15 illustrate the existence of the added value in the higher spatial resolution simulation.


Introduction
The Antarctic continent possesses a unique geography that is vital for our understanding of climatic phenomena on local and large scales. In addition, some of the strongest and most convincing evidence of climate change was obtained from studies over West Antarctica and the Antarctic Peninsula, and provided important arguments about the long-term future effects of global climate change such as surface warm-ing and melting (Marshall et al., 2006;Steig et al., 2009;Bromwich et al., 2013aBromwich et al., , 2014Holland et al., 2019). Despite the important evidence for climate change and its impacts on cryosphere and ecosystem processes (e.g., Rignot et al., 2004;Cape et al., 2014), the Antarctic continent suffers from inadequate observational coverage due to its remote and harsh environmental conditions. This imposes a limitation on the surface meteorological data to characterize and reduce the uncertainty of climate change.
Although the Antarctic Peninsula has more research stations compared to the rest of the Antarctic continent, several meteorological stations are underused due to a lack of archiving and complete time series (Lazzara et al., 2012;Fraiman et al., 2014). This is an impediment to expanding our knowledge of the climate variability of the peninsula. In particular, the Antarctic Peninsula cordillera constitutes an orographic obstacle to the westerlies, and thus the peninsula presents two different climatic zones: a relatively mild and humid marine climate on the west coast (windward), where northwesterly winds prevail, and a cooler continental climate on the east coast (leeward) (Fig. 1) mainly affected by southerly winds (King and Turner, 2009). The steep terrain of the Antarctic Peninsula, therefore, results in harsh conditions that further prevent the deployment of extensive field observations to obtain long-term records. On the one hand, with the aid of few available long-term surface meteorological records, the Antarctic Peninsula is considered to be one of the most vulnerable climate change "hotspots" with a long-term warming trend in near-surface temperature observed over the last 50 years [e.g., Faraday/Vernadsky station, 2.94°C (50 yr) −1 ] (Marshall et al., 2006;Turner et al., 2016, Jones et al., 2019. However, since the late 1990s, a cooling period has been observed in the Antarctic Peninsula that is attributed to atmospheric teleconnections (Car-rasco, 2013;Turner et al., 2016;Oliva et al., 2017). On the other hand, a sparse observation network prevents extensive analyses to minimize the regional-scale uncertainties associated with climate variability and trends. Excluding the relatively short time series of satellite products, one common method of overcoming the difficulties arising from the inadequate observational network is to use gridded atmospheric data at high temporal resolution (i.e., reanalysis data) and/or high spatial resolution regional climate models (RCMs) to represent the main surface climatic features as well as to explore physical mechanisms behind the observed changes.
In recent years, atmospheric reanalysis data have been widely used for various studies such as surface climate characteristics of the Antarctic region as well as large-scale atmospheric forcing mechanisms modifying the surface climate variables. In a recent study, Gossart et al. (2019) performed a comprehensive comparison and evaluation of different reanalysis products in representing the surface climatology of the Antarctic Ice Sheet. They demonstrated that, although the reanalysis products could be useful tools, they can perform very differently depending on the region of interest, season and variable. Regarding the interplay between the localand large-scale climate in the Antarctic continent, Hosking et al. (2013) investigated the Amundsen/Bellingshausen Sea low (hereafter ASL) using reanalysis data, and constructed diagnostic indices (i.e., the strength and location of the ASL). Also, Hosking et al. (2013) highlighted that the ASL is an important synoptic system modulating the West Antarctic climate variability. In another study, with the aid of reanalysis data, Rondanelli et al. (2019) highlighted the role of tropical variability in connection with the highest temperature recorded on continental Antarctica and associated large melting events over the Antarctic Peninsula.
In addition to surface observations and reanalysis products, a number of regional weather and climate model simulations have been employed over the Antarctic continent, particularly over West Antarctica and the Antarctic Peninsula. These modeling studies mainly consisted of the dynamical downscaling of boundary conditions provided by reanalysis, and covered a broad of spectrum of applications such as surface mass balance analysis (Lenaerts et al., 2012;van Wessem et al., 2014;Agosta et al., 2019), characterizing surface climate patterns and variability Deb et al., 2018), and foehn events (Steinhoff et al., 2014;Elvidge et al., 2015;Bozkurt et al., 2018;Datta et al., 2019;Zou et al., 2019).
