Partial pressure of CO2 (pCO2) and dissolved oxygen (DO) in the surface waters of the Amundsen Sea Polynya (ASP) were measured during austral summer 2010–2011 on the Amundsen Sea Polynya International Research Expedition (ASPIRE). Surface pCO2 in the central polynya was as low as 130 µatm, mainly due to strong net primary production. Comparing saturation states of pCO2 and DO distinguished dominant factors (biological activity, temperature, upwelling, and ice melt) controlling pCO2 across regions. Air-sea CO2 flux, estimated using average shipboard winds, showed high spatial variability (-52 to 25 mmol C m-2 d-1) related to these factors. The central region exhibited a high flux of -36 ± 8.4 mmol C m-2 d-1, which is ∼ 50% larger than that reported for the peak of the bloom in the well-studied Ross Sea, comparable to high rates reported for the Chukchi Sea, and significantly higher than reported for most continental shelves around the world. This central region (∼ 20,000 km2) accounted for 85% of the CO2 uptake for the entire open water area. Margins with lower algal biomass accounted for ∼ 15% of regional carbon uptake, likely resulting from pCO2 reductions by sea ice melt. During ASPIRE we also observed pCO2 up to 490 µatm in a small region near the Dotson Ice Shelf with an efflux of 11 ± 5.4 mmol C m-2 d-1 that offset about 3% of the uptake in the much larger central region. Overall, the 2010–2011 ASP was a large net sink for atmospheric CO2 with a spatially averaged flux density of -18 ± 14 mmol C m-2 d-1. This high flux suggests a disproportionate influence on the uptake of CO2 by the Southern Ocean. Since the region has experienced a significant increase in open water duration (1979–2013), we speculate about whether this CO2 sink will increase with future climate-driven change.
The increase of atmospheric CO2 as a result of human activity has drawn much attention in the past years, primarily with respect to its role in altering the Earth’s climate (Manabe et al., 1980). The ocean has sequestered 25–28% of the anthropogenic CO2 since 1960 (Le Quéré et al., 2013), acting as a carbon sink and thus playing a significant role in mitigating climate change (Sabine et al., 2004; Sarmiento et al., 2002; Solomon et al., 2007). The Southern Ocean makes a substantial contribution to this atmospheric carbon sink; over 40% of the anthropogenic CO2 in the ocean has been absorbed south of 40°S (Sallée et al., 2012).
High-latitude oceans are capable of taking up massive amounts of atmospheric CO2 due to high biological productivity and low temperature. The response of the Southern Ocean to climate change and the efficiency of the biological pump influence the degree to which atmospheric carbon is sequestered in the deep ocean and thus the global atmospheric CO2 level (Takahashi et al., 2009; Sigman and Boyle, 2000; Sigman et al., 2010). The CO2 sink in the Southern Ocean is affected by rates of upwelling, wind speed (McNeil et al., 2007; Le Quéré et al., 2007; Lovenduski et al., 2008), biological uptake (Arrigo et al., 1999; de Baar et al., 1995), and ice melt (Ishii et al., 2002; Fransson et al., 2011). Yet the specific role of the Southern Ocean in future atmospheric CO2 uptake is still uncertain due to spatial and temporal variability in the biological and solubility pumps and to under-sampling in critical regions such as coastal Antarctic polynyas (Arrigo et al., 2008a; Carrillo et al., 2004).
Polynyas are recurring areas of open ocean surrounded by sea ice and characterized by high energy and material transfers between the atmosphere and the polar ocean (Smith and Barber, 2007). The open water area typically expands in spring and summer (e.g., Arrigo and van Dijken, 2003), but is mostly ice-covered in autumn and winter, although small winter coastal polynyas are responsible for significant heat exchange and dense water formation in the coastal Antarctic (e.g., Chapman, 1999; Barber and Massom, 2007). Polynyas are often areas of high biological production during summer, facilitating substantial CO2 exchange with the atmosphere (Yager et al., 1995; Miller and DiTullio, 2007). Sea ice can restrict air-sea gas exchange and limit the equilibration between surface waters and the atmosphere (Hood et al., 1999; Tortell et al., 2011). Sea ice, however, is also habitat for microorganisms performing both photosynthesis and respiration, as well as a site for calcium carbonate precipitation and dissolution, all of which can influence gas exchange and affect surface ocean CO2 concentrations (Gosink et al., 1976; Miller et al., 2011; Rysgaard et al., 2007; Fransson et al., 2011).
The Amundsen Sea, located in the South Pacific sector of the Southern Ocean (Figure 1), is one of the least explored areas in Antarctica due to its remote location and historically heavy sea ice cover. It is characterized by a continental shelf that widens from west to east, and deepens toward the continent via a deep trough system that influences ocean circulation and ice sheet dynamics in the region (Nitsche et al., 2007; Wåhlen et al., 2010; Jacobs et al., 2012). It is distinguished by its thick but variable multiyear (perennial) sea ice, interspersed with areas of seasonal sea ice and a number of coastal polynyas (Arrigo et al., 2012), the Amundsen Sea Polynya (ASP) being the largest (Stammerjohn et al., 2014). Among all Antarctic polynyas, the ASP is the fourth largest (with a 1997–2010 average area of 27,300 ± 8,700 km2 during the open period from October 1 to March 31, and maximum open area of ∼ 80,000 km2; Arrigo et al., 2012). From 1997 to 2010, the ASP opened to >10,000 km2 for an average of 132 ± 17.5 (n = 14) days per year (Arrigo et al., 2012). The eastern ASP has experienced a rapid increase in seasonal open water duration (currently 2.6 months longer than in 1979; Stammerjohn et al., 2014), and is also flanked by some of the world’s fastest melting glacial ice (Rignot et al., 2013; Mouginot et al., 2014), including the Pine Island, Thwaites, Crosson, Dotson, and Getz Ice Shelves.
