Secular change in atmospheric Ar∕N2 and its implications for ocean heat uptake and Brewer–Dobson circulation
- 1Environmental Management Research Institute, National Institute of Advanced Industrial Science and Technology (AIST), Tsukuba 305-8569, Japan
- 2Faculty of Education, Miyagi University of Education, Sendai 980-0845, Japan
- 3Center for Environmental Measurement and Analysis, National Institute for Environmental Studies, Tsukuba 305-8506, Japan
- 4Division for Research and Education, National Institute of Polar Research, Tokyo 190-8518, Japan
- 5Department of Climate and Geochemistry Research, Meteorological Research Institute, Tsukuba 305-0052, Japan
Correspondence: Shigeyuki Ishidoya (email@example.com)
Systematic measurements of the atmospheric Ar∕N2 ratio have been made at ground-based stations in Japan and Antarctica since 2012. Clear seasonal cycles of the Ar∕N2 ratio with summertime maxima were found at middle- to high-latitude stations, with seasonal amplitudes increasing with increasing latitude. Eight years of the observed Ar∕N2 ratio at Tsukuba (TKB) and Hateruma (HAT), Japan, showed interannual variations in phase with the observed variations in the global ocean heat content (OHC). We calculated secularly increasing trends of 0.75 ± 0.30 and 0.89 ± 0.60 per meg per year from the Ar∕N2 ratio observed at TKB and HAT, respectively, although these trend values are influenced by large interannual variations. In order to examine the possibility of the secular trend in the surface Ar∕N2 ratio being modified significantly by the gravitational separation in the stratosphere, two-dimensional model simulations were carried out by arbitrarily modifying the mass stream function in the model to simulate either a weakening or an enhancement of the Brewer–Dobson circulation (BDC). The secular trend of the Ar∕N2 ratio at TKB, corrected for gravitational separation under the assumption of weakening (enhancement) of BDC simulated by the 2-D model, was 0.60 ± 0.30 (0.88 ± 0.30) per meg per year. By using a conversion factor of 3.5 × 10−23 per meg per joule by assuming a one-box ocean with a temperature of 3.5 ∘C, average OHC increase rates of 17.1 ± 8.6 ZJ yr−1 and 25.1 ± 8.6 ZJ yr−1 for the period 2012–2019 were estimated from the corrected secular trends of the Ar∕N2 ratio for the weakened- and enhanced-BDC conditions, respectively. Both OHC increase rates from the uncorrected- and weakened-BDC secular trends of the Ar∕N2 ratio are consistent with 12.2 ± 1.2 ZJ yr−1 reported by ocean temperature measurements, while that from the enhanced-BDC is outside of the range of the uncertainties. Although the effect of the actual atmospheric circulation on the Ar∕N2 ratio is still unclear and longer-term observations are needed to reduce uncertainty of the secular trend of the surface Ar∕N2 ratio, the analytical results obtained in the present study imply that the surface Ar∕N2 ratio is an important tracer for detecting spatiotemporally integrated changes in OHC and BDC.
The Ar∕N2 ratio of air is a unique tracer for detecting changes in the spatiotemporally integrated air–sea heat flux or ocean heat content (OHC). This is because variations in the Ar∕N2 ratio at the Earth's surface are driven by air–sea Ar and N2 fluxes that reflect changes in the solubility of these gases in seawater (e.g., Keeling et al., 2004). The increase in the global OHC is one of the most important parameters for evaluating Earth's climate system (e.g., Trenberth and Fasullo, 2010). The relative temperature dependence of the solubility of Ar is larger than that of N2, so that the atmospheric Ar∕N2 ratio increases with increasing ocean temperature. Other noble gases behave in a similar way. Bereiter et al. (2018), for example, analyzed Kr∕N2 and Xe∕N2 ratios in air trapped in ice cores and estimated that the mean global ocean temperature increased by 2.57 ± 0.24 ∘C over the last glacial transition (20 000 to 10 000 years ago). In terms of ocean heat content, the present-day global OHC increase is evaluated from analyzing the ocean temperature measurements using Argo floats (e.g., Cheng et al., 2019). Therefore, precise measurements of the Ar∕N2 ratio in air can be used as an independent validation of the OHC estimation from the ocean data. However, long-term changes in the atmospheric Ar∕N2 ratio have not been reported so far due to difficulties in detecting a trend with sufficient accuracy, although a few past studies observed its seasonal variations (Keeling et al., 2004; Blaine, 2005; Cassar et al., 2008; Ishidoya and Murayama, 2014).
