The U.S. Department of Energy Atmospheric Radiation Measurement (ARM) West Antarctic Radiation Experiment (AWARE) performed comprehensive meteorological and aerosol measurements and ground-based atmospheric remote sensing at two Antarctic stations using the most advanced instrumentation available. A suite of cloud research radars, lidars, spectral and broadband radiometers, aerosol chemical and microphysical sampling equipment, and meteorological instrumentation was deployed at McMurdo Station on Ross Island from December 2015 through December 2016. A smaller suite of radiometers and meteorological equipment, including radiosondes optimized for surface energy budget measurement, was deployed on the West Antarctic Ice Sheet between 4 December 2015 and 17 January 2016. AWARE provided Antarctic atmospheric data comparable to several well-instrumented high Arctic sites that have operated for many years and that reveal numerous contrasts with the Arctic in aerosol and cloud microphysical properties. These include persistent differences in liquid cloud occurrence, cloud height, and cloud thickness. Antarctic aerosol properties are also quite different from the Arctic in both seasonal cycle and composition, due to the continent’s isolation from lower latitudes by Southern Ocean storm tracks. Antarctic aerosol number and mass concentrations are not only non-negligible but perhaps play a more important role than previously recognized because of the higher sensitivities of clouds at the very low concentrations caused by the large-scale dynamical isolation. Antarctic aerosol chemical composition, particularly organic components, has implications for local cloud microphysics. The AWARE dataset, fully available online in the ARM Program data archive, offers numerous case studies for unique and rigorous evaluation of mixed-phase cloud parameterization in climate models.
West Antarctica is one of the most rapidly warming regions on Earth, and this warming is closely connected with global sea level rise. The discovery of rapid climate change on the West Antarctic Ice Sheet (WAIS) has challenged previous explanations of Antarctic climate change that focused on strengthening of circumpolar westerlies in response to the positive polarity trend in the southern annular mode (Bromwich et al. 2013; Nicolas and Bromwich 2014). West Antarctic warming trends do not yet have a comprehensive explanation. Dynamical mechanisms may vary from one season to the next, and these mechanisms very likely involve complex teleconnections with subtropical and tropical latitudes (e.g., Ding et al. 2011; Schneider et al. 2012). Field work for atmospheric and climate science has historically been sparse due to logistical challenges (Bromwich et al. 2012), especially for West Antarctica, where the areas of greatest interest for sea level rise are very distant from the major or permanent field stations of any nation’s Antarctic program. Direct meteorological information on the WAIS has mostly been limited to a few automatic weather stations (AWS) for several decades (Lazzara et al. 2012). And yet satellite imagery, measurements, and meteorological reanalyses indicate that West Antarctica is highly susceptible to advection of warm and moist maritime air, with related cloud cover, depending on the location and strength of low pressure centers in the Amundsen, Ross, and Bellingshausen Seas (Jolly et al. 2018; Nicolas and Bromwich 2011). At the same time, satellite profiling, even with active sensors, often misses important details regarding clouds and precipitation in the Antarctic lower troposphere (e.g., Maahn et al. 2014), and this further emphasizes the need for comprehensive surface-based measurements. Recently, Scott et al. (2019) have linked surface melting conditions on the WAIS to blocking activity in the Amundsen Sea region and to a negative phase of the southern annular mode, both of which correlate with El Niño conditions in the tropical Pacific Ocean. There is a need to quantify the role of these changing air masses on the surface energy balance (SEB), including all surface energy components and cloud radiative forcing (e.g., Bromwich et al. 2012; Trenberth and Fasullo 2010; Hyder et al. 2018; Silber et al. 2019a). More generally, global climate model simulations are known to perform poorly over the Antarctic and Southern Ocean (e.g., Trenberth and Fasullo 2010; Hyder et al. 2018), and the relative scarcity of cloud information at southern high latitudes has so far inhibited progress.
Surface melt conditions during summer are increasingly realized to have a potentially important role in WAIS mass loss. Analysis of satellite and aerial photographic observations by Kingslake et al. (2017) reveals how extensively and frequently surface melt conditions can occur throughout lower-elevation regions of Antarctica. The largest immediate cause of ice sheet acceleration in West Antarctica is recognized to be ice shelf thinning via basal melting from a warming ocean (Pritchard et al. 2012; Paolo et al. 2015). Concurrent with this ocean-induced ice shelf loss is retreat of the grounding line (the transition between the ice sheet and floating ice shelf) throughout West Antarctica (Rignot et al. 2014). Once stabilization by ice shelf buttressing is lost (Fürst et al. 2016), ice sheet acceleration in West Antarctica is potentially rapid due to the underlying topography that slopes downward as one goes inland. This is the well-known marine ice sheet instability (MISI; Weertman 1974; Oppenheimer 1998; Alley et al. 2015). A MISI-related collapse may have already started for the Thwaites Glacier basin (Joughin et al. 2014).
However, the major role of oceanic warming in West Antarctica does not signify that direct atmospheric warming is a negligible factor. Pollard et al. (2015) and DeConto and Pollard (2016) have identified a marine ice cliff instability (MICI) that operates in conjunction with the MISI. When surface air temperatures approach and exceed freezing, surface meltwater filtering into crevasses can induce hydrofracturing near the grounding line, weakening the grounded ice column at its edge and increasing the calving rate (see also Bassis and Jacobs 2013). Hydrofracturing will also occur on the ice shelves themselves, further increasing their loss rate and exposing these unstable ice cliffs at the grounding line (DeConto and Pollard 2016). The three overarching processes in cryosphere mass loss are direct melt runoff, glacier and ice sheet calving, and ice shelf ablation through basal melting. The difference between the net of these processes and accumulation defines the mass balance of the cryosphere (Zwally et al. 2005). These three processes are also interrelated. For example, on grounded ice sheets, meltwater can accelerate ice sheet motion and calving by 1) filtering down to the base of the ice sheet and lubricating its downslope motion and 2) hydrofracturing, in which surface meltwater ponds and infiltrates crevasses, acting as a slow-motion “jackhammer” that weakens an ice shelf structure (e.g., Scambos et al. 2000).