The ASP is estimated by satellite to be the most productive polynya in the Southern Ocean (per unit area) on average, with the highest interannual variability (Arrigo and van Dijken, 2003). Average primary production in summer typically exceeds 1 g C m-2 d-1 (Lee et al., 2013; Alderkamp et al., 2012), much higher than offshore waters of the open Southern Ocean (0.2–0.4 g C m-2 d-1; Arrigo et al., 2008b). Only a few in situ biogeochemical studies have been conducted in the ASP, primarily in the past few years. Tortell et al. (2012) reported measurements of surface water pCO2 and DO in the ASP during January–February 2009, with sea-air CO2 exchange averaging -41.9 µmol m-2 d-1 in the open waters of the polynya, and argued on that basis that the ASP alone contributes 5% of the Southern Ocean CO2 flux.
During the austral summer of 2010–2011, a multidisciplinary team of oceanographers embarked on the Amundsen Sea Polynya International Research Expedition (ASPIRE) to examine the controls and fate of the massive Phaeocystis antarctica bloom of the ASP (Figure 1; Yager et al., 2012; Alderkamp et al., 2014; Schofield et al., 2014; Williams et al., 2014; Yager et al., 2014) during its initial buildup in early summer. Here, we examine the distribution and variability of surface pCO2 and air-sea CO2 flux, assess the sensitivity to physical and biological drivers in the ASP region, and compare our findings with previous studies to estimate the global importance of this climate-sensitive region.
2. Study site and methods
From December 2010 to January 2011, the ASP region was explored extensively by the ASPIRE team onboard the RVIB Nathaniel B. Palmer (NBP; Figure 1; Yager et al., 2012). The cruise track focused on the highly productive central region, but in an effort to link observations with processes, the influences on the polynya from the coastal margins, particularly the Getz Ice Shelf (GIS), Dotson Ice Shelf (DIS), and the Thwaites Iceberg Tongue (TIT), were also explored. Here we focus on underway data collected from the NBP in the open waters (< 50% sea ice cover) of the polynya (December 14, 2010, to January 3, 2011; 72.6–74.3°S, 110–119°W).
Ice concentration and open water
For navigation and planning purposes during the field expedition, sea ice concentration images from Moderate Resolution Imaging Spectroradiometer (MODIS) Terra (250 m resolution) were collected and delivered to the ship electronically from the Antarctic Geospatial Information Center (AGIC), Department of Geology and Geophysics, University of Minnesota. Additionally, ice concentrations were obtained from both in situ field observations and satellite remote sensing images for use in data analysis, as described below.
Throughout the sampling period, visual observations of sea ice concentration were recorded using standardized protocols (Worby and Allison, 1999). These shipboard measurements were used to determine the “open water” sections of the cruise track for which underway data are presented, with open water defined as ice concentration < 50%.
While field observations provided sea ice concentrations for the exact location of our cruise track as it was sampled, satellite remote sensing techniques were also used in this analysis. Daily ASMR-E satellite images (12.5 km resolution) were obtained for the 2010–2011 season to provide an assessment of ice conditions over the larger ASP region and in the months prior to and after our sampling period. Using satellite-derived sea ice concentrations for a patch of ocean surrounding each station, we calculated the open water duration (or number of open water days) as the total number of days the location had < 50% ice concentration from the date of first opening until (and including) the date of sampling. Additionally, we plotted the time course of sea ice concentration around each station and compared it to the measurement of ocean color by MODIS Aqua (1.24 km) to determine the approximate time needed for bloom development. Finally, we estimated the total open water area within the ASP region as all waters that were ice-free, using a stricter threshold of < 10% ice concentration to define ice-free waters. This method and the geographic constraints used to define the ASP region are consistent with calculations of polynya open water area employed by Arrigo et al. (2012).
Parameters at the sea surface
Surface seawater was sampled from the main underway seawater system onboard NBP which draws from a nominal depth of 5 m and pumps the seawater directly (with a minimum of 90° turns) to the Hydro Lab on the main deck (3 m above sea level) where it is analyzed. The 15-cm diameter piping is made of a non-metallic, chemically resistant material that maintains structural integrity under low temperatures and minimizes algal and bacterial growth. Sea surface temperature (SST) and salinity (SSS) were recorded every 10 seconds using an onboard thermo-salinograph (SBE-45 Micro TSG, SeaBird Inc., Bellevue, WA). The precision of temperature and salinity data were 0.002°C and 0.005, respectively.
The NBP carried a pCO2 measurement system from Lamont-Doherty Earth Observatory (LDEO) that was linked to the underway seawater system. The LDEO system continuously measured sea surface mole fraction of CO2 (xCO2 in ppm), using a showerhead equilibrator and a non-dispersive infrared CO2 gas analyzer, and recorded data as part of the Research Vessel Data Acquisition System (RVDAS). Precision of the system was ± 1.5 µatm; accuracy was maintained using a 4th order calibration curve on voltages from 5 CO2 gas standards run every 75 min. The CO2 concentrations in the gas mixtures were calibrated using SIO standards determined by C. D. Keeling’s group using the manometric method. See Sutherland et al. (2011) for further details regarding the CO2 measurement system.
The partial pressure of CO2 in surface water at the temperature of equilibration (pCO2(eq), in µatm) was converted from measured xCO2 (Jiang et al., 2008):
where xCO2(water) is the measured mole concentration of CO2 (ppm), Peq is the barometric pressure at equilibration (atm), and Pv is the water vapor pressure at 100% humidity calculated using the temperature at equilibration Teq (K) and salinity S (Weiss and Price, 1980).