We have reported in past studies that the Ar∕N2 ratio decreases with increasing altitude in the stratosphere due to gravitational separation of the atmospheric constituents (e.g., Ishidoya et al., 2013; Sugawara et al., 2018). The magnitude of gravitational separation is determined by a balance between mass-independent atmospheric transport, that is, advection and eddy diffusion, and mass-dependent molecular diffusion in the atmosphere. This implies that gravitational separation will be influenced by the atmospheric circulation changes. Therefore, we can use the observed gravitational separation as an indicator of the Brewer–Dobson circulation (BDC) in the stratosphere. There has been no study to evaluate the effect of gravitational separation changes in the stratosphere on the concentrations and isotopic ratios of atmospheric trace gases at the surface, since it has been believed that the gravitational separation signal from the stratosphere is too small to be detected at the surface. Therefore, in our previous studies, we simulated δ, which is an indicator of gravitational separation derived from the Ar∕N2 ratio and stable isotopic ratios of N2, O2 and Ar, using atmospheric transport models by assuming the surface δ to be zero (Ishidoya et al., 2013; Sugawara et al., 2018; Belikov et al., 2019). However, because long-term changes in the Ar∕N2 ratio near the surface are expected to be extremely small, e.g., 0.00026 % corresponding to a heat input of 100 ZJ (1 zetajoule = 1021 J) into a 10 ∘C ocean (Keeling et al., 2004), a very small secular change in the stratospheric gravitational separation signal near the surface may modify the long-term change in the surface Ar∕N2 ratio. If so, an evaluation of gravitational separation of the whole atmosphere is needed for a precise estimate of the global OHC increase based on long-term changes in the surface atmospheric Ar∕N2 ratio.
In this paper, we present results from an analysis of 8-year-long measurements of the atmospheric Ar∕N2 ratio at the ground surface stations and propose δΩ as a new indicator of gravitational separation of the whole atmosphere by using a 2-D model. By using the simulated δΩ, we derived the secular trend of the Ar∕N2 ratio corrected for gravitational separation changes associated with the BDC change. Finally, we estimated the global OHC change based on the corrected Ar∕N2 ratio.
Atmospheric Ar∕N2 has been observed at Tsukuba (TKB; 36∘ N, 140∘ E), Japan, continuously since February 2012 (Ishidoya and Murayama, 2014). Located on the roof of a laboratory building of the National Institute of Advanced Industrial Science and Technology (AIST), sample air is taken from an air intake by using a diaphragm pump with gas velocity higher than 5 ms−1 (4 mm i.d. and a flow rate of 4 L min−1) at the tip of the air intake to prevent thermally diffusive inlet fractionation (Sturm et al., 2006; Blaine et al., 2006). The sample air is introduced into a 1 L stainless-steel buffer tank after water vapor in the air is reduced by using an electric cooling unit at 2 ∘C. The gas is then exhausted from the buffer tank at a flow rate of about 4 L min−1. A small portion of this exhausted gas is introduced into a 3.2 mm (1∕8 in.) o.d. stainless-steel tube, and any remaining water vapor is removed using a cold trap at −90 ∘C. Finally, the remaining sample air is vented through an outlet path at a rate of about 10 mL min−1, and only a minuscule amount of it is transferred to the ion source (or waste line) of a mass spectrometer (Thermo Scientific Delta V) through an insulated thin fused-silica capillary. As for the reference air, it is always supplied from a high-pressure cylinder at a flow rate of about 4 mL min−1, and a minuscule amount of it is introduced into the ion source (or waste line) of the mass spectrometer through another fused-silica capillary. For the continuous measurements, alternate analyses of the sample and reference air are made repeatedly. The measurement time required to obtain one data value is 62 s, but we usually use the 550-data averaged value as the reported Ar∕N2 ratio obtained from the continuous observations (about 11 h averaged value). We also measure stable isotopic ratios of N2, O2 and Ar, and O2∕N2 ratio and CO2 mole fraction simultaneously, and use the 550-data averaged values for the stable isotopic ratios and one data value without averaging for O2∕N2 ratio and CO2 mole fraction; these measurements constitute the continuous observations. Details of the continuous measurement system used are given in Ishidoya and Murayama (2014).
We have also collected air samples at a rate of once per month at Hateruma Island (HAT; 24∘ N, 124∘ E) and Cape Ochiishi (COI; 43∘ N, 146∘ E), Japan, since July 2012 and October 2013, respectively, and at Syowa station (SYO; 69∘ S, 40∘ E) since January 2016 for the analyses of the atmospheric Ar∕N2 ratio. Each air sample is taken from an air intake by using a diaphragm pump at a flow rate of about 5 L min−1 and filled into a 1 L stainless-steel flask whose inner walls are silica-coated after removing water vapor using a cold trap (−40 ∘C at HAT and COI, and −80 ∘C at SYO). Similar to our previous study (Ishidoya et al., 2016), the 1 L stainless-steel flasks are equipped with two metal-seal valves on each side to equalize the inner pressure to the pressure between the two metal-seal valves to prevent a mass-dependent fractionation due to small leak through the valve. During air sampling, the inner pressure of the flask is kept at an absolute pressure of 0.2 MPa using a back-pressure valve (Tohjima et al., 2003). The sample air collected in the flasks are then sent to AIST and analyzed by using the same mass spectrometer as described above. The sample air is supplied from the flask at a flow rate of about 4 mL min−1 through a cold trap (about −50 ∘C), and a minuscule amount of it is introduced into the ion source (or waste line) of the mass spectrometer through a fused-silica capillary. It is noted that we also used 760 mL glass flasks with Viton O-ring seal valves on each side for collecting air samples at HAT and COI prior to September 2015 and January 2019, respectively. However, we found slight seasonally dependent differences in the Ar∕N2 and O2∕N2 ratios between the analytical results from the 1 L stainless-steel flasks and those from the 760 mL glass flasks. It is interesting to note that the O2∕N2 ratio from the 1 L stainless-steel flasks agrees well with the O2∕N2 ratio reported by the National Institute for Environmental Studies (NIES) (e.g., Tohjima et al., 2019), considering the difference in the span sensitivity of the O2∕N2 ratio between the AIST and NIES (Aoki et al., 2021). Therefore, we have decided to adopt the Ar∕N2 data obtained from the 1 L stainless-steel flasks and correct the data from the 760 mL glass flasks based on the comparison of the Ar∕N2 ratios measured from the stainless-steel flasks and the glass flasks at HAT for the period of October 2015–January 2019. The cause(s) of such an offset between the stainless-steel flasks and glass flasks has not been determined yet, but it may be related to the seasonal difference in the ambient temperature during the time the flasks were shipped from the observational sites to our laboratory and its effect on the condition of Viton O-ring seal valves used in the glass flasks.