All three of these processes play important roles in Greenland (e.g., Fürst et al. 2015). In Antarctica, we are mainly concerned about the stability of systems of moving ice sheets partially buttressed by their adjacent and attached floating ice shelves. Fürst et al. (2016) demonstrate that ice shelf buttressing plays a critical role in the stability of ice sheets adjacent to the Amundsen and Bellingshausen Seas. Moreover, the recent work of Pollard et al. (2015) and DeConto and Pollard (2016) indicates an important role for direct atmospheric forcing on ice shelf hydrofracturing in West Antarctica. Parameterizations for ice shelf hydrofracturing and the MICI in coupled climate models are still in their early stages; actual field data are required for model testing and refinement, and for attribution of surface melting events to specific atmospheric processes such as warm air intrusion (Nicolas and Bromwich 2011; Scott et al. 2019), cloud all-wave surface radiation enhancement (Bennartz et al. 2013; Hu et al. 2019), or foehn winds (e.g., Elvidge et al. 2015; Zou et al. 2019).
AWARE is an effort to acquire critical atmospheric data to fundamentally understand atmospheric forcing on West Antarctica, and to foster related improvements to climate model performance. Within the past two decades other regions of the Antarctic continent have seen several field campaigns and growing permanent installations of advanced atmospheric science equipment, all of which are providing new insights into the continent’s unique meteorology and climatology. Two of the most persistent efforts have occurred on the high plateau of East Antarctica: 1) at the South Pole with Fourier transform infrared (FTIR) spectroradiometer measurements (e.g., Walden et al. 2006; Town et al. 2007), and micropulse lidar (MPL) combined with tethered balloon cloud microphysical observations (Lawson and Gettelman 2014), and 2) multisensor observations of ice clouds over Dome C that include multispectral microwave radiometry (Ricaud et al. 2017). Research radars for cloud and precipitation recently deployed at Dumont d’Urville Station in Adélie Land have revealed how katabatic outflows sublimate precipitation, thus impacting the long-term ice mass balance (Grazioli et al. 2017). A climate observatory has been established at Princess Elizabeth Base in Queen Maud Land, East Antarctica, that presently maintains a precipitation radar along with comprehensive meteorological measurements whose combined data enable studies of both cloud microphysics and surface mass balance (Gorodetskaya et al. 2015). The British Antarctic Survey’s Rothera Station, in the southern Antarctic Peninsula region, serves as a base for aircraft-based in situ cloud microphysical observations that have revealed details about warm-temperature secondary ice production in Antarctic clouds (Lachlan-Cope et al. 2016). West Antarctica, due to its extreme remoteness, has yet to see a permanent installation of atmospheric or climate science instrumentation beyond AWS (Lazzara et al. 2012), but the AWARE campaign has made a start. Figure 1 shows the location of the two AWARE deployments. Within the entire sector of Antarctica shown in this figure, only four locations (indicated by red markers) have seen atmospheric and climate science experiments using modern instrumentation with multiple sensors: McMurdo Station and its immediate surroundings on and near the western Ross Ice Shelf (RIS), South Pole Station, WAIS Divide Ice Camp, and Rothera Station.
This report on the AWARE campaign is organized with three scientific motivations. The first is to illustrate contrasts between the Antarctic and the relatively better-observed Arctic. The high Arctic is a partially frozen ocean surrounded by continental landmasses, with one major ice sheet (Greenland) contributing to sea level rise. The Arctic radiation budget is strongly influenced by persistent and long-lived mixed-phase clouds (e.g., Morrison et al. 2012; Bennartz et al. 2013). High southern latitudes are characterized by a continent with greatly varying topography at high elevations surrounded by the world’s most turbulent ocean. The SEB at the vulnerable extremities of Antarctic ice sheets is influenced on one hand by katabatic and topographic influences on atmospheric dynamics and cloud physics, and on the other hand by adjacent Southern Ocean storm tracks (Nicolas and Bromwich 2011) that are in turn influenced by teleconnections with lower latitudes. The more varied influences on Antarctic clouds often yield markedly different manifestations of mixed-phase cloud microphysics than seen in the Arctic (Scott and Lubin 2016).
A second motivation is the need to keep aerosol chemistry and microphysics on an equal footing with meteorology and cloud microphysics. The study of aerosol–cloud interaction has become inseparable from any thorough and current study of mixed-phase cloud life cycle, and our presentation of contrasts between the Antarctic and the Arctic must necessarily include aerosol climatology. Finally, we demonstrate how AWARE data from West Antarctica can be used to evaluate performance of both regional and climate models, in the region where atmospheric warming is expected to exacerbate ice shelf loss and Antarctic contribution to sea level rise.