Given the temperature difference between the equilibrator and the sea surface, pCO2 in the equilibrator pCO2(eq) was corrected to surface water pCO2(water) at in situ temperature (Takahashi et al., 1993):
For comparison to other data sets such as chlorophyll a fluorescence, the influence of temperature on in situ pCO2 was removed by applying the same equation to convert to a single sea surface temperature (T = -1°C):
Atmospheric xCO2 was measured onboard NBP by the same system that measured sea surface xCO2, but ship contamination was difficult to remove objectively. In this study, therefore, we interpolated between available hourly air xCO2 observations during the time of ASPIRE from the NOAA/ESRL network (Thoning et al., 2013) at American Samoa (389.06 ± 0.56; n = 366) and South Pole Station (387.30 ± 0.13; n = 484). Thus, xCO2(atm) was assumed to be 388 ppm. As described above, pCO2 in the atmosphere at equilibration (pCO2 (atm), in µatm) was calculated by equations (1) and (2) with xCO2(atm), sea surface temperature Tin situ, and assuming the barometric pressure at sea surface was the same as that measured in the lab by the barometer on the pCO2 system Peq (range of 975–992 mbar).
Underway surface dissolved oxygen (DO) was measured with an oxygen Optode (Model # 3835; AADI Inc., Attleboro, MA; precision < 1 µmol L-1) and surface chlorophyll a fluorescence (Chl a) was measured with an ECO-AFL/FL Fluorometer (Wet Labs, Philomath, OR). The Optode DO measurements were calibrated with titrated samples using the Winkler method. An RMA regression (n = 100; r2 = 0.996) gave standard errors for the slope and y-intercept of < 1% and 6.5%, respectively. Chlorophyll a calibrations at sea were problematic, so we report uncalibrated fluorescence values here for comparison purposes only.
Discrete seawater samples were also collected from below the surface, using a conventional CTD-rosette, and analyzed for nutrients, total dissolved inorganic carbon and alkalinity, chlorophyll a, and dissolved oxygen (see Yager et al., 2014).
Processes controlling pCO2 distribution
Surface pCO2 and DO saturation states were compared in accordance with the method described in Carrillo et al. (2004) to determine the qualitative importance of changes in temperature and biological processes on pCO2:
where DO* is the solubility of O2 for standard air pressure, and was corrected to in situ temperature and salinity using the equations in Garcia and Gordon (1992). Because DO equilibrates with the atmosphere much faster than pCO2, the effects of gas exchange on the data distribution can also be modeled using the Carrillo et al. (2004) approach.
We also calculated the theoretical distribution of pCO2_sat and DO_sat that would be observed if Winter Water (WW) was subject to primary production and warming. Properties for WW were derived from ASPIRE measurements made at the base of the deep mixed layer (∼ 100 m) in the polynya region (temperature, T = -1.8°C; salinity, S = 34.1; total dissolved inorganic carbon, DIC = 2215 µmol kg-1; total alkalinity, ALK = 2291 µmol kg-1; dissolved oxygen, DO = 290 µmol L-1; nitrate, NO3 = 31 µmol L-1; phosphate, PO4 = 2 µmol L-1, silicate, SiO4 = 90 µmol L-1; Yager et al., 2014). We applied a photosynthetic quotient (PQ) of 1.25 mol O2 evolved per mol DIC removed (e.g., Tortell et al., 2011) and used elemental stochiometry observed in the upper 100 m of the ASP (C:Si:N:P = 116:13:16:1; Yager et al., 2014; results were not significantly different if traditional Redfield values were used), reflecting a mixed bloom of diatoms and Phaeocystis antarctica (Arrigo et al., 1999). We allowed nitrate drawdown to contribute to changes in total alkalinity (1:1; Wolf-Gladrow et al., 2007) and included phosphate and silicate in our calculations of the carbonate system. Changes were made stepwise to the above inventories; pCO2 was calculated using CO2calc (Robbins et al., 2010; based on CO2SYS, Lewis and Wallace, 1998), with Mehrbach constants refit by Dickson and Millero (1987) and Dickson (1990). We calculated pCO2_sat and DO_sat as described above. We also calculated similarly the pCO2_sat and DO_sat expected from these photosynthetic impacts plus warming (PQ + warming) to the maximum SST observed in the ASP (+0.1°C).
Additionally, we applied a simple two-end member mixing model to investigate the pCO2 and DO saturation states ASPIRE observed. In this case, we mixed Antarctic Surface Water (AASW) from the central polynya (T = -0.2°C, S = 33.8, DIC = 2041 µmol kg-1, ALK = 2344 µmol kg-1, DO = 490 µmol L-1, NO3 = 6 µmol L-1, PO4 = 0.8 µmol L-1, SiO4 = 67 µmol L-1; Yager et al., 2014) with WW (as above). From values along each mixing line, we then calculated pCO2 using CO2calc, and pCO2_sat as described above, and compared them to calculated values for DO and DO_sat. We assumed that DO mixed linearly as a mass property (as is done with apparent oxygen utilization, AOU, calculations; e.g., Craig, 1971). The resulting mixing-only relationship was not distinguishable from the PQ curve (data not shown).
To model the predicted effects of sea ice melt on the carbonate system (Rysgaard et al., 2007), we added 56 µatm pCO2 (a value determined recently for the ASP region; Fransson et al., 2011) to every observation and compared the distribution to DO, which is not affected by carbonate dissolution. Because of the heterogeneity of sea ice in this region, we might expect some variation in this contribution, but the authors did not report variation (Fransson et al., 2011).
Wind speed and transfer velocity
Underway wind speed was measured by an anemometer (RM Young 5106) located in the ship’s Aloft Observation Station (about 25 m above the sea surface) and corrected for ship motion during the cruise. We also corrected the data to a height of 10 m (u10) by a factor of 0.91 according to Thomas et al. (2005; see also Crusius and Wanninkhof, 2003, and Benschop, 1996).