The Ar∕N2 ratio is usually reported in per meg units as follows.
Here, the subscripts “sample” and “standard” indicate the sample air and the standard gas, respectively. Because Ar constitutes 9334 µmol mol−1 of air by volume (Aoki et al., 2019), 5 per meg of δ(Ar∕N2) is equivalent to about 0.05 µmol mol−1. In this study, δ(Ar∕N2) of each air sample was determined against our primary standard air (cylinder no. CRC00045) using the mass spectrometer Thermo Scientific Delta V. Our air standards, which are classified into primary and secondary, are dried ambient air or industrially purified air-based CO2 standard filled in 48 L high-pressure cylinders. As shown in Fig. 1, variations in the annual average δ(Ar∕N2) of our three secondary standards are within ±0.9–±2.2 per meg (±1.6 per meg, on average) and nearly stable for 8 years with respect to the primary standard. Therefore, we allowed an uncertainty of ±1.6 per meg for the annual average δ(Ar∕N2) observed in the present study associated with the stability of the standard air, which corresponds to an uncertainty of ±0.28 per meg per year for the 8-year-long secular trend. We have also prepared high-precision gravimetric standard mixtures of Ar, O2, N2 and CO2, with standard uncertainties for the Ar and O2 molar fractions of 0.6 to 0.8 µmol mol−1 (Aoki et al., 2019). From the measurements of the gravimetrically prepared standard mixtures by the mass spectrometer, it was confirmed that the span sensitivity of δ(Ar∕N2) obtained from the mass spectrometer agreed to within 0.2 % of the gravimetric values of the standard mixtures, in the range from −4500 to +1800 per meg of δ(Ar∕N2) against our primary standard air.
In the present study, we use 1-week averaged values from the continuous observation at Tsukuba after implementing the following data selection procedure. First, the δ(Ar∕N2) values with δ15N higher than 3.0 per meg were excluded from the analyses. As mentioned above, the δ(Ar∕N2) and δ15N values are already 11 h averaged values. We have found these high-δ15N events accompanied by high-CO2 events, as well as occasionally with slightly high-δ(Ar∕N2) events, especially in the winter, but they did not correlate with variations in the isotopic ratio of O2 and Ar. Therefore, it appears that some unspecified interferences of mass 29 (possibly 13C16O and/or fragments of hydrocarbons) rather than the molecular–diffusive separation of 15N14N and 14N14N must have been superimposed on the observational results of δ15N during these events. It is possible that these high-CO2 and δ15N events occur under a stable atmospheric condition in the winter, so that simultaneously observed δ(Ar∕N2) may also be modified by local effects such as thermally diffusive separation of Ar and N2 due to a temperature inversion near the surface (Adachi et al., 2006). Therefore, the threshold value of 3.0 per meg was determined to be reasonable, considering that an average δ15N value of 1.1 ± 1.7 per meg was observed at HAT for the period of October 2015–January 2020, while the observed CO2 mole fractions over the same period were much closer to the values of the background air than those observed at TKB. After the above data selection procedure, 1-week averaged values of δ(Ar∕N2) were calculated. The measurement uncertainty of the 1-week averaged values of the continuous observation was estimated to be about ±3 per meg as a standard deviation from the best-fit curve shown in Fig. 2 discussed below, while that of the flask air sample measurements was estimated to be about ±7 per meg from repeated analyses of the same air samples.
3.1 Atmospheric δ(Ar∕N2) observed at ground surface stations in Japan and Antarctica
Figure 2 shows atmospheric δ(Ar∕N2) observed at COI, TKB, HAT and SYO. Best-fit curves to the data and long-term trends obtained using a digital filtering technique (Nakazawa et al., 1997) are also shown. Using this filtering technique, the average seasonal cycle of δ(Ar∕N2) was modeled by a fundamental sine–cosine and its first harmonic with the respective periods of 12 and 6 months. The residuals obtained by subtracting the average seasonal cycle from the data were interpolated linearly to calculate the daily values of δ(Ar∕N2), which were then smoothed by a 26th-order Butterworth filter with a cutoff period of 36 months to obtain the interannual variation. The interannual variation was then subtracted from the original data, and the average seasonal cycle was determined again from the residuals. These steps were repeated until we obtained an unchanging interannual variation. In this study, we have defined an average linear increasing–decreasing trend as the “secular trend” (as in Fig. 5 discussed below).