AWARE deployed the second ARM Mobile Facility (AMF) to McMurdo Station on Ross Island, Antarctica, to sample an annual cycle in atmospheric structure and thermodynamics, surface radiation budget and cloud properties. The ARM Mobile Facility deployments began in 2005 in response to the substantial success that the three fixed ARM sites realized for gathering advanced atmospheric sensor data for climate model development and validation (Mather and Voyles 2013). The AMFs consist of cloud research radars, lidars, multiple broadband and spectral radiometers, an aerosol observation suite, and thorough meteorological sampling ranging from surface turbulent flux equipment to radiosondes. The AMFs are intended to address key issues in atmospheric science by deploying the entire multisensor suite to a given location for at least several months of data collection, thereby making a substantial advance in the field.
In October 2013 the AWARE campaign, organized by researchers from the Scripps Institution of Oceanography (SIO), Byrd Polar and Climate Research Center (BPCRC), The Pennsylvania State University, and Brookhaven National Laboratory (BNL), was awarded the use of the second Mobile Facility (AMF2) to address the current concerns related to Antarctic climatic warming discussed above. Transportation, construction and power requirements of an AMF necessitated the choice of McMurdo Station as the site for the full AMF deployment. At the same time, the ARM Program recognized the value in collecting data directly from West Antarctica, and the AWARE campaign was fortunate to be awarded a second and smaller suite of instruments optimized for SEB measurement for deployment at one of the summer-only field stations in West Antarctica.
McMurdo Station (77°50΄47˝S, 166°40΄6˝E) is generally a challenging location for meteorological and aerosol sampling because of complex terrain variability and related microclimates including rapidly shifting wind direction. The CosRay location 1 km from McMurdo (Fig. 2) provided the research radars with a clear view across an open fetch of water in southeasterly through southwesterly directions, which are the prevailing wind directions. The WAIS Divide Ice Camp (WAIS Divide; 79°28΄03˝S, 112°05΄11˝W; elevation: 1797 m) was chosen as the most logistically suitable station for the SEB measurement suite, based on power and transportation constraints. The U.S. Antarctic Program (USAP) allocated the AWARE campaign’s extended facility component (Fig. 1) one LC-130 aircraft mission to transport to WAIS Divide all personnel and equipment, including laboratory housing (half-size sea container) and helium for radiosondes. The extremely flat and even terrain at WAIS Divide offered an ideal site for radiometry and SEB measurement, with the largest instrumental challenge being optical obstruction and occasional instrument fouling during extended periods of strong winds and blowing snow. Figure 3 shows the sea container installation at WAIS Divide. Table 1 lists the AMF2 instruments at CosRay and Table 2 lists the instruments deployed to WAIS Divide. These tables also provide the instrument acronyms used in the text. At McMurdo Station the AMF2 began full operation on 1 December 2015, with some instruments operating earlier, and continued through 31 December 2016. At WAIS Divide, the AWARE instruments began operation with sondes on 4 December 2015, with all instruments operating by 7 December and continuing until 17 January 2016.
In the following sections we demonstrate how climatological information on cloud properties is derived from the AMF2 measurements, and we discuss contrasts with cloud properties obtained from Arctic locations with nearly identical instrumentation. We also discuss AMF2 case studies suitable for model evaluation, again contrasting AWARE retrievals from their Arctic counterparts. We then illustrate how the WAIS Divide dataset can be used as a case study for both regional and global climate model evaluation regarding cloud microphysics. At WAIS Divide AWARE was fortunate to sample the edge of a surface melt event that spanned a third of West Antarctica and most of the RIS and lasted from 10 to 18 January 2016 at WAIS Divide (Nicolas et al. 2017). The rapid transition between climatologically typical summer conditions and the much warmer conditions of the melt onset represents a step function that provides a stringent test of microphysical parameterization performance in response to the changing model input fields (e.g., Wilson et al. 2018).
Preliminary instrumental results and Arctic comparison
Silber et al. (2018a,b, 2019a) have developed a multisensor approach to determine key climatological cloud properties from high-latitude ARM data, including occurrence fraction, cloud persistence and boundaries, and cloud location relative to temperature and moisture inversions. In the application of this approach at McMurdo, Ka-band ARM zenith radar (KAZR) data from both general and moderate sensitivity operating modes are used for hydrometeor detection throughout the troposphere, similar to Clothiaux et al. (2001), and these detections are gridded to the High Spectral Resolution Lidar (HSRL) 7.5-m vertical resolution and 30-s time sampling. HSRL data are then used to refine the cloud detection process by analyzing the log-scaled particulate backscatter cross section βp as a function of the linear depolarization ratio (LDR). Different regions in the scatter diagram of βp versus LDR correspond to liquid water droplets, cloud ice particles, or aerosol particles, and the observational occurrence in each of these regions provides climatological information as a function of altitude.
The multisensor approach used here is optimized for polar regions. The liquid water cloud-base-height algorithm in Silber et al. (2018b) differs from earlier ARM retrievals in that it is optimized for detection of a polar cloud base, as opposed to any cloud base (e.g., as in ceilometer algorithms). This algorithm uses the backscatter cross section’s first and second derivatives to accurately determine the cloud base height. The hydrometeor detection algorithm described in Silber et al. (2018a, 2019a) using lidar is based on identifying local minima in monthly histograms of backscatter versus LDR, such that no fixed backscatter and/or LDR thresholds for liquid or ice are used, but instead, adaptive-dependent thresholds may vary in time, thereby reducing error in phase classification. Hydrometeor detection using KAZR as describe in Silber et al. (2018a) is based on a signal-to-noise ratio (SNR) threshold but is otherwise not significantly different than earlier ARM retrieval methods.