In the absence of meteorological buoy or station observations in the region, we assumed the underway wind speeds were representative of the entire ASP region (reasonable given the relatively small size of the ASP). This assumption was tested by comparing ASPIRE data (December 14, 2010, to January 3, 2011) to wind data collected by other expeditions to the same general area but with different dates and cruise tracks (NBP 09–01, DynaLiFe, January 11 to February 15, 2009, Tortell et al., 2011; Araon, January 2010, and Araon, February–March 2012, data courtesy of the Korean Polar Research Institute).
Temporally-averaged, height-corrected shipboard wind speed (u10) during the sampling period in the polynya was used to derive the CO2 transfer velocity k for long-term averaged winds (Wanninkhof, 1992):
where Sc is the Schmidt number, a function of sea surface temperature (Wanninkhof, 1992).
Air-sea CO2 flux
The sea surface pCO2 gradient (ΔpCO2, relative to the atmosphere), temperature, salinity, wind speed, and sea level pressure were used to calculate the air-sea CO2 flux (Wanninkhof, 1992) over the study area. The air-sea CO2 flux (mmol C m-2 d-1) was determined as:
where K0 is the solubility of CO2 in the seawater, which is a function of temperature and salinity (Weiss, 1974). Air-sea CO2 flux was spatially interpolated over the polynya region using the underway data from the ship track and the DIVA gridding method built into Ocean Data View 4 (Schlitzer, 2014; http://odv.awi.de). A spatially-averaged flux was then calculated for the entire open-water region as well as for sub-regions such as the central polynya and the southeast region near the DIS.
Total annual flux was roughly estimated by multiplying this spatially-averaged flux by the 1997–2010 average open water period (days) and the average open water area of the polynya (Arrigo et al., 2012), assuming that the flux ASPIRE measured is representative of the entire open water season. When averages were calculated, they are reported with ±1 standard deviation and the total number (n) of observations.
Ice concentration and open water
The springtime polynya opened initially from the southeastern region near the TIT and DIS, with daily open water area in October 2010 averaging 5190 ± 3090 km2 (n = 31; Figure 2). In early November, the open water region began to expand rapidly toward the north into the sea ice pack and toward the east near the GIS (Figure 2A). By mid November and early December, the polynya had grown to about 25,000 km2 (Figures 2B, C, and F). As the NBP entered the polynya in mid-December 2010 for ASPIRE, the open water area was 41,400 km2 (Figures 2D, F). Total polynya area at our departure from the region in early January was 63,300 km2, with the open water area significantly expanded to both the north and west compared to when we first arrived (Figures 2E, F). The average of daily open water area estimates during the measurement period was 48,000 ± 10,400 km2 (n = 21). The maximum open water area that summer was ∼ 78,000 km2 in mid-January 2011 (after the NBP departed). Over the entire austral spring-summer season of ASPIRE (October 1, 2010, to March 31, 2011), the mean daily open water area of the ASP was 28,200 ± 22,100 km2 (n = 182 days), similar to the 1997–2010 average reported by Arrigo et al. (2012).
Stations visited during the cruise had been open for an average of 49 ± 24 (n = 57) days prior to our sampling. By comparing AMSRE (12.4 km2) and MODIS Aqua (1.24 km2) observations, we were able to estimate that the length of time between the disappearance of sea ice and the observation of increasing ocean color (bloom “spin up”) was ∼ 20 days for most stations.
Parameters at the sea surface
Large spatial variability of surface water pCO2 was observed across the ASP (Figure 3A). As the NPB entered the polynya in the west (near 118°W) in mid-December (see Figure 1), undersaturated pCO2 values near 300 µatm were observed across the western region and near the Getz Ice Shelf (GIS). As the NBP departed in early January, traveling again through the western region (∼ 116°W) of the polynya, low pCO2 values of ∼ 200 µatm were observed, suggesting a drawdown of ∼ 100 µatm over about 20 days. Over the entire time we sampled there, the central polynya (73.0–73.7°S) showed strong undersaturation of pCO2 with low values ranging from 130 to 200 µatm. Somewhat higher pCO2 values were observed in the sea ice zone bordering the polynya, especially near the TIT in the northeast. The area near the DIS showed strongly supersaturated pCO2 values of ∼ 430 µatm, with the very highest value (490 µatm) at the western edge of the ice sheet where a large northward current (0.2–0.3 m s-1) of iron-rich, oxygen-poor, modified Circumpolar Deep Water (mCDW) was observed exiting just below the ice shelf at 150–400 m (Sherrell et al., 2014).
During the cruise, surface Chl a was found to be highest across the central ASP, north of 73.7°S (Figure 3B). Relatively low levels of Chl a fluorescence were observed near the GIS, DIS, and TIT. Peak fluorometric and HPLC measurements of Chl a on discrete surface water samples from the central region were ∼ 20 mg m-3 (Alderkamp et al., 2014), so the numeric values from the underway fluorometer are likely too high to be used as mg m-3, but good for relative comparisons.
The distribution of surface DO (Figure 3C) exhibited a pattern similar to Chl a. DO at the surface ranged from 230 to 490 µmol L-1 (or 65 to 130% saturation). As the NBP entered the open water area on December 14, the western portion of the polynya exhibited DO concentrations between 350 and 400 µmol L-1 and was near DO saturation (90–110%). The highest DO values (> 400 µmol L-1) were observed in the central polynya, typically exceeding 125% saturation and corresponding well with maximum Chl a. DO values were lowest (230–350 µmol L-1) near the DIS, especially at the western edge where pCO2 was highest.