Although the aforementioned efforts based on different data sources have helped to improve our understanding of the local-, regional-and large-scale climate variability of the Antarctic Peninsula, there is still a general lack of multiple-data source comparison and evaluation efforts that combine observed, reanalysis and RCM data. This is important for assessing and minimizing uncertainties and possible errors of interpreting the data arising from using a single data source. In particular, analyzing the recent spatiotemporal contrasts of temperature trends over the Antarctic Peninsula using multiple-data sources is crucial for accurately interpreting the climate variability of the region.
The main objective of the present study is, therefore, to investigate recent (1991−2015) near-surface temperature trends of the Antarctic Peninsula by combining observed, reanalysis and RCM data. Given the different climate characteristics of the peninsula on the windward and leeward sides of the cordillera, we first analyze the available near-surface temperature records to demonstrate trend differences on both sides. Then, we use the ECMWF's ERA5, and its predecessor ERA-Interim, for further analysis and comparison. Finally, we use hindcast simulations performed with the Polar-WRF (v3.9.1) RCM forced with ERA-Interim over the Antarctic Peninsula on a nested domain configuration at 45 km and 15 km spatial resolutions for the period 1991−2015. To our knowledge, this is the first complete high-resolution long-term simulation (> 20 years) including all seasons performed with Polar-WRF focusing on the Antarctic Peninsula. In addition, we include hindcast simulations of the KNMI-RACMO21P model forced with ERA-Interim obtained from the CORDEX-Antarctica domain at a spatial resolution of 50 km for further comparison. This allows us to contrast the changes in ERA5 and its predecessor ERA-Interim as well as the comparison of dynamical downscaling simulations with the boundary conditions from ERA-Interim. Section 2 describes the observed data, reanalysis and numerical simulations. Results are presented in section 3. Section 4 summarizes the results and presents concluding remarks.

Meteorological stations
We use four temperature observations located in the cent-ral and northern section of the Antarctic Peninsula (see Fig. 1). Eduardo Frei Montalva Base (Frei station) is the largest Antarctic base of Chile located at Fildes Peninsula near the northern tip of the Antarctic Peninsula. The data is provided by the Chilean National Weather Service (Dirección Meteorológica de Chile, DMC). Another station used in the northern tip of the peninsula is the Argentine Marambio Base. Although only ~250 km away from Frei station, it has a different climate as it is located on the leeward side of the northern peninsula (see section 3.1). In a similar manner, we use two more stations located in the center of the peninsula: the San Martin Base of Argentina on the windward side and the Larsen Ice Shelf station operated by the University of Wisconsin-Madison and the British Antarctic Survey on the leeward side. It should be noted that other weather stations are also available near the San Martin station; namely, Rothera and Faraday/Vernadsky stations. These two stations have already been extensively used in previous studies (e.g., Marshall et al., 2006;van Wessem et al., 2015;Turner et al., 2016); therefore, we use San Martin station, which has received less attention in the literature. On the leeward side, Esperanza station could also be used; however, Marambio station is located on the more leeward side about 100 kilometers southeast of Esperanza station, and is therefore more representative of the leeward conditions over the northern tip of the peninsula. The monthly data from the Marambio, San Martin and Larsen Ice Shelf stations are provided by the Scientific Committee on Antarctic Research (SCAR) Reference Antarctic Data for Environmental Research (READER; Turner et al., 2004) manned stations (San Martin and Marambio) and automatic weather station (Larsen Ice Shelf). Given the difficulties of finding a complete long-term record in the region, we use 1991−2015 as the period for the analysis. This period is also chosen to have a common period consistent with the RCM simulations (see section 2.3). We focus on the annual as well as summer (December−January−February, DJF) and autumn (March−April−May, MAM) time scales, as both large-and local-scale events can cause temperatures to rise above freezing, resulting in surface melting during these seasons (e.g., Nicolas et al., 2017;Bozkurt et al., 2018;Carrasco, 2018;Zou et al., 2019). Note that Larsen Ice Shelf station includes a low percentage of observations between 1990 and 1995 to perform the analysis; therefore, we have omitted the data between those years for this station. For station-based comparisons, temperature fields from gridded products (reanalysis and numerical simulations) are corrected using a constant lapse rate of 0.65°C (100 m) −1 when there is a considerable elevation difference.