This multisensor approach is applied here to both McMurdo AMF2 and ARM North Slope of Alaska (NSA) data, with climatological contrasts demonstrated in Figs. 4–7. The NSA site is located at Utqiaġvik (71.3°N, 156.8°W; formerly referred to as Barrow, Alaska), adjacent to the Beaufort Sea, and is representative of an Arctic maritime location with variable sea ice concentration. Instrumentation at the NSA site is very similar to the AMF2 deployed at McMurdo, and the ARM data reduction and quality-control pipeline is identical for the two sites (Peppler et al. 2008). The NSA data analysis presented here is based on measurements from 2015, which correspond with previous analyses of longer datasets from this site (e.g., Shupe 2011).
Figure 4 shows 30-day running-mean total hydrometeor and liquid-cloud occurrence fractions at McMurdo and NSA over an annual cycle. The total duration is 721 h, and an odd hour number was required for the smoothing to center the data properly, hence the indication of plus 1 h in the caption. The temperature curve, based on radiosonde profiles, represents the average temperature between the surface and 4-km altitude. We see that the annual hydrometeor (liquid) occurrence fraction is higher by ∼20% (∼31%) at NSA relative to McMurdo. Figure 5 shows seasonal averages of cloud thickness, highest cloud-top height and highest cloud-top temperature. Here the highest cloud-top height is the highest bin with any detected hydrometeor using the combined HSRL and KAZR method of Silber et al. (2018b), and the highest cloud-top temperature is the corresponding temperature computed from the sonde data linearly interpolated in time. Most clouds are thicker at McMurdo relative to NSA, but the deepest, likely frontal, clouds are observed at NSA. The annual highest cloud-top heights are more variable at NSA but generally comparable at both sites (both having elevation close to sea level), while the highest cloud-top temperatures are mostly lower and less variable at McMurdo.
Figure 6 provides similar seasonal averages of total cloud and liquid-bearing layer persistence. Liquid-cloud layers are significantly more persistent at NSA than McMurdo, a result likely influenced by 1) the complex topography and lack of significant moisture sources at McMurdo relative to NSA (Monaghan et al. 2005), and 2) synoptic flow and advection being different for the two sites. While the longest-lived layers are observed in summer at NSA, McMurdo exhibits different seasonal behavior (depending on the examined percentile). Figure 7 illustrates the seasonal variability of the lowest liquid-bearing cloud layer base height, as well as its annual cumulative distribution function. The lowest liquid-bearing cloud layers are significantly higher at McMurdo relative to NSA, but liquid is detected at higher altitudes at NSA, due to typically warmer temperatures in the atmospheric profile (Fig. 5). These cloud layers are evenly distributed up to ∼3 km at McMurdo while over NSA, they are mostly concentrated near the surface.
Statistical significance of the comparisons between McMurdo and Utqiaġvik in Figs. 4–7 was assessed using a two-sample Kolmogorov–Smirnov test at the 95% confidence level, to determine if the samples represent different variable distributions. The distributions were found to be different at this confidence level for all retrievals in Figs. 4, 5, and 7, and for liquid water clouds during spring in Fig. 6.
The distribution of aerosol particles in the Antarctic is characterized by its unique location and surrounding ocean (which largely isolates it from the sources present on other continents), its near-complete coverage by ice and snow (which eliminates most local non-sea-salt-dust and terrestrial biological particle sources), and its near-absence of human activities (which minimizes the emissions from combustion, cooking, and other human activities). The lack of orographic features in the Southern Ocean surrounding Antarctica supports the midlatitude westerlies, effectively defying substantial transport of continental emissions into the Antarctic region. The result is that aerosol concentrations reflect the seasonal trends of ocean phytoplankton (non-sea-salt sulfate), seabirds (organic mass), wind-driven sea spray (salt), and non–sea salt dust, as is shown in Fig. 8b.
The OM concentration is highest in summer during AWARE, when seabird activity is also high. The breakdown products of urea deposits from seabirds result in a variety of organic products in the vapor phase (Legrand et al. 2012), some of which condense and, along with ammonia (Legrand et al. 1998), contribute to particle-phase ammonium and OM. Of course human activities at McMurdo Station, while minimal compared to those of urban regions, also contribute OM, but in the summer that accounts for less than half of the observed OM (Fig. 3 of Liu et al. 2018). Some OM may also be associated with the submicron salt from sea spray, but the FTIR spectroscopy spectra are more consistent with seabird sources (Schmale et al. 2013) and the seasonal trend of OM concentration is not consistent with an association with salt from sea spray (Liu et al. 2018). Even though the non–sea salt sulfate concentration tracks the OM closely, the strong summertime signature is likely attributable nearly entirely to a different source, namely, the production of DMS by ocean phytoplankton and subsequent oxidation to form non–sea salt sulfate. Submicron non–sea salt dust mass concentration is also highest in summer, likely as a result of both increased human activities and more exposed soil. During AWARE, the salt mass concentration is very small, with seasonal means and medians from 0.02 to 0.11 µg m‒3 and maximum weekly values below 0.2 µg m‒3 in winter. This cycle is driven by the local upwind wind speeds at the sea surface as well as the additional contributions of wind-driven frost flowers on new sea ice in winter (Liu et al. 2018).