The lowest pCO2 observations tended to occur in warmer, low-salinity surface waters where high DO was also observed (Yager et al., 2012). Significant correlations were found between pCO2 and sea surface temperature (SST; R = 0.50, n = 6500) and between pCO2 and sea surface salinity (SSS; R = -0.57, n = 6500), but the relationships were non-linear (Figures 4A and 4B). Chl a and pCO2 were more closely correlated (R = -0.87; n = 6500; Figure 4C). This correlation did not improve significantly when pCO2 was corrected to a single temperature (pCO2 (T), where T = -1°C). The best linear relationship with pCO2 was found when Chl a was log transformed (R2 = 0.89, n = 6500, p < 0.01; Figure 5).
Processes controlling pCO2 distribution
A strong linear association was observed between surface pCO2 and DO saturation states (R2 = 0.95, n = 6500, p < 0.01; Figure 6A). The distribution of observations was consistent with our model of Winter Water (pCO2_sat = 126%, DO_sat = 75%) being modified by net photosynthesis alone (PQ) or by both net photosynthesis and warming (PQ + warming; Figure 6A). Underway data fell into three of the four quadrants described by Carrillo et al. (2004). The spatial distribution of data from each of the quadrants (Figure 6B) indicated that most observations in Quadrant I (corresponding to net photosynthesis) were located in the central polynya, where the maximum DO_sat (133%; 484 µmol L-1) and minimum pCO2_sat (34%; 133 µatm) were observed. Saturation of pCO2 (pCO2_sat) and undersaturation of DO typically decreased with increasing distance from both the ice shelf and the northern sea ice margin. Observations in Quadrant IV (both gases undersaturated) were found at the margins of the central zone, along the western inbound leg, and in other areas where some sea ice was present (south central and eastern areas of the polynya). Observations from Quadrant III (indicating net respiration) were located mainly to the southeast of the polynya near the DIS, where the highest supersaturation of pCO2 (126%; 489 µatm) and the greatest undersaturation of DO (55%; 203 µmol L-1) were recorded. No observations fell into the fourth quadrant designated by Carrillo et al. (2004), where both pCO2 and DO are supersaturated (suggestive of warming).
A small subset of the data did not follow the PQ model; these data, located at the edge of the DIS, fell in the lower right of Quadrant III, dominated by respiration (Figure 6A). Because Chl a there was very low, and no other significant sources of labile organic matter were detected in this region, active microbial respiration at the surface was unlikely (see Williams et al., 2014). Instead, the low O2 and high pCO2 suggest the influence of deep water brought to the surface. The physical properties of this region indicate a much deeper mixed layer than elsewhere in the polynya (Figure 7); given the arrangement of the DIS and TIT, the offshore winds from the south may be favorable for upwelling (Figure 8). Buoyancy-driven upwelling was also likely with known interactions between warmer, saltier mCDW and ice shelf basal melt (see Jacobs et al. 2012; Yager et al., 2012; Sherrell et al., 2014). Indeed, if we plot the pCO2_sat and DO_sat for mCDW brought to surface ocean pressure (mCDW in ASP has properites of: T = +0.7°C, S = 34.6, DIC = 2255 µmol kg-1, ALK = 2344 µmol kg-1, DO = 200 µmol L-1, PO4 = 2.1 µmol L-1; SiO4 = 107 µmol L-1; Yager et al., 2014) the DIS data suggest a mixing line between WW and mCDW (Figure 6A).
The pCO2_sat versus DO_sat data distribution was significantly offset from the origin (equilibrium saturation for both gases; Figure 6A). If we account for the effects of sea ice alkalinity contributions in this region (Fransson et al., 2011), however, the data intersect the origin (see inset, Figure 6A). Local variations in the sea ice contribution could explain some of the scatter in the data; e.g., deviations from the PQ and PQ + warming lines. Some variation could also be attributable to air-sea gas exchange, but few data followed the expected curvature (Figure 6A), except perhaps data in the uppermost left of Quadrant I.
Wind speed and transfer velocity
Variable wind speeds were observed across the ASP during ASPIRE (Figure 9) with a shipboard average of 8.7 ± 3.5 m s-1 (n = 6209), a maximum value of 19 m s-1, and a minimum of 0.2 m s-1. Average wind speeds were not significantly different (p < 0.01) from the average winds of three other summertime ASP expeditions (DynaLiFe 2009, Araon 2010, Araon 2012). When height-corrected to 10 m, ASPIRE values reduce to 7.9 ± 3.2, with maximum at 17 m s-1. NCEP/NCAR reanalysis wind data (National Weather Service, 2014), which are interpolated over a much larger area of the Amundsen Sea, report monthly averaged wind speeds of 5.0 ± 2.6 m s-1 for December 2010 (http://www.cpc.ncep.noaa.gov/products/wesley/reanalysis.html), considerably lower than our observations. This difference is not surprising given that there are few in situ meteorological data available for input to the NCEP/NCAR reanalysis. Since our data agreed reasonably well with those from three other recent expeditions to the ASP, we used them here for flux estimates.
With a range in sea surface temperature from -1.8 to 0.1°C (average = -0.74 ± 0.40; n = 6209), the Schmidt number varied from 2061 to 2304 (average = 2169 ± 52, n = 6209). Gas transfer velocity varied from 12.9 to 13.7 cm h-1 (average = 13.3 ± 0.2 cm h-1; n = 6209). Solubility of CO2 ranged from 0.063 to 0.068 mol kg-1 atm-1 (average = 0.065 ± 0.001 mol kg-1 atm-1; n = 6209).