Reanalysis
We use monthly near-surface air temperature, mean sea level pressure, 850-hPa specific humidity and wind from the ECMWF's ERA-Interim reanalysis dataset  in order to present recent changes in surface and large-scale circulation patterns. The data assimilation system used to produce ERA-Interim is based on a 2006 release of the IFS (Cy31r2). The system includes a 4D variational analysis with a 12-h analysis window. The ERA-Interim data assimilation and forecast suite produces: (i) four analyses per day, at 0000, 0600, 1200 and 1800 UTC; and (ii) two 10-day forecasts per day, initialized from analyses at 0000 and 1200 UTC (Berrisford et al., 2011). The spatial resolution of the dataset is approximately 80 km (T255 spectral) on 60 vertical levels from the surface up to 0.1 hPa.
In this work, we also include the ERA5 reanalysis, which is the most recent reanalysis product of the ECMWF and an updated version of ERA-Interim that combines large amounts of historical observations into global estimates using advanced modeling systems and data assimilation (C3S, 2017). ERA5 uses a more recent and improved version of the IFS Earth System Model and associated observational assimilation system [Cy41r2; Hersbach and Dee (2016)]. ERA5 has a globally improved spatial and vertical resolution on a 0.28° × 0.28° (~30 km) grid and resolves the atmosphere using 137 levels from the surface up to 0.01 hPa (~80 km). ERA-Interim has recently been replaced by the ERA5 reanalysis. The reanalysis data extend from 1950 to the present, and we use the period 1991−2015 for the analysis. In the same way as ERA-Interim, we use monthly near-surface air temperature, mean sea level pressure, 850-hPa specific humidity and wind components from ERA5. This allows us a multi-comparison of reanalysis products as well as dynamically downscaled simulations versus their boundary conditions (ERA-Interim) and the new ERA5 reanalysis. A summary of the observations and reanalysis products used in this study are given in Table 1.

Regional climate model simulations
We employ the Polar Weather Research and Forecasting Model (Polar-WRF, version 3.9.1) (Hines and Bromwich, 2008;Bromwich et al., 2009;Hines et al., 2011), which is a polar-optimized version of the WRF model (Skamarock et al., 2008). Polar-WRF solves a fully compress-ible non-hydrostatic system of equations on an Arakawa Cgrid in the horizontal, and it includes a terrain-following coordinate system in the vertical. The model includes modified land-surface model sea-ice representation, allowing the specification of variable sea-ice thickness and snow depth over sea ice. These modifications also include optimal values of snow thermal properties and improved heat flux calculations. Time-variable fractional sea ice is represented by separate calls to the surface layer scheme for ice and open water, and the surface heat fluxes are areally averaged to obtain the final values for the fractional sea-ice grid box (Steinhoff et al., 2014).
Polar-WRF is a limited-area model and it requires information on the wind, temperature, geopotential, and relative humidity at the lateral boundaries. In addition, the surface elevation, pressure, sea-ice conditions, and sea surface temperatures also have to be provided. Polar-WRF has been tested over polar ice regions including permanent ice (Hines and Bromwich, 2008;Bromwich et al., 2013b;Deb et al., 2016;Listowski and Lachlan-Cope, 2017), Arctic pack ice (Bromwich et al., 2009), and Arctic land (Hines et al., 2011;Wilson et al., 2012). The model has also been used to produce operational real-time weather forecasts for Antarctica (Powers et al., 2012).