As seen in Fig. 2, we can distinguish clear seasonal δ(Ar∕N2) cycles at COI, TKB, and SYO and some interannual variations at TKB and HAT. Figure 3 shows the detrended values of δ(Ar∕N2) and average seasonal δ(Ar∕N2) cycles observed at all four sites. The seasonal maxima were found in the summertime, which is expected since the sea surface temperatures around the observational sites reach seasonal maximum in the summertime, due to the larger relative-temperature-dependent solubility of Ar compared to that of N2. The peak-to-peak amplitudes of the seasonal δ(Ar∕N2) cycles were 21 ± 10, 11 ± 4, 5 ± 10 and 32 ± 9 per meg at COI, TKB, HAT and SYO, respectively. The uncertainties for the amplitudes indicate standard deviations of the detrended values from the average seasonal cycle. The uncertainties at COI, HAT and SYO were found to be not only larger than that at TKB, but also ±7 per meg of the uncertainty originated from the repeated analyses of the same flask air sample. This would be due to the fact that the uncertainty of each analysis value of the standard air (about ±5 per meg, black dots in Fig. 1) is superimposed on the uncertainty of each analysis of the flask air sample and continuous measurement. Therefore, a mean squared error expected for the observational data from the flask air sample is about ±9 per meg, which is comparable to the uncertainties in the seasonal amplitudes in Fig. 3. Corrections to the δ(Ar∕N2) data at HAT and COI prior to September 2015 and January 2019 discussed above (corrections based on the comparison of the δ(Ar∕N2) values from the stainless-steel flasks and the glass flasks) could also be contributing to the uncertainties.
Similar increases in the seasonal δ(Ar∕N2) cycle amplitude with increasing latitude were also observed by Keeling et al. (2004) and Cassar et al. (2008). Cassar et al. (2008) also reported on the seasonal δ(Ar∕N2) cycle at SYO with a peak-to-peak amplitude of 21 ± 8 per meg. The amplitude at SYO found in this study is consistent with that found by Cassar et al. (2008), within the quoted uncertainties. For La Jolla (LJO; 33∘ N, 117∘ W), USA, located at a similar latitude to TKB, Keeling et al. (2004) and Blaine (2005) found a seasonal δ(Ar∕N2) cycle with a peak-to-peak amplitude of about 10 per meg. This agrees with the amplitude at TKB observed in this study. Seasonal minima and maxima at SYO and LJO reported by Cassar et al. (2008) and Keeling et al. (2004), respectively, are in general agreement with those observed at SYO and TKB in this study. On the other hand, the seasonal δ(Ar∕N2) cycle at HAT was not so clear, but the average peak-to-peak amplitude may be slightly smaller than the 14 ± 6 per meg observed at Kumukahi (20∘ N, 155∘ W), USA, located at a similar latitude to HAT (Keeling et al., 2004). Similar and consistent results obtained by this and other studies give confidence in our ability to capture natural variations of δ(Ar∕N2) in the atmosphere.
Figure 4 shows variations in δ(Ar∕N2) observed at COI, TKB and HAT, after subtracting the seasonal cycles and shorter-term variations of less than 36 months. For analyses of the interannual variation, we mainly used the data from TKB and HAT since the observations at these stations date back to 2012 and are longer than data from other sites. Variations in the 0–2000 m global OHC are shown (Fig. 4), reported by the National Oceanographic Data Center (NOAA) and National Centers for Environmental Information (NCEI) (updated from Levitus et al., 2012, https://www.nodc.noaa.gov/OC5/3M_HEAT_CONTENT/, last access: 14 January 2020). The OHC values are shown as anomalies from the baseline value observed in mid-1980s. In the figure we also plot interannual variation of the OHC values obtained by using the same digital filtering technique used in Fig. 2 and globally averaged surface temperature anomalies (Japan Meteorological Agency, http://www.data.jma.go.jp/cpdinfo/temp/nov_wld.html, last access: 14 January 2020). Rates of change of the interannual variations of δ(Ar∕N2) and OHC are also shown. As can be seen from the figure, δ(Ar∕N2) show significant interannual variations and slight secular increasing trends while the global OHC shows a more prominent secular increase. Moreover, the observed variations in the change rates of δ(Ar∕N2) and OHC are quite similar to each other in phase, suggesting a strong correlation between the large-area air–sea heat flux and the interannual variations in δ(Ar∕N2). The minima of the rate of change of δ(Ar∕N2) and OHC appeared at the beginning of 2016 when a maximum in the surface temperature anomaly appeared. This correspondence is qualitatively reasonable since a decrease in the OHC change rate indicates a decrease in the net ocean heat uptake, thus leading to an increase in surface temperature.
As mentioned above, the ratio of interannual variation to secular increase is larger for δ(Ar∕N2) than for OHC. To examine this difference, we estimated the interannual variation of the atmospheric δ(Ar∕N2) expected from the air–sea Ar and N2 fluxes caused by the interannual variation in the global OHC. We converted the change rate of OHC to that of δ(Ar∕N2) by assuming a coefficient of 3.5 × 10−23 or 3.0 × 10−23 per meg per joule, which was derived from the following equations (Keeling et al., 1993).