Air-sea CO2 flux
With ΔpCO2 values from -242 to 116 µatm (median = -106 µatm; average = -102 ± 99 µatm; n = 6209), air-sea gas exchange rates ranged from -51.8 to 24.9 mmol C m-2 d-1 (negative values indicate oceanic uptake, positive values are oceanic outgassing). The spatial variability of the CO2 flux (Figure 10) mirrored the pCO2 distribution since temperature and salinity varied comparatively little, with the highest uptake in the central polynya. Over the entire open water region from December 14 to January 3, we calculated a spatially averaged flux of -18 ± 14 mmol C m-2 d-1 (-0.21 ± 0.17 g C m-2 d-1). Summed over the daily open water area of the polynya (average = 48,000 ± 10,400 km2) over the time of ASPIRE sampling (21 d), carbon uptake was 0.22 ± 0.17 Tg C. The CO2 flux in the central polynya was double the polynya-wide rate, at -36 ± 8.4 mmol C m-2 d-1 (-0.43 ± 0.10 g C m-2 d-1) and accounted for 85% of the total uptake when summed over the central region (∼ 20,000 km2): 0.18 ± 0.04 Tg C. The efflux in the southeast near the DIS was 11 ± 5.4 mmol C m-2 d-1 (0.13 ± 0.07 g C m-2 d-1). Covering a much smaller area (about 2000 km2), this efflux added up to 0.01 ± 0.003 Tg C, offsetting only ∼ 3% of the drawdown in the center polynya over the same time period (21 d).
Comparison to other regions
As the most biologically productive polynya per unit area Arrigo and van Dijken, 2003), the ASP provides a window to investigate and better understand the sensitivities and vulnerability of biogeochemical cycling in the coastal regions of Antarctica. Our analysis confirms that the extremely low surface pCO2 observed in the central ASP was driven by the intense phytoplankton bloom. With the Southern Ocean’s highest algal productivity, then, it is perhaps not surprising that the carbon flux density (CO2 flux per unit area) observed in this productive zone during ASPIRE was greater than for most other continental shelves and comparable to the highest rates reported in other Antarctic and Arctic polynyas (Ducklow and McCallister, 2004) and the Chukchi Sea (Bates et al. 2006).
Much of our current knowledge about carbon biogeochemical cycling in coastal Antarctica comes from field studies at a few sites, most extensively in the Ross Sea Polynya (RSP) and along the western Antarctic Peninsula (wAP). Extensive phytoplankton blooms occur on the Ross Sea continental shelf during spring and summer (Sweeney, 2003), corresponding with surface pCO2 as low as ∼ 130 µatm (Sweeney et al., 2000). In the central region of ASP, we observed a similar minimum surface pCO2 (∼ 130 µatm) but a higher spatially-averaged air-sea CO2 flux (-36 ± 8.4 mmol C m-2 d-1) than the peak flux of ∼ 24 mmol C m-2 d-1 observed in the RSP (Sweeney 2003). The ASP is smaller in area, but its early summer CO2 flux density is at least 50% larger than peak rates in the RSP. We note, however, that Sweeney (2003) applied the NCEP-NCAR reanalysis wind speed, which may underestimate the flux.
Carrillo et al. (2004) investigated the surface waters of the Palmer LTER site along the wAP and showed that DO and pCO2 varied systematically from atmospheric equilibrium, according to the relative importance of various physical and biological controls (their “four quadrant” approach). Unlike ASPIRE, LTER observations were found in all four quadrants (on a quadrant map similar to Figure 6A) and the data go solidly through the origin (100% pCO2_sat, 100% DO_sat). Large temperature and gas exchange effects on oxygen and CO2 saturation in the wAP surface waters were more obvious than in the ASP. Their study was later in the season (January–February) and the site was mostly ice-free by the time of sampling. Moreover, their study also found that observations in Quadrant I (with DO supersaturation and pCO2 undersaturation) were mainly distributed adjacent to the coast or to the south (in Marguerite Bay), where surface stratification was enhanced by recent glacial run-off or sea ice melt, respectively. Their study did not include any observations in the vicinity of ice shelves (which were located south of their study region). The strong net respiration signal they observed (Quadrant III) was associated with shelf-break upwelling, as opposed to the wind- or buoyancy-driven upwelling that we observed in the ASP in the vicinity of the DIS.
Mechanisms important to ASP CO2 flux
Polynyas are defined by the dynamics of sea ice. In addition to biological dynamics in sea ice and the impacts of microbial photosynthesis and respiration on surface ocean pCO2 and DO (e.g., Yager et al., 1995; Fransson et al., 2011), sea ice can impact surface pCO2 via CaCO3 precipitation during ice formation or dissolution during melt, in combination with brine rejection (Rysgaard et al., 2007). In a study of this effect in the pack ice surrounding the ASP during 2008–2009, Fransson et al. (2011) estimated that the dissolution of CaCO3 during sea ice melt could explain a reduction in surface fCO2 of up to 56 µatm, in close agreement with results of 60 µatm obtained by Rysgaard et al. (2007) for the Arctic. Such a reduction in pCO2, independent of a change in DO, is consistent with the offset in the ASPIRE data from the origin in Figure 6A. ASPIRE data therefore independently confirm the Fransson et al. (2011) estimate, although the scatter of data around the PQ and PQ + warming curves (Figure 6a) suggests some variability in the sea ice contribution. The sea ice alkalinity-driven reduction in surface pCO2 (relative to O2) also explains the data found in Quadrant IV (which in the absence of sea ice processes would indicate cooling) that we observed in the marginal zones of the ASP. Most importantly, the sea ice contribution reduces pCO2_sat before the phytoplankton bloom develops, reduces opportunities for springtime outgassing of wintertime respiration (from supersaturated WW), and contributes modestly (∼ 15%) to the carbon uptake in the region, supporting the idea that sea ice contributes significantly to this polar carbon pump (Rysgaard et al., 2007).