The modeling experiment consists of two nested domains at 0.4° (~45 km) and 0.13° (~15 km) spatial resolutions with a one-way nesting approach on a polar stereographic projection (Fig. 2). The mother domain includes much of western Antarctica and southern South America, and has 118 × 114 grid cells (PWRF-45). The inner domain is centralized on the Antarctic Peninsula and Larsen Ice Shelf, and has 208 × 190 grid cells (PWRF-15). Both domains employ 61 vertical levels between the surface and the model top at 10 hPa. Initial and lateral boundary conditions are provided by ERA-Interim at 6-h intervals with a grid spacing of 0.75° × 0.75°. ERA-Interim (six-hourly, 0.75° × 0.75°) sea surface temperature fields, initial soil parameters (soil water, moisture and temperature) as well as sur- face pressure and skin temperatures are used as surface boundary conditions for the mother domain. The sea-ice data are based on the 25-km resolution Bootstrap dataset (Comiso, 2000). Land-type and topography information for the model are from the default United States Geological Survey landuse data and GTOPO30 elevation data, respectively. Spectral nudging is applied for wind components (u, v), air temperature, specific humidity and geopotential height with a nudging coefficient of 3 × 10 −4 s −1 and wave numbers (3, 3) and (2, 2) for the mother and inner domains, respectively. The choice of spectral nudging parameters is based on previous Polar-WRF simulations performed over West Antarctica (Deb et al., 2016). The simulations are performed on Amazon Web Services−High Performance Computing with an elastic computed cloud instance (c5n.18xlarge) and 360 cores (10 computing nodes of 36 cores each). The simulations are based on a continuous run using restart files of three-year batches starting from 1 January 1989 to 31 December 2015, and the first year of simulations (1989) is used as the spin-up period. Based on the previous Polar-WRF experiments performed by Deb et al. (2016) and Listowski and Lachlan-Cope (2017), as well as a couple of test simulations done with different physical configurations, the Polar-WRF runs are performed using (1) the new version of the rapid radiative transfer model (Iacono et al., 2008) for general circulation models (RRTMG) for both shortwave and longwave radiations; (2) the Morrison double-moment microphysics scheme (Morrison et al., 2009); (3) the Mellor−Yamada− Janjic (MYJ) boundary layer scheme (Janjic, 2002); (4) the Grell−Freitas ensemble cumulus scheme (Grell and Freitas, 2013); and (5) the Noah-MP land-surface model Yang et al., 2011).
In addition to the Polar-WRF simulations, we use the Royal Netherlands Meteorological Institute (KNMI) Regional Atmospheric Climate Model (KNMI-RACM021P; hereafter RACMO) model outputs forced with ERA-Interim for comparisons. RACMO simulations were performed by the KNMI and obtained from the Coordinated Regional Climate Downscaling Experiment (CORDEX; Giorgi et al., 2009) dedicated to the Antarctic domain at 0.44° (~50 km) spatial resolution and 40 vertical levels. The reason for choosing this simulation is merely based on the availability of data and the integrity of the simulations. Given that RACMO simulations end in 2012, we use a common period of 1991−2012 for the comparison of RCM simulations and reanalysis products. More information about the model and its application in polar regions can be found in van Meijgaard et al. (2008) and Lenaerts et al. (2012). Figure 3 shows the mean annual cycle of near-surface temperature for the selected stations on the windward (Fig. 3a) and leeward (Fig. 3b) sides. The mean annual temperature cycle shows that there are differences of around 3°C (for summer) and 10°C to 15°C (for winter) between the windward and leeward stations of the peninsula. The cold- est temperatures are observed at the Larsen Ice Shelf station among the four seasons (e.g., approximately −25°C in July). The temperature contrast between the windward and leeward sides tends to increase in the central parts of the peninsula compared to its northern end. For instance, the mean annual temperature across the peninsula shows a contrast of around ~8°C and ~4°C between both sides at the latitude of San Martin and Marambio stations, respectively (Cook and Vaughan, 2010).   (10 yr) −1 ], which is more pronounced on the leeward side, in agreement with the observed trends. However, in contrast to ERA5, ERA-Interim shows a warming trend (although not statistically significant) in the central-southern coastal windward side (Alexander Island) (Fig. 5b). Unlike the overall cooling trend in summer, both products show the existence of a clear warming in major parts of the peninsula in the autumn season. Particularly, ERA-Interim exhibits a statistically significant warming on the southern windward coasts and central leeward side (Alexander Island and Larsen Ice Shelf region) [approximately +1.5°C (10 yr) −1 ]. This pronounced warming depicted by ERA-Interim appears weakened in ERA5, especially over Alexander Island [+0.6°C (10 yr) −1 to +1.0°C (10 yr) −1 ]. Compared to ERA-Interim, the weaker warming trend in ERA5 exists also over the inland territory of the Antarctic Peninsula, particularly over the northern and central parts. At the annual time scale, the warming on the Larsen Ice Shelf region is notable in both reanalyses [+0.2°C (10 yr) −1 to +0.6°C (10 yr) −1 , mostly non-significant]. A general dipole-like trend pattern over the Antarctic Peninsula (i.e., the windward warm-ing and leeward cooling) exists at the annual time scale, except at the Larsen Ice Shelf. This dipole-like trend is largely confined to the coastal zones of both sides.