Here, FAr (F) is the net sea-to-air Ar (N2) flux in moles m−2 s−1, d (d) is the temperature derivatives of the solubility of Ar (N2) in mole m−3 K−1 (Weiss, 1970), is the net air-to-sea heat flux in J m−2 and CP is the heat capacity of seawater in J m−3 K−1. In Eqs. (2) and (3), the assumption that surface waters fully equilibrate could lead to overestimation of the gas fluxes. As a first approximation we modeled the global ocean as one box and assumed an average temperature of 3.5 or 7.5 ∘C. The temperatures of 3.5 and 7.5 ∘C, corresponding to the respective coefficients of 3.5 × 10−23 (including deep water) and 3.0 × 10−23 per meg per joule (not including deep water), were the average values of the ocean model shown in Fig. 1 of Bereiter et al. (2018) for the present-day ocean. We also assumed constant CP and salinity of 3.9 × 106 J m−3 K−1 and 35 ‰, respectively. To convert FAr and to changes in atmospheric δ(Ar∕N2), we employed 5.124 × 1021 g for the total atmospheric mass of dry air (Trenberth, 1981), 28.97 g mol−1 for the mean molecular weight of dry air, 3.6 × 1014 m2 for the surface-ocean area of the Earth, and respective fractions of 0.00933 and 0.7808 for Ar and N2 in the atmosphere.
As a result, the interannual variation in the change rates of the global OHC was estimated to drive only 10 % of that of the atmospheric δ(Ar∕N2). This discrepancy would be due to the fact that the troposphere, and not only the ocean, does not mix perfectly on a timescale of a year and that the surface-ocean temperature anomalies would be a large source of interannual variation on a yearly timescale for the observed δ(Ar∕N2) in the near-surface air. Therefore, in order to interpret the relationship between the interannual variations of OHC and δ(Ar∕N2) more quantitatively, we need to consider the local heat anomalies and atmospheric transport effects. In other words, a much longer-term δ(Ar∕N2) variation is less affected by the surface-ocean anomalies and atmospheric transport but will include the influence signature of the average temperature from the surface to the deeper part of the ocean. In this regard, Suga et al. (2008) estimated the renewal time of permanent pycnocline water in the North Pacific to be 2–4 years for eastern subtropical mode water; 2 and 5–9 years for the lighter and denser subtropical mode water, respectively; and 10–20, 20–30 and >60 years for the lighter, middle and denser central mode water, respectively. Therefore, it is expected that the secular trend of the δ(Ar∕N2) values obtained during 2012–2019 (8 years) in the present study does not reflect the deep OHC change.
Figure 5 shows the δ(Ar∕N2) values observed at TKB and HAT, along with their best-fit curves and interannual variations from Fig. 2. In the figure, we have also plotted the annual average values of δ(Ar∕N2) obtained at these sites. The data are expressed as anomalies from the average value for the observation period. From the figure, we can distinguish secularly increasing trends of δ(Ar∕N2) at both of the sites throughout the observation periods, with large interannual variations superimposed on these trends. Therefore, we applied another best-fit curve consisting of the fundamental and its first harmonics and a linear secular trend to the observed data (black dotted lines) to extract the secular trends as a component of the linear trend of the best-fit curve (thick black solid lines). The secular trends were found to be 0.75 ± 0.30 and 0.89 ± 0.60 per meg per year at TKB and HAT, respectively. The uncertainties for TKB (HAT) were evaluated, taking into account the respective uncertainties of ±0.11 and ±0.28 per meg per year (±0.53 and ±0.29 per meg per year) for the regression and the long-term stability of the standard air. Comparable secular trends of 0.70 ± 0.33 per meg per year for TKB and 1.06 ± 0.61 per meg per year for HAT were also obtained from the difference in the annual average value between 2012 and 2019 for each station. Although, it is possible that these changes observed over the study period might not represent a long-term trend but are part of a large interannual variation. Nevertheless, it would of interest to see if it is possible to obtain a scientifically meaningful OHC change based on the secular δ(Ar∕N2) trend reported earlier. Accordingly, we used the secular trend at TKB (0.75 ± 0.30 per meg per year), because of the smaller uncertainty than that obtained at HAT, to propose a method to estimate the global OHC or BDC change based on the surface and the stratospheric secular trends of δ(Ar∕N2). For this purpose, we simulate the gravitational separation effect on the δ(Ar∕N2) in the whole atmosphere by using a 2-D model described below in Sect. 3.2.