In Fig. 9 we present data from two Arctic sites for comparison with AWARE. Figure 10 provides seasonal statistics comparing Utqiaġvik with AWARE. At the Alert Observatory (82.45°N, 62.51°W; Leaitch et al. 2018), the contributions from organic functional groups to the Arctic submicron aerosol were measured using 126 weekly integrated samples collected from April 2012 to October 2014. Routine outdoor high-volume samples of total suspended particles have been collected at Alert for inorganic chemical composition since 1980 (e.g., Barrie and Hoff 1985), and submicron sampling for inorganic ion analysis was started in March 2011. As a special study, weekly collections of particles smaller than 1 µm on Teflon filters were collected for FTIR spectroscopy of organic functional groups (OFG) from April 2012 to October 2014.
At Alert the cycle in salt mass concentration is similar to that of AWARE, with as much as 0.5 µg m‒3 in winter and below 0.1 µg m‒3 in summer (Fig. 9). At NSA the winter concentrations are higher with a mean of 1 and weekly averaged values of up to 2 µg m‒3, consistent with the closer proximity to seasonal new sea ice associated with higher frost flower frequency (Shaw et al. 2010; Xu et al. 2013, 2016). The evidence for Na depletion relative to Cl supports a wintertime contribution from frost flowers during AWARE (Liu et al. 2018), since the higher freezing temperature of Na salts relative to Cl salts indicates the role of wicking from brine pools in particle formation.
In contrast, the highest non–sea salt sulfate and organic mass concentrations in the annual cycles in the Arctic at both NSA and Alert show the well-known springtime haze that results from transport from the northern midlatitudes, as illustrated in Fig. 9 (Shaw 1982; Law and Stohl 2007; Quinn et al. 2007). The overall low concentrations of submicron mass concentration are otherwise a common feature of the Arctic and Antarctic. The Utqiaġvik sulfate mass concentration means and medians in winter and spring exceed those of summer and autumn by more than a factor of 2, obscuring any smaller differences that could be present for biological sources of non–sea salt sulfate between summer and winter seasons. Another interesting difference is the relative amount of non–sea salt sulfate to organic mass, which is nearly 1:1 in summer at AWARE and NSA, but it exceeds 2:1 at Alert, especially in early spring. Summer sulfate (and OM) at Alert, after June, is primarily biological with some transient contributions from biomass burning (BB). Utqiaġvik is likely similar, but has a larger contribution to OM from BB during the summer, giving the smaller SO4/OM value. In spring (and winter), both sites experience transport from Eurasia with Utqiaġvik seeing a little more from Southeast Asia (e.g., Xu et al. 2017). OM relative to sulfate is similar at both sites.
The higher organic and non–sea salt sulfate mass concentration in summer in Antarctica is coincident with higher concentrations of CCN at supersaturations of 0.1% and 1% (Fig. 8a). This correlation means that the biogenic non–sea salt sulfate and organic sources may well both contribute significantly to summertime CCN concentrations, as they do in the Arctic (Abbatt et al. 2019). The relationship between biogenic non–sea salt sulfate and organic means that both can have an effect on cloud droplet number concentrations, potentially increasing cloud drop effective radius and shortwave reflection.
Examples of representative individual cases.
Following these climatological comparisons, we now discuss some representative individual cases that illustrate the potential for evaluating climate model simulations with nearly identical multisensor datasets from both the Antarctic and the Arctic. AWARE obtained the first ever triple-wavelength radar observations of ice and mixed-phase clouds over Antarctica. These observations point to a new paradigm in unraveling ice microphysics processes at high latitudes. When observing ice particles with a single-wavelength radar in the “Rayleigh regime” (i.e., when the wavelength is large compared to the size of the ice particles), the radar reflectivity Z is proportional to the square of the particle masses m(D) integrated over the particle size distribution (PSD) but it is more intricately related to other moments of the PSD, for example the cloud ice water content (IWC) or the ice mass flux, which are indeed the most relevant for microphysical studies. When the wavelength of the radars becomes comparable to the size of the particles being probed (“non-Rayleigh” regime) the measured reflectivity decreases sometimes by more than 10 dB relative to the Rayleigh reference (Matrosov 1998; Kneifel et al. 2011, 2015). The main reason for this decrease is that interferences (usually destructive) of the incident wave and reflected waves from different parts of the particle cause the backscattered energy to be smaller than for pure Rayleigh scatterers.
Dual-wavelength reflectivity ratios (DWR) are then indicative of a characteristic size of the PSD such as mass median diameter (Matrosov 1998; Kneifel et al. 2011). Depending on the radar wavelength pair, they are particularly effective within specific particle size ranges. For example, the Ka–W frequency pair is effective for a particle size range between 0.5 and 3 mm, whereas to cause a difference at X–Ka frequencies the particle size has to exceed sizes of ∼8 mm. When more than two frequencies are considered not only can the characteristic size of the ice PSD be derived for broader size ranges but also information on bulk density can be gleaned (Kulie et al. 2014; Leinonen and Moisseev 2015; Kneifel et al. 2015; Stein et al. 2015), which better constrains the ice microphysics.
Figure 11 shows a two-dimensional histogram of the data collected at McMurdo during 10 January 2016 from the X–Ka- and W-band ARM radars. While most of the data are concentrated around the origin (0 dB, 0 dB), thereby corresponding to small ice crystals that produce the same reflectivities at all frequencies, histogram bins with large DWRs signal the presence of larger ice crystals. Following the rationale proposed by Kneifel et al. (2015) the three different branches indicated by the continuous, dotted and dashed lines correspond to different growth mechanisms. For example, the typical hook signature (continuous line) is likely associated with low-density aggregates, while the points with large Ka–W and small X–Ka DWR (dashed line) are linked to denser and more spherical particles. Retrieval methodologies focused at using this information in a quantitative way are currently under study (Leinonen et al. 2018; Chase et al. 2018; Mason et al. 2018; Tridon et al. 2019; Battaglia et al. 2020). Surprisingly, the strength of the observed multifrequency radar signatures are overall in a similar range (both DWRs exceeding 10 dB) as observed during the deployment of the AMF2 at the Biogenic Aerosols–Effects on Clouds and Climate (BAECC; Petäjä et al. 2016) campaign in Finland (Kneifel et al. 2015). The unexpected strong multifrequency radar signatures revealed during AWARE indicate that growth processes such as aggregation and riming play an important role in the processes related to snowfall production in Antarctica—at least in areas with sufficient supply of moisture such as close to the coast.