Observed temperature
To illustrate the potential role of atmospheric circulation changes on the temperature trend contrasts of the summer and autumn seasons, we compare the summer and autumn trends (1991−2015) in mean sea level pressure and 850-hPa wind components (u, v) from ERA5 in Fig. 6. In general, the most notable change in the summer season is the strengthening of the Weddell Sea low [−2 hPa (10 yr) −1 ] and an anticyclonic trend over the Amundsen Sea (Fig. 6a). In autumn, on the contrary, deepening of the ASL [−4 hPa (10 yr) −1 ] dominates over the West Antarctic sector. In connection with these summer−autumn surface circulation changes, low-level westerlies (850 hPa) tend to be weakened and strengthened over the South Pacific in the summer and autumn seasons, respectively (Fig. 6b). The existence of a dipole-like pattern of sea level pressure trend in the summer season (i.e., windward anticyclonic and leeward cyclonic conditions) is associated with the strengthening of northward (positive) meridional winds over the Antarc- tic Peninsula, indicating the possibility of more advection of cold air from the continent (Fig. 6c). On the other hand, the strengthening of southward (negative) meridional winds in the autumn season could lead to the transport of warmer midlatitude air to the Antarctic Peninsula, particularly to the windward side. Compared to ERA5, the amplified leeward warming observed in ERA-Interim in the autumn season could be associated with a more strengthened ASL [−5 hPa (10 yr) −1 ] and southward winds, and thus moister conditions over the Antarctic Peninsula in ERA-Interim [Figs. S1 and S2 in the electronic supplementary material (ESM)].

Comparison of numerical simulations to observations and reanalyses
A comparison of the recent period (1991−2012) near-surface air temperature and sea level pressure climatology from ERA5, ERA-Interim and numerical simulations is provided in the supplementary material (Fig. S3 in the ESM). Overall, simulations generally capture the temperature and sea level pressure climatology; that is, a relatively mild and humid marine climate on the western coast and a colder continental climate on the east coast.