3.2 Simulation of gravitational separation and its effect on δ(Ar∕N2) at ground surface
As mentioned in the Introduction, we have reported observational results of gravitational separation in the stratosphere (Ishidoya et al., 2008, 2013, 2018; Sugawara et al., 2018). Those results showed that stratospheric δ(Ar∕N2) also decreases rapidly with increasing altitude above the tropopause. Also, not only are there large year-to-year variations in the difference between the stratospheric and tropospheric δ(Ar∕N2) values, but year-to-year variations in stratospheric δ(Ar∕N2) are much larger than those observed in the troposphere (Ishidoya et al., 2013, 2018). Therefore, we need to explore the possibility of tropospheric δ(Ar∕N2) variations caused by changes in the stratospheric gravitational separation that influence the whole troposphere. We have compared the observed and simulated gravitational separation of atmospheric major components above the tropopause in previous studies (Ishidoya et al., 2013, 2018; Sugawara et al., 2018; Belikov et al., 2019), but we did not consider gravitational separation in the troposphere. Therefore, in this study we updated the SOCRATES model (Huang et al., 1998) to calculate variations in Ar and N2 from the surface to 120 km, taking into account molecular diffusion processes generating gravitational separation. SOCRATES is a 2-D model with parameterized eddy diffusivity coefficients, tuned to produce a realistic stratospheric age of air distribution. In the present study we carry out sensitivity studies by arbitrarily modifying the mass stream function in the model. Here, we describe only those modifications we made to the model for the calculation of δ(Ar∕N2). An additional description of the SOCRATES model is presented in Appendix A.
First, our 2-D model was expanded to be able to calculate explicitly any inert gas components and their isotopic ratios and elemental ratios, including δ(Ar∕N2). In our previous model studies, we used 44CO2 and 45CO2 to reproduce gravitational separation for the sake of simplicity. However, it is now necessary to explicitly include the molecular diffusion coefficients of all gas components in order to reproduce the molecular diffusion processes in the stratosphere more accurately, because the molecular diffusion coefficient is dependent on the molecular mass. In this study, the molecular diffusion coefficient of the gas component A in air (DA) was calculated using the following equation (Poling et al., 2001).
Here, T and p are the temperature (K) and pressure (hPa), respectively. The reciprocal average of mA and mair, mA-air, is defined as follows.
Here, mA and mair are the molecular masses of component A and air, respectively. σA and σair are the diffusion volumes of the component A and air, respectively. The diffusion volumes of 40Ar, 28N2 and air are 16.2, 18.5 and 19.7, respectively (Poling et al., 2001).
Second, a new δ value has been defined and used for δ(Ar∕N2) in this study. Usually, the isotopic ratios or elemental ratios of the atmospheric major compositions are expressed as values relative to their ratios in the troposphere. Therefore, it is common to treat the δ values at the ground surface as zero. However, high-precision analyses have recently revealed that, as is the case in δ(Ar∕N2), the δ values at the ground surface are not always constant, and they have seasonal and interannual variations, as well as long-term trends (Keeling et al., 2004; Cassar et al., 2008; Blaine, 2005; Bent, 2014). The purpose of our analysis here is to evaluate the effect of gravitational separation on the δ value at the ground surface using the 2-D model. Therefore, it is no longer appropriate to assume that the δ value at the ground surface is always zero. Observationally, small variations at the ground surface can be detected by using specific gas cylinders as constant references. In a numerical model, a constant reference is also needed for evaluating the effects of gravitational separation on the δ value at the ground surface. In our 2-D model, we used the ratio of the total amount (M) of each gas component in the model atmosphere as the constant reference and defined a new δ value, δΩ, using the following equation.
The total amount was calculated by integrating from the ground surface to the altitude of 120 km. According to this definition, δΩ will be zero if there are neither molecular separations nor sinks/sources in the entire atmosphere. In the actual atmosphere, δΩ becomes negative in the stratosphere due to gravitational separation but will be a small positive value in the troposphere. A 50-year-long spin-up calculation was carried out for δ(Ar∕N2)Ω under steady-state condition, and we found that δ(Ar∕N2)Ω in the troposphere reached a steady-state value of about 30 per meg. In other words, the tropospheric Ar∕N2 ratio is enriched by about 30 per meg relative to the homogenous atmosphere due to the atmospheric gravitational separation. If the gravitational separation is strengthened due to atmospheric circulation changes in the stratosphere, δΩ at the ground surface will slightly increase. On the other hand, if the gravitational separation is weakened in the stratosphere, δΩ at the ground surface will decrease. Therefore, by using δΩ, it is possible to examine how a change in the gravitational separation in the stratosphere affects δΩ at the ground surface. The meridional distribution of δ(Ar∕N2)Ω calculated using the updated SOCRATES model and its comparison with the stratospheric δ(Ar∕N2) observed in our previous studies are presented in Appendix B.
Third, the age of air (AoA) is calculated using an idealized tracer. In our previous model calculations, the AoA was calculated from the CO2 mole fraction. However, since the actual increase in CO2 mole fraction given at the ground surface is not a linear increase but includes non-linear trends and interannual fluctuations, it is not possible to estimate the correct AoA from the simple lag time method (e.g., Waugh and Hall, 2002). Therefore, in this study, we introduced an inert idealized tracer that increases linearly at the ground surface and calculated the AoA in the stratosphere from the mole fraction of this idealized tracer.