ASPIRE observations in Quadrant III (with supersaturated pCO2 and undersaturated DO) were largely distributed near the DIS and TIT. Expression of wintertime respiration-driven oversaturation under the ice (e.g. Yager et al., 1995) is an unlikely explanation for these waters, because this southern region of the ASP is often partially open during winter and then fully opens in early November (see Figure 2, as well as Stammerjohn et al., 2014). As there are no significant sources of allochthonous organic carbon in coastal Antarctica, these surface waters are probably not actively net-heterotrophic (see Williams et al., 2014), but rather reflect the surfacing of long-submerged deep water through deep mixed layers or wind-driven or buoyancy-driven upwelling. Oversaturation from winter respiration may explain the Quadrant III waters near the TIT, because the sea ice interspersed in this iceberg field was observed during ASPIRE to be thick and impenetrable.
Gas exchange should leave a “fingerprint” on the quadrant plot (Figure 6A). As described by Carrillo et al. (2004), with O2 equilibration faster than that for pCO2, we would expect to see observations tipping toward the horizontal axis as individual water parcels experience gas exchange. This effect is very well illustrated in the LTER data from the wAP (Carrillo et al., 2004), but not so obvious in the ASPIRE data. Because we observed a highly linear relationship in these data, with little scatter between the model PQ curves and the 100% DO_sat axis, the impact of gas exchange is either indistinguishable from variability in the PQ or sea ice alkalinity contribution, or simply low compared to net photosynthesis. Most of the deviations from the model photosynthesis curve are above the line and can be explained by warming; exceptions are the observations in the left, uppermost corner of Quadrant I that appear to “fall off” the PQ + warming line toward the 100% DO_sat line, probably indicating gas exchange.
The estimate of carbon uptake during the 21-day period of ASPIRE is quite small (0.22 Tg) compared to other large ocean carbon sinks (e.g., Takahashi et al., 2000), including the RSP (25 ± 10 Tg; Sweeney et al., 2000). The ASP, however, very likely takes up carbon outside of the ASPIRE observation window. Indeed, the AMSR-E satellite estimates of open water area show that the polynya continued to expand (Figure 2F) and MODIS Aqua ocean color time series data, processed to Level 2 for each ASPIRE station, indicate that chlorophyll a continued to rise for several more weeks after we sampled (data not shown). We also know that nitrate was still available at the surface (> 7 µM) when the NBP departed the region (Williams et al., 2014). With some assumptions about continuity, scaling up the flux density can be attempted both temporally (extending the bloom season) and spatially (extending the open water area). If we apply ASPIRE flux observations to the sea-ice climatology (Arrigo et al., 2012) and propagate the errors (Bevington 1969), we can extend the ASPIRE estimate to the full season using the daily average polynya flux (-18 ± 14 mmol C m-2 d-1) and the productive open water season (132 ± 18 d; less 20 d for spin up). This calculation results in an estimate of -2.0 ± 1.6 mol C m-2 a-1. The rate doubles to -4.0 ± 1.1 mol C m-2 a-1, if we apply the central polynya flux density. For comparison, the annual air-sea CO2 flux in the Ross Sea is estimated to be -1.5 ± 1.5 mol C m-2 a-1, based on multi-season studies conducted during 1996–1997 (Sweeney, 2003).
Additional justification for extending our observations into late summer can be found from Tortell et al. (2012), who report findings on pCO2 and air-sea CO2 flux in the ASP during the mid-to-late summer season of a previous year (January 11 to February 16, 2009); i.e., one month later compared to our study, just after the peak in the Phaeocystis antarctica bloom (Alderkamp et al., 2012). They reported surface pCO2 as low as ∼ 100 µatm and the air-sea CO2 flux density for ice-free polynya waters to be -41.9 mmol C m-2 d-1. At the same time, nitrate lower than that seen during ASPIRE (7 µM) was observed in a few areas of the central polynya (Alderkamp et al., 2012). The observations suggest that the bloom likely continued for at least another month after the NBP departed, supporting a continuation and enhancement of the high flux observed during ASPIRE, although it could also indicate interannual variability, known to be high in this region (Arrigo and van Dijken, 2003; Stammerjohn et al., 2014).
If we apply the spatially-averaged flux to the average open water area of the polynya (27,300 ± 8,700 km2) and propogate the errors, the ASP CO2 uptake scales up to 0.65 ± 0.57 Tg C. Again, the rate doubles (to 1.3 ± 0.56 Tg C) using the central polynya flux density. Clearly, some understanding is needed of seasonally-changing spatial distributions; our extrapolation is tenuous, as we do not know the relative contributions of the three zones over the entire season. Assuming that their relative contributions do not change, and comparing this estimate of annual uptake with that of the Southern Ocean south of 62°S (an area of 1.5 × 107 km2 and annual flux of -40 Tg C; Takahashi et al., 2009), the ASP accounts for 2–3% of the annual carbon uptake by the Southern Ocean, even though the ASP occupies only 0.25% of the total area. This calculation is more conservative than the estimate by Tortell et al. (2011), yet the ASP is still clearly disproportionally important in its contribution to Southern Ocean air-sea CO2 flux and the global carbon cycle.