To illustrate more details of the spatiotemporal differences between the simulations and reanalysis products, we provide the mean annual cycle of near-surface temperature for the windward and leeward sides in Fig. 7. On the windward side, ERA5 and ERA-Interim are very close to each other, with temperatures above 0°C in the summer months and around −6°C in the winter months (Fig. 7a). Dynamically downscaled simulations show a significantly colder annual cycle to those in the boundary conditions (ERA-Interim) and ERA5, particularly in winter months (~2°C dif-ference). On the leeward side, ERA5 indicates colder temperatures compared to ERA-Interim, especially from April to September (Fig. 7b). RACMO reproduces almost the same annual cycle as its boundary conditions (ERA-Interim). Both Polar-WRF simulations exhibit a similar annual cycle, but with much lower temperatures in winter months (approximately −20°C). Some differences in radiative fluxes (i.e., surface downwelling longwave radiation) in Polar-WRF over the leeward side (see Fig. S4 in the ESM) can lead to a more pronounced radiative cooling with either too little cloud or clouds that are optically thin (King et   parisons indicate that both reanalysis products and numerical simulations generally capture the observed annual cycle at each station ( Fig. S5 in the ESM). However, large winter temperature differences between Polar-WRF and RACMO simulations at Marambio station (Fig. S5b in the ESM) could be associated with differences in other simulated surface variables such as wind speed and mean sea level pressure (Fig. S6 in the ESM). Figure 8 compares the maps of summer near-surface air temperature trends (1991−2012) for dynamically downscaled simulations and their boundary conditions (ERA-Interim) as well as ERA5. There is an overall summer cooling over most of the peninsula exhibited by the reanalyses. The warming trend (although not statistically significant) depicted by ERA-Interim (approximately +0.4°C (10 yr) −1 , Fig. 8b] over the central-southern windward coasts (Alexander Island) is mostly absent in ERA5 (Fig. 8a), as also illustrated in Fig. 5a. Numerical simulations reproduce the overall cooling trend and, in contrast to the boundary conditions of ERA-Interim, they show a cooling trend over Alexander Island (Figs. 8c−e). It can be speculated that the coarser local details of the topography and land−atmosphere physics in ERA-Interim might account for the existence of different trends. In addition, unlike the RCMs, there is a strengthening of southward (negative) meridional winds at the surface (i.e., 10 m) in ERA-Interim (Fig. S7 in the ESM). Furthermore, westerlies at 10 m tend to be more strengthened in ERA-Interim (p < 0.05), which might prevent cold-air advection from the continent towards the central-southern windward coasts in ERA-Interim. Over the northern tip of the peninsula, both reanalyses and numerical simulations indicate less cooling [approximately −0.2°C (10 yr) −1 ] compared to the rest of the peninsula, even with some local warming (non-significant) depicted in the reanalyses and Polar-WRF simulations.
The trend map of the autumn season illustrates important differences between the reanalyses and numerical simulations (Fig. 9). Overall, the reanalyses show a warming trend, except on the southern leeward coasts (Figs. 9a and b). On the other hand, the numerical simulations produce a very close trend to each other, exhibiting a marked dipolelike trend pattern over the Antarctic Peninsula (i.e., the wind- The differences in temperature trends between multiple data sources exist in the annual-scale trend map too. For instance, unlike in ERA-Interim and ERA5, the simulations show a clearer pattern of windward warming and leeward cooling (Figs. 10c−e). On the other hand, although the simulations largely agree on the cooling trend over the central and southern leeward coasts, they differ towards the northern tip of the peninsula, particularly on the eastern side. For instance, unlike in RACMO, Polar-WRF simulations show warming trends over the Larsen A and Larsen B embayments (Figs. 10d and e).
The results presented so far have revealed that there is a notable difference between the reanalyses products and numerical simulations in presenting the recent temperature trends on the central windward and leeward coasts. To delve deeper into this finding, we close this section by comparing the reanalyses and numerical simulations with annual time series of near-surface temperature at the San Martin and Larsen Ice Shelf stations on the central windward and leeward slopes, respectively. San Martin station shows a statistically significant warming trend [+0.9°C (10 yr) −1 ] for the 1991−2012 period (Fig. 11a). Both reanalysis products exhibit statistically significant warming trends: +0.67°C (10 yr) −1 and +0.83°C (10 yr) −1 for ERA5 and ERA-Interim, respectively. RACMO and PWRF-45 simulations estimate very similar warming trends that are smaller than the observed trend [+0.23°C (10 yr) −1 and +0.27°C (10 yr) −1 , respectively]. PWRF-15 gives a statistically significant warming trend of +0.45°C (10 yr) −1 . Station-based comparison shows that among the reanalysis products and numerical simu-   lations, PWRF-15 has the largest temporal correlation (r = 0.9) and lowest root-mean-square-difference (1.7°C) for the San Martin station (Table S1). On the leeward side, a marked cooling trend exists for Larsen Ice Shelf station [−1.4°C (10 yr) −1 , p < 0.05] for the 1996−2012 period (Fig.  11b). ERA5 shows a smaller cooling trend for the same period [−0.3°C (10 yr) −1 ], whereas ERA-Interim does not capture the observed annual-scale cooling trend at this station. On the other hand, dynamically downscaled simulations forced with ERA-Interim capture the observed cooling trend at this point, albeit with magnitudes smaller than observed [−0.78°C (10 yr) −1 for RACMO, −0.74°C (10 yr) −1 for PWRF-45, and −0.81°C (10 yr) −1 for PWRF-15]. Polar-WRF simulations exhibit the largest temporal correlations (r = 0.83 for PWRF-45 and r = 0.79 for PWRF-15), and PWRF-15 has the lowest root-mean-square-difference (1.9°C) for the Larsen Ice Shelf station comparison (Table S1 in the ESM).