3.3 Secular trends in the observed and simulated δ(Ar∕N2) and their implication for changes in OHC and BDC
To examine how δ(Ar∕N2)Ω is influenced by changes in the BDC, model simulations were made by arbitrarily changing the mean meridional circulation (MMC) represented by mass stream function in the 2-D model so that AoA changed by ±0.02 yr yr−1 at 35 km over the northern mid-latitudes. The simulated AoA values for the 35 km height are shown in Fig. 6. Here the positive and negative rates correspond to the weakening and enhancement of the BDC simulations, respectively. These simulations with fixed horizontal mixing are not enough to represent the mechanism to drive the observed AoA change in the real atmosphere, but they do serve as a kind of sensitivity test. In this regard, we present the annual mean meridional distribution of the AoA trend for the weakened- and enhanced-BDC simulations in Appendix B. Based on some past studies, we have adopted a value of ±0.02 yr yr−1 as AoA trends for the BDC simulations: for example, Diallo et al. (2012) reported an increase in AoA of about 0.03 yr yr−1 in the middle stratosphere for the period 1989–2010 based on the ERA-Interim reanalysis data, while Fritsch et al. (2020) reported AoA unchanged within uncertainties over the northern mid-latitudes for the period 1975–2016 based on the observations of CO2 and SF6 updated from Engel et al. (2009), and Waugh (2009) showed, based on results from chemistry–climate models, a negative AoA trend between −0.005 and −0.02 yr yr−1 for the time period and location considered by Engel et al. (2009). The secular AoA trends forced in our study fall within the range of these studies, although the observation periods do not overlap with each other. We regard these simulations to be a first step in investigating the effect of gravitational separation of the whole atmosphere on δ(Ar∕N2) at the surface.
Secular changes in the simulated δ(Ar∕N2)Ω at the surface obtained from the weakened- and enhanced-BDC simulation and those at 35 km are also shown in Fig. 6. As can be seen from the figure, clear inverse relationships are found between the secular trends of δ(Ar∕N2)Ω at the surface and those at 35 km. In the weakened-BDC simulation, δ(Ar∕N2)Ω changes secularly by 0.15 and −4.5 per meg per year, respectively, at the surface and 35 km. In the enhanced-BDC simulation, respective secular changes in δ(Ar∕N2)Ω by −0.13 and 4.0 per meg per year at the surface and 35 km are found. As discussed above, atmospheric δ(Ar∕N2) is estimated to increase by 3.5 × 10−23 per meg when 1 J of heat is added to a 3.5 ∘C ocean water mass. Based on this relationship, when OHC increases by 93 ZJ during 2012–2019, which is the global 0–2000 m OHC increase from the NOAA/NCEI data, the increase rate in atmospheric δ(Ar∕N2) is estimated to be 0.46 per meg per year. Therefore, 0.15 (−0.13) per meg per year for the surface δ(Ar∕N2)Ω due to the weakening (enhancement) of the BDC is a non-negligible trend compared with the expected changes in atmospheric δ(Ar∕N2) due to the global OHC increase.
Figure 7 shows the same annual average values and secular trend of atmospheric δ(Ar∕N2) at TKB as in Fig. 5. We calculated an increase rate of δ(Ar∕N2)cor by subtracting 0.15 per meg per year from the observed secular trend of 0.75 ± 0.30 per meg per year to remove the estimated effects of δ(Ar∕N2)Ω increase obtained from the weakened-BDC simulation. Thus, the derived secular increase rate of δ(Ar∕N2)cor, which represents the increase rate of δ(Ar∕N2) driven only by the OHC change, is 0.60 ± 0.30 per meg per year. We can convert this increase rate to the global OHC increase rate by assuming the abovementioned coefficient of 3.5 (3.0) × 10−23 per meg per joule (hereafter referred to as the increase rate of “OHC”). The obtained secular increase in OHC by 17.1 ± 8.6 (20.2 ± 10) ZJ yr−1 is shown in Fig. 7, together with that of the global 0–2000 m OHC reported by NOAA/NCEI (hereafter referred to as “OHCoc”). The increase rate of OHC is consistent with the OHCoc value of 12.2 ± 1.2 ZJ yr−1 within uncertainties. Recently, by extracting a solubility-driven component of APO from their atmospheric O2∕N2 ratio and CO2 measurements and ocean model simulations, Resplandy et al. (2019) estimated the increase rate of the global OHC to be 12.9 ± 7.9 ZJ yr−1 for the period 1991–2016, which is consistent, within the uncertainties, with the OHCoc during the same period. The results of the present study and Resplandy et al. (2019) suggest the usefulness of atmospheric observations for independent confirmation of ocean heat uptake estimated from ocean temperature measurements.