ARM’s extensive multispectral capabilities deployed at McMurdo Station offer the ability to construct specific case studies for model evaluation (e.g., Silber et al. 2019b), as has been done with several Arctic field campaigns (e.g., Fridlind et al. 2007; Verlinde et al. 2007; McFarqhuar et al. 2011; Fridlind and Ackerman 2018). Here we demonstrate some AWARE ground-based remote sensing retrievals and contrasting Arctic cases from NSA. Figure 12 shows two representative examples of mixed-phase clouds observed at McMurdo and at the ARM NSA Utqiaġvik site as detected by the HSRL at visible wavelengths (532 nm) and the KAZR at millimeter wavelengths (∼8.5 mm). As the two instruments operate at wavelengths that differ by four orders of magnitude, their measurements are sensitive to different aspects of the cloud. The lidar is more sensitive than radar to small particles with high number concentrations such as liquid droplets, as seen at the top of the cloud by a region of strong backscatter (Figs. 12a,b) and a low depolarization ratio indicating spherical droplets (Figs. 12c,d). Ice particles form in the layer of supercooled liquid water that precipitate from its base. This is seen as significantly nonzero lidar depolarization ratios indicating nonspherical particles (Figs. 12c,d) that are large enough to strongly reflect energy at the significantly longer radar wavelengths (Figs. 12e,f). The mixed-phase clouds shown are representative in that the clouds at Utqiaġvik tend to form in the boundary layer with the ice virga often reaching the surface, while the McMurdo clouds tend to form above the boundary layer; the latter probably being related to the strong katabatic flow and other topographic effects (see Fig. 7; see also Silber et al. 2018a; Zhang et al. 2019).
Retrievals from the Atmospheric Emitted Radiance Interferometer (AERI) provide an important complement to the HSRL and radar measurements. The magnitude and spectral shape of the downwelling longwave radiance measured by the AERI from 8 to 25 µm is sensitive to cloud temperature, optical depth, thermodynamic phase, and particle effective radius. Cloud properties retrieved from AERI measurements using the Cloud and Atmospheric Radiation Retrieval Algorithm (CLARRA; Rowe et al. 2019) are shown in Figs. 11g–n.
The full year of measurements at McMurdo allows comparison of Arctic and Antarctic clouds over a full seasonal cycle. As an example, Fig. 12 compares Arctic and Antarctic clouds for two time periods. The dates were chosen such that temperatures are similar at the cloud heights (–30° to –20°C) and where supercooled cloud liquid water can exist. Although surface temperatures differed markedly for these two cases, four other cases were also considered for which surface temperatures were similar between locations (8 and 13 March 2016 at McMurdo, and 5 November 2014 and 20 January 2016 at Utqiaġvik; not shown). For all cases, the optical depth of liquid is higher than for ice (Figs. 12g,h) and variations in optical depth, liquid effective radius, and liquid water path are typically correlated with each other. However, differences are apparent in clouds between the two locations. At McMurdo clouds are higher (Figs. 12a–f) and optically thinner overall (Figs. 12g,h), and liquid droplets typically have smaller effective radii (Figs. 12i,j) for these cases. Similar contrasts were also found between the two locations for the other case examined. For example, the liquid effective radii at Utqiaġvik was found to be typically between 4 and 10 µm, in keeping with previous measurements in the Arctic (e.g., Cox et al. 2014), whereas at McMurdo it was typically below 5 µm. The latter is consistent with Zhang et al. (2019), who find similar small values for McMurdo using active-sensor techniques described in Snider et al. (2017). Work is in progress to retrieve and compare cloud microphysical properties including liquid and ice optical depths and effective particle sizes over a full year.
Climate modeling applications
The AWARE campaign’s first major result came from WAIS Divide, when the sea container equipment recorded atmospheric and SEB fluxes at the edge of a major West Antarctic melt event (Nicolas et al. 2017). This melt event was associated with a strong El Niño year. The onset of the melt event on 10 January was accompanied by an abrupt temperature increase at WAIS Divide (Fig. 13). The immediate cause of this melt event was an amplified high pressure ridge (“blocking high”) over the 90°–120°W sector of the Southern Ocean. By creating a prominent dent in the circumpolar westerly flow, this ridge generated a strong north–south advection of warm marine air toward West Antarctica. The ridge was strongest during 10–13 January 2016 but persisted through 20 January, maintaining warm conditions favorable to surface melt in the sector West Antarctica adjacent to the RIS. Positive sea surface temperature anomalies of >2°C near 50°S, 120°W provided additional heat to the air traveling south. The unusual extent and duration make the melt event one of the greatest observed in the RIS since the beginning of the satellite record in 1978 (Nicolas et al. 2017). The SEB evolution was derived from nearly all the AWARE instruments at WAIS Divide and is described in Nicolas et al. (2017). The “step function” in temperature and moisture throughout the lower troposphere that occurred around 10 January, captured by AWARE instruments, provides a unique case study for both regional and global climate models.