Summary and concluding remarks
This study investigates the recent (1991−2015) near-surface temperature trends over the Antarctic Peninsula using observations, ECMWF's ERA5 and its predecessor ERA-Interim, and dynamically downscaled RCM simulations forced with ERA-Interim. Given that the peninsula has two distinct regions with different climate characteristics, separated by the Antarctic Peninsula cordillera, the aim was to investigate whether the reanalyses and dynamical downscaling products are able to capture the differences in the observed trends of temperature on the windward and leeward sides. This allowed us to contrast the changes in ERA5 and its predecessor ERA-Interim as well as compare dynamical downscaling simulations with the boundary conditions of ERA-Interim. We first assess the recent observed temperature trends using four stations, namely Frei and San Martin stations (windward), and Marambio and Larsen Ice Shelf stations (leeward). We use hindcast simulations performed with the Polar-WRF RCM forced with ERA-Interim over the Antarctic Peninsula on a nested domain configuration at 45 km (PWRF-45) and 15 km (PWRF-15) spatial resolutions for the period 1991−2015. In addition, we include hindcast simulations of KNMI-RACMO21P (RACMO) obtained from the CORDEX-Antarctica domain at a 50-km spatial resolution for further comparisons.
Observed near-surface temperature trends indicate im- Despite the long-term warming trend, recent studies also show the existence of a regional cooling trend in some parts of Antarctica, including the Antarctic Peninsula, since the late 1990s (Carrasco, 2013;Turner et al., 2016;Oliva et al., 2017). However, this recent cooling period on the peninsula does not yet represent a shift in the overall robust warming trend, and is instead attributed to internal climate variability (Jones et al., 2016;Gonzalez and Fortuny, 2018;Clem et al., 2019;Jones et al., 2019). The persistent windward warming trend in the autumn season as well as at the annual time scale during the recent cooling period could lead to important implications for the fate of ice sheet surfaces on the windward coasts. Indeed, following the general dipole-like trend pattern over the Antarctic Peninsula (i.e., the windward warming and leeward cooling), the simulations indicate a decreasing and increasing trend in sea ice on the windward and leeward coasts, respectively (not shown). This warming and concurrent ice-sheet surface changes observed on the windward coasts are likely to be associated with the recent deepening of the ASL and anomalous northerly warm advection towards the West Antarctic sector and Antarctic Peninsula depicted by the reanalyses. This large-scale forcing mechanism has also been reported in previous studies (e.g., Bromwich et al., 2013a;Raphael et al., 2016;Jones et al., 2019). Jones et al. (2019) further highlighted the linkage between the recent ASL deepening and a positive Southern Annular Mode trend. On the other hand, the reanalyses show that the summer season is characterized by strengthening of the Weddell Sea low as well as an anticyclonic trend over the Amundsen Sea. This synoptic spatial variability is accompanied by northward (positive) meridional winds, which results in increased transport of cold continental air over the Antarctic Peninsula. This is consistent with the work of Turner et al. (2016), who found that more cyclonic conditions in the northern Weddell Sea are associated with the observed cooling trend over the Antarctic Peninsula. Understanding the determinants of the complex interplay between the strengthening phases of the ASL and Weddell Sea low is an intriguing aspect that deserves further investigation. As highlighted by Hosking et al. (2013), a correct representation of the ASL is an important factor in representing West Antarctic surface climate characteristics properly in climate models. In a similar manner, compared to ERA5, the amplified autumn leeward warming detected in ERA-Interim could be associated with a more strengthened ASL, and thus moister conditions over the Antarctic Peninsula, which might eventually trigger more episodic leeward Foehn warming (e.g., Cape et al., 2015;Bozkurt et al., 2018;Datta et al., 2019) in ERA-Interim. The better spatial and temporal resolution of ERA5 compared to ERA-Interim tends to reduce the amplified warming trends detected in ERA-Interim over the central-southern windward and leeward sides of the Antarctic Peninsula. This improvement could be associated with better representation of large-scale forcings (e.g., the ASL) as well as the finer local details of the topography and refined land−atmosphere physics. Very recently, some improvements in the performance of ERA5 over ERA-Interim in representing surface climate characteristics of the Antarctic continent were also reported (Tetzner et al., 2019;Gossart et al., 2019).