The high pCO2 variability associated with high interannual variability of productivity may contribute to strong climate sensitivity in the ASP (Yager et al., 2012). Based on satellite data (Arrigo et al., 2012), temporal variation of primary production in the ASP is closely related to the timing and duration of open water in the polynya, which in turn affects the timing and duration of the phytoplankton bloom. The satellite sea ice record indicates a strong trend toward earlier sea ice retreat in the eastern ASP region over the observing period of 1979 to 2013 (Stammerjohn et al., 2014). Because the ASPIRE data offer a first glimpse at early season conditions, we can make some inferences about future carbon cycling in this region. Specifically, an earlier sea ice retreat would not necessarily increase phytoplankton productivity if the system were still light limited. In that case, buildup of wintertime respiration (indicated by supersaturated pCO2 and undersaturated DO in WW) could outgas if sea ice were simply exported from the region by winds to expose open water. Depending on the wind speed, however, equilibration with the atmosphere could take several weeks. Although there are satellite observations of a small, wind-driven ASP in the winter, the dense pack ice offshore would prevent a much larger wind-driven opening. Instead, the polynya likely opens initially by wind-driven exposure, but grows via solar warming of low-albedo surface water and subsequent sea ice melt (e.g., Minnett, 1995). What we see currently in the early-season ASP is a reduction in both surface salinity and pCO2 by the freshwater and alkalinity of the sea ice melt itself, and a switch from oceanic outgassing to oceanic uptake before the phytoplankton bloom begins. We note that the pCO2 reduction of 56 µatm due to sea ice melt according to Fransson et al. (2011) is for the entire 70-m mixed layer and assumes complete melting of the sea ice column; only a partial melt into the surface layers would be needed to reduce surface pCO2 and prevent CO2 outgassing.
When combined, Figures 2 and 3A reveal the close connection between surface pCO2 and the timing of sea ice melt observed during ASPIRE. The polynya first opened in the eastern ASP (east of ∼ 115°W) in early November, allowing for a longer season of phytoplankton growth and the almost 200 µatm differential in pCO2 between the central and western polynya (west of ∼ 115°W), which was just opening when we arrived in mid-December. Furthermore, we observed temporal pCO2 variation when we resampled some areas: the western ASP at the beginning of the cruise (December 14, 2010; the westernmost leg of the cruise track at ∼ 117.5°W) was slightly undersaturated in pCO2 (∼ 330 µatm), presumably due to newly exposed water; during the final period of the cruise (December 24, 2010) in a nearby area (cruise leg at ∼ 116°W), pCO2 was substantially more undersaturated (∼ 200 µatm) due to a longer open water period. As in the Weddell Sea (Bakker et al. 2008) and many other polynyas (Miller and DiTullio, 2007), the seasonal pattern of melting sea ice plays a crucial role in affecting pCO2, and thus the air-sea CO2 flux in the ASP.
How even near future regional sea ice changes might affect CO2 fluxes in this critically important region is uncertain. We speculate that an earlier opening of the ASP could extend the productive season and enhance the magnitude of the phytoplankton bloom, if enough light and iron are available. In this event, the ASP could become a greater carbon sink in the near future. However, extending the open water season too much could reduce sea ice melt-induced stratification and enhance light limitation (Schofield et al., 2014), suggesting that the ASP carbon sink also depends on the continued longevity of the surrounding seasonal marginal ice zone.
Recent studies (Le Quéré et al., 2007; Lovenduski et al., 2008) indicate that the Southern Ocean CO2 sink has weakened over the past three decades (1979–2004) due to large-scale changes in winds and in the wind-driven ocean circulation. This trend is predicted to continue into the future. Climate changes in the Antarctic are playing an increasingly significant role in regulating the size of the carbon sink in the Southern Ocean. There is no doubt that Antarctic polynyas are highly climate-sensitive, with some undergoing radical changes like the ASP and Mertz Glacier Polynya (Shadwick et al., 2013); they should continue to be foci of future studies of biogeochemical cycling in the Antarctic.
As the most biologically productive polynya per unit area in Antarctic waters, with the highest interannual variability (Arrigo and van Dijken, 2003), the ASP provides a window to investigate and better understand the sensitivities and vulnerability of biogeochemical cycling in the coastal regions of Antarctica. With ASPIRE, we were able to identify three main regions of the ASP having different pCO2 concentrations and thus different air-sea CO2 fluxes: a large central zone dominated by a massive phytoplankton bloom, low pCO2, and high rates of CO2 uptake; a small near-ice-shelf zone dominated by deep mixed layers, high pCO2, and outgassing; and a third marginal ice zone with relatively low biological productivity but undersaturated pCO2, resulting from sea ice melt-driven reductions in pCO2. Currently, the regional impact of the ASP is dominated by the phytoplankton bloom, making the ASP a significant carbon sink relative to other continental shelves and a disproportionate contributor to the overall Southern Ocean carbon uptake. As the net impact of the ASP on future global carbon cycling depends on the climate sensitivity and temporal distribution of these three zones, a better seasonal understanding of these distinctive regions is greatly needed.
Data accessibility statement
Original pCO2 data is publically available at Lamont Doherty Earth Observatory: http://www.ldeo.columbia.edu/res/pi/CO2/carbondioxide/Palmer_data/1005SFC.PRT. All other data are publically available from BCO-DMO: http://www.bco-dmo.org/dataset/540038
© 2014 Mu et al. This is an open-access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.
We thank the captain and crew of the R/V Nathaniel B. Palmer and the Raytheon Polar Services support team for their hard work and dedication. We also thank the rest of the ASPIRE science team and the Yager Lab group for providing many useful comments and feedback. A special thanks goes to Leta Schoeller, Michelle LaRue, and Paul Morin at the AGIC for providing ASPIRE with near real-time MODIS Terra images at sea, and to Povl Abrahamsson (British Antarctic Survey) for generating the polynya cruise track map on one of those images (Figure 1). The pCO2 instrument and data processing for the NB Palmer is skillfully operated by the Lamont Doherty Earth Observatory Carbon Dioxide Research Group led by T. Takahashi. We thank Pieter Tans and Kirk Thoning for permission to use the NOAA/ESRL network data. We also thank A.C. Aldercamp, B. Hopkinson, two anonymous reviewers, and the Associate Editor for their very constructive comments on earlier drafts.
This project was funded by NSF Office of Polar Programs, Antarctic Organisms and Ecosystems (ANT-0839069 to PY, ANT-0838975 to SS, and ANT-0944727 to K. Arrigo for support of KEL).
The authors have no competing interests or conflicts of interest.
This is an open-access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.