In Fig. 13 we show an evaluation of the Polar Weather Research and Forecasting regional model (PWRF), which is a version of the Weather Research and Forecasting (WRF) Model (Skamarock et al. 2008) adapted for high latitudes (e.g., Hines and Bromwich 2017); this comparison complements the comprehensive investigation by Hines et al. (2019) of the WAIS Divide warming using PWRF simulations. Here PWRF uses a double-moment cloud microphysics scheme (Morrison et al. 2005), and is initialized in the first simulation using ERA-Interim (PWRF-EI; Dee et al. 2011) and then in the second using analysis data from the NOAA Global Forecast System (GFS; PWRF-FNL). Figure 12 focuses on the transition period 8–13 January 2016 when the step function in tropospheric temperature and moisture occurred. We first consider the precipitable water vapor (PWV), comparing both simulations against observations from the AWARE MWR retrievals. These WAIS Divide radiosonde data, used to derive the MWR PWV retrievals, were not contributed to the Global Telecommunication System (GTS) that feeds information into data assimilation for global meteorological reanalyses; and therefore we have an independent assessment of model performance at a completely data-sparse location. Both simulations capture much of the observed time evolution of this field, but there are key differences late on 10 January and throughout 11–12 January.
The PWV from the analysis/reanalysis should have a strong impact on the produced cloud liquid water in mesoscale simulations, and this is seen in the time evolution of cloud liquid water path (LWP). Observations show relatively high occurrence of liquid water on 9–10 January, and the simulations failed to capture this. The analyzed water vapor field may contribute to the error. The ERA-Interim simulation does a better job of capturing the liquid water early on the 11 January. Later in the day, more liquid water is simulated than observed. Liquid water is generally undersimulated on 12 January.
Figure 13c shows the 2-m air temperature. The near-surface temperature should be important for tracking West Antarctic melting. Early on 10 January, little cloud liquid water is simulated, and as a possible result the simulations are several degrees too cold. However, much of the warming event during the latter half of 10 January is captured by the simulations (cf. Figs. 13a and 13c). The simulation driven by ERA-Interim better captures the liquid water during the first half of the 11 January, so it better represents the temperature.
Figure 14 illustrates a global climate model (GCM) evaluation example, for GCMs presently under development, again using the WAIS Divide melt event data as a case study. The models considered here are the first version of the atmospheric component of the DOE Energy Exascale Earth System Model (E3SM), EAMv1 (see Rasch et al. 2019), and the most recent update of the NASA Goddard Institute for Space Studies (GISS) GCM (Schmidt et al. 2014), the ModelE. Fields used to nudge horizontal winds in ModlE3 and run EAMv1 are taken from ERA5, the fifth-generation atmospheric reanalysis from the European Centre for Medium-Range Weather Forecasts (ECMWF; Hersbach and Dee 2016). Results show that both models generally simulate the PWV well (Fig. 14a), but that both models overestimate the LWP of the supercooled clouds, particularly for E3SMv1 (Fig. 14b). These overestimations have important consequences to the amount of energy into the snowpack (netSnowpack) at the WAIS Divide, computed as the residual of the net shortwave and longwave radiative energy (netRadiation) into the surface minus the turbulent fluxes (sensible and latent heating) removing energy from the surface (netTurbulence):
An interesting interplay is seen among these terms in Figs. 14c–e. The netRadiation term for both models tends to have a positive bias (too much energy into the snowpack), although ModelE has a greater day-to-day oscillation about zero net flux than does EAMv1 (Fig. 14c). The turbulent flux of energy away from the snowpack’s surface, netTurbulence, is positively biased for EAMv1 while ModelE generally performs well (Fig. 14d). The net effect of the radiative and turbulent fluxes on the energy into the snowpack (Fig. 14e) shows that the positive biases for EAMv1 largely cancel, while the oscillatory nature of the radiative component for ModelE tends to dominate its good simulation of the surface turbulence. A likely contributor to the radiative biases for both models is the change in the surface longwave radiative flux resulting from errors in the LWP that affect cloud emissivity (e.g., Silber et al. 2019c). Figure 14f shows the model bias relative to observations of the net longwave radiation at the surface versus the LWP bias. The plot shows a clear tendency for overestimates in LWP to yield overestimates in surface longwave flux, and vice versa, indicating that the LWP bias is an important factor. Collectively, the results in this figure demonstrate the ability to attribute model biases using component analyses made available from the AWARE data.
Summary and future work
Any time-limited field campaign, even one such as AWARE with its robust suite of instruments and relatively longer duration (1 year), has associated issues regarding representativeness. Geographically, the AMF2 deployment at McMurdo sampled an Antarctic coastal location with adjacent high terrain with complex topography, such that cloud formation and persistence are often influenced by katabatic flows and/or terrain-induced gravity waves. This general situation might apply to numerous coastal Antarctic locations. The AWARE instrumentation at WAIS Divide sampled the SEB under cloud cover representative of most of West Antarctica (e.g., Scott et al. 2017), although WAIS Divide is at a much higher elevation than the West Antarctic ice shelves that are most vulnerable to a warming climate. Hence, the SEB measurements during the January 2016 melt event describe a precursor to and onset of surface melt, rather than a fully developed surface melt that directly impacts an ice shelf or ice cliff via hydrofracturing. AWARE did not make any measurements on the high terrain of East Antarctica, and so a researcher should be very careful about generalizing AWARE findings in cloud physics or aerosol microphysics and chemistry to East Antarctica. Regarding climatology of the specific regions sampled, AWARE trailed a large ENSO event and was then followed by unprecedented sea ice loss and another extensive surface melt event the following spring linked to strong negative southern annular mode (SAM) index combined with a positive index in the first Pacific–South America pattern having a classic Rossby wave train structure (Scott et al. 2019). AWARE data from both McMurdo Station and WAIS Divide might therefore be representative of warmer than normal conditions compared with recent climatology.