Finally, regarding numerical simulations, we further demonstrate the potential added value introduced by the dynamically downscaled simulations. For instance, PWRF-15 exhibits higher temporal correlations and lower rootmean-square-differences with respect to the boundary conditions of ERA-Interim for the San Martin and Larsen Ice Shelf stations. Further station-based comparisons with the coarser resolution simulation (i.e., PWRF-45) also indicate that PWRF-15 shows an overall better performance in representing the spatiotemporal variability of the near-surface air temperature, highlighting the importance of the spatial resolution. As illustrated by van Wessem et al. (2015) and Deb et al. (2016), the improved RCM simulations using higher spatial resolution might be crucially important to achieve a better assessment of surface meteorological variables over complex terrain such as the Antarctic Peninsula, particularly along the coastal sites. For instance, Zhang and Zhang (2018) demonstrated that higher resolution simulations are able to resolve foehn warming, and thus tend to produce larger warming and larger temperature fluctuations on the leeward side of the peninsula, including the Larsen Ice Shelf region. In addition to spatial resolution improvement, more research is warranted to further investigate the impact of model tuning and physics schemes on the surface climate characteristics of the Antarctic Peninsula. We have refrained here from comprehensively analyzing the physical mechanisms of some of the local differences in temperature trends depicted by the reanalyses and RCM simulations. Therefore, further research is also needed to better clarify these mechanisms, at both large and local scales, that can lead to large differences of temperature trends in the multiple-data sources.
Acknowledgements. This work was funded by FONDAP-CONICYT (Grant No. 15110009). D. B. acknowledges support from CONICYT-PAI (Grant No. 77190080). This paper is Contribution Number 1588 of the Byrd Polar and Climate Research Center. The authors acknowledge two anonymous reviewers for their constructive comments that helped to improve the manuscript. DB acknowledges the Scientific Committee on Antarctic Research (SCAR) Expert Group on Operation Meteorology in the Antarctic (OPMet) for a partial funding award for the 14th Workshop on Antarctic Meteorology and Climate (WAMC) as well as the Year of Polar Prediction in the Southern Hemisphere (YOPP-SH) meeting in Charleston, SC, USA, between 25 and 28 June 2019. We thank David B. REUSCH (Department of Earth and Environmental Science, New Mexico Technology), Rodrigo Delgado URZÚA (Dirección General de Aeronáutica Civil, Chile), Kevin MAN-NING (National Center for Atmospheric Research, Boulder, Colorado), Andrew ORR (British Antarctic Survey) and Pranab DEB (Indian Institute of Technology) for useful discussions on the Polar-WRF simulations. We are grateful for data from the SCAR-READER dataset and we wish to acknowledge ECMWF for ERA-Interim and ERA5 data. The Polar-WRF simulations were per-formed within a project entitled "Simulaciones climáticas regionales para el continente Antártico y territorio insular Chileno" funded by the Chilean Ministry of Environment. This research was partially supported by the Basal Grant AFB 170001 and the supercomputing infrastructure of the NLHPC (ECM-02:Powered@ NLHPC). The authors appreciate the support of Amazon Web Services (AWS) for the grants PS_R_FY2019_Q1_CR2 & PS_R_ FY2019_Q2_CR2, which allowed us to execute the Polar-WRF simulations on the AWS cloud infrastructure. We thank Francisca MUÑOZ, Nancy VALDEBENITO and Mirko DEL HOYO at CR2 for post-processing of Polar-WRF simulations.
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