Although separated by 1,600 km, there is often a meteorological relationship between the two AWARE sites at McMurdo Station and WAIS Divide Ice Camp. Low pressure troughs in the Ross Sea frequently bring moisture and cloud cover over the WAIS, which can eventually descend onto the Ross Ice Shelf and reach Ross Island from a southerly direction (Coggins et al. 2014; Nigro and Cassano 2014; Silber et al. 2019a). This is particularly evident in case studies described in Scott and Lubin (2014). In contrast to the Arctic, this airmass trajectory also traverses mountain ranges that cause substantial orographic lifting and related ice cloud formation (Scott and Lubin 2016). Tracking of these synoptic-scale patterns by satellite remote sensing and validation of the “end point” in cloud evolution from AWARE measurements at McMurdo might provide further insight into mixed-phase cloud properties that are distinct from the Arctic.
In the first Antarctic climatological assessment from AWARE data presented here, we have seen many contrasts with the high Arctic. These include persistent differences in liquid cloud occurrence, cloud height, and cloud thickness. Antarctic aerosol properties are also quite different from the Arctic, due to the continent’s isolation from lower latitudes by Southern Ocean storm tracks. This brings a seasonal cycle in which most aerosol constituents have maximum concentration in summer, and in which abundances are almost entirely from a variety of Antarctic rather than transported sources. Comparable measurements from two high Arctic sites show springtime maxima comprising the “Arctic haze” that has origins from northern midlatitudes. AWARE data show that Antarctic aerosol abundances are not negligible despite the large-scale dynamical isolation, and the aerosol chemical composition revealed by AWARE measurements implies that aerosol–cloud interaction in the Antarctic deserves further study.
In the preliminary model evaluations presented here, we have considered the WAIS Divide case study sufficiently to note some basic discrepancies between simulations and observations. Much work needs to be done on the specific cloud microphysical parameterizations, or other model components, to realize improvements to model performance over Antarctica. The AMF2 data are an additional resource for developing very stringent tests of mixed-phase cloud parameterization performance. In addition to the orographic forcing by the Transantarctic Mountains that causes climatological contrasts from the Arctic, terrain variability in the local Ross Island area often induces low-level gravity waves that produce unique mixed-phase cloud realizations. The AWARE science team is presently constructing some AMF2 case studies that might be suitable for model evaluation and improvement, and many coauthors on this paper already have experience with AWARE data that could assist other researchers with selecting data for a variety of modeling requirements. Finally, AWARE data should be valuable for planning future Antarctic fieldwork using advanced instrumentation. Examination of the AWARE campaign data in the online ARM Archive can provide guidance for what to expect when various types of meteorological and remote sensing equipment are deployed for extended Antarctic research programs.
AWARE was jointly sponsored and supported by the U.S. Department of Energy Atmospheric Radiation Measurement (ARM) Program and the National Science Foundation via the United States Antarctic Program. AWARE data are available online at the ARM data archive. DL, DHB, KH, IS, JV, and LMR were supported by U.S. Department of Energy Grant DE-SC0017981 and NSF Grant PLR-1443549. DZ and AMV were supported by the U.S. Department of Energy under Grant DE-SC0012704. RCS was supported by NASA Earth and Space Science Fellowship Grant NNX15AN45H. AB and SK were supported by U.S. Department of Energy Grant DE-SC0017967, with additional support for SK by the German Research Foundation (DFG) via the Emmy-Noether Program (Grant KN 1112/2-1). MC is supported by the U.S. Department of Energy under contract DE-AC02-06CH11357. PR was supported by NSF Grant PLR-1543236. AMF was supported by the NASA Radiation Science Program and Modeling, Analysis and Prediction Program. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Center for Climate Simulation (NCCS) at Goddard Space Flight Center. AMF and IS thank Andrew Ackerman and Maxwell Kelley for their assistance using ModleE3. The aerosol composition measurements used in this work are archived at https://doi.org/10.6075/J0GX493P, which includes the Alert aerosol composition measurements (https://doi.org/10.6075/J0959G22), which were supported by Environment Canada, and the Utqiaġvik aerosol composition measurements (https://doi.org/10.6075/J01N7ZN2), which were funded by NSF (ARC-0714052) and are also available from the Arctic Data Center (https://doi.org/10.18739/A22Z12P9Z). The authors are thankful to the technicians, operators, and students who assisted with the aerosol measurements reported here, and in particular Patrick Shaw, Anne Jefferson, and Lelia Hawkins for Utqiaġvik, Desiree Toom and the Department of Defense Canadian Forces staff at Alert, and Jun Liu for the FTIR and XRF analysis for AWARE (https://doi.org/10.6075/J0WM1BKV). Retrievals from the AERI instrument use CO2 concentrations from CarbonTracker (version CT2017, NOAA ESRL; http://carbontracker.noaa.gov; Peters et al. 2007), ozone, temperature, and pressure data from ERA-Interim. This paper is PMEL Contribution Number 4976. This paper is Contribution Number 1587 of the Byrd Polar and Climate Research Center.