As described above, the increase rate in OHC obtained by using δ(Ar∕N2)Ω from the weakening BDC simulation agrees with the OHCoc estimate. On the other hand, the increase rate in OHC of 25.1 ± 8.6 (29.6 ± 10) ZJ yr−1, obtained by using δ(Ar∕N2)Ω from enhanced-BDC simulation assuming the coefficient of 3.5 (3.0) × 10−23 per meg per joule, is significantly larger than the OHCoc estimate. In general, modeling studies have pointed to an accelerating BDC due to anthropogenic climate change (e.g., Austin and Li, 2006). However, the increase rate in OHCoc agrees well with OHC based on the weakened-BDC simulation rather than on the enhanced-BDC simulation. In this regard, several balloon-borne observations (Ray et al., 2014) and the ERA-Interim reanalysis data (Diallo et al., 2012) have suggested aging of air in the northern-hemispheric mid-latitude mid-stratosphere, implying a slowdown in the deep northern-hemispheric branch of the BDC. Garfinkel et al. (2017) analyzed a series of chemistry–climate model experiments conducted for the period of January 1960 through 2014. They found that structural changes in BDC have occurred in the BDC since 1980s; BDC accelerated in the lower stratosphere in the Northern Hemisphere and tropics but not in the mid-stratosphere, and specifically since 1992, mean age increased by 0.12 years in the mid-stratosphere of the northern-hemispheric mid-latitude, and tropical mass upwelling has slowed down by 2 %. As discussed in our previous study (Sugawara et al., 2018), gravitational separation of the stratospheric air is sensitive to changes in mean meridional circulation rather than horizontal mixing. Therefore, it is thought that the increase in mean age in the mid-stratosphere in the northern mid-latitude and the slowdown of tropical upwelling, suggested by the recent observational and modeling studies, are consistent with our weakened-BDC simulation of the δ(Ar∕N2)Ω.
We also carried out an additional simulation of δ(Ar∕N2)Ω, considering the interannual variation in the BDC, to examine its effect on the large interannual variations of the observed δ(Ar∕N2) seen in Fig. 4. As the BDC interannual variation, we simply assume a 10 % change in the MMC intensity with a 3-year cycle by changing the mass stream function in the 2-D model. Flury et al. (2013) reported that the speeds of BDC towards the NH and SH show interannual variabilities with amplitudes of about 21 % and 10 %, respectively, and that the amplitude of variability in the ascent rate at the Equator is 21 %. Therefore, the 10% change in the MMC in our simulation is not an unrealistic assumption. As a result, the increase rate of δ(Ar∕N2)Ω showed an interannual variation with a peak-to-peak amplitude of ±0.4 per meg per year. This interannual variation is non-negligible but still rather small compared to that found in the observed δ(Ar∕N2), about ±4.5 per meg per year, as seen from Fig. 4. Therefore, it is suggested that the interannual variation of surface δ(Ar∕N2) is driven mainly by solubility change in seawater and/or that the assumed ±10 % changes in the MMC intensity in our model are smaller than the actual interannual variation of the MMC. In addition, analytical artifacts and the extremely difficult challenge of maintaining stable standard air for δ(Ar∕N2) could also be the cause(s) of the interannual variation. Therefore, further studies are needed to achieve quantitative understanding of the discrepancy.
Consequently, if we regard OHCoc as representing “true” global OHC, then we can estimate the secular trend and interannual variations in the BDC from δ(Ar∕N2) observed at the surface. Conversely, if the simulated δ(Ar∕N2)Ω represents true BDC changes, then we can validate OHCoc by using OHC. Therefore, the surface δ(Ar∕N2) is found to be a unique tracer for detecting changes in a spatiotemporally integrated OHC and BDC. Not only precise observations of δ(Ar∕N2) over longer periods of time, but also improvements in δ(Ar∕N2)Ω simulation using 3-D atmospheric transport models are important for future research advances in this field. For example, recently, Birner et al. (2020) simulated lower-stratospheric δ(Ar∕N2) using the TOMCAT/SLIMCAT 3-D chemical transport model, which has been updated to include gravitational fractionation of gases. Such activities will contribute significantly to understanding the mechanisms of spatiotemporal variations in the stratospheric and the surface δ(Ar∕N2).
We have been carrying out systematic measurements of atmospheric δ(Ar∕N2) at TKB and HAT since 2012 and at COI and SYO since 2013 and 2016, respectively. Clear seasonal cycles of δ(Ar∕N2) with summertime maximum were found at TKB, COI and SYO, with peak-to-peak amplitudes of 21 ± 10, 11 ± 4, 5 ± 10 and 32 ± 9 per meg at COI, TKB, HAT and SYO, respectively, which are in general agreement with those observed at similar latitudinal sites by other investigators. The observed δ(Ar∕N2) at TKB and HAT, after subtracting seasonal cycles and shorter-term variations, showed significant interannual variations and slight, but detectable, secularly increasing trends. The observed interannual variations correlated positively with that of the global OHC, suggesting a strong correlation between large-area air–sea heat flux and the long-term change in δ(Ar∕N2). However, the ratio of interannual variation to secular increase is found to be much larger in δ(Ar∕N2) than that in OHC, so further studies are needed to interpret the discrepancy.
We improved the 2-D model we used in previous studies to calculate gravitational separation in order to evaluate its effect on the long-term change in the surface δ(Ar∕N2). We simulated weakened and enhanced BDC by arbitrarily changing the MMC (represented by mass stream function in the model) and obtained effects of 0.15 and −0.13 per meg per year, respectively, on the secular trend of the surface δ(Ar∕N2). If we apply the correction for gravitational separation to the secular trend of δ(Ar∕N2) observed at TKB, then an average increase rate of 0.60 ± 0.30 per meg per year for δ(Ar∕N2) during 2012–2019 was obtained by assuming a weakening BDC. By using a conversion factor of 3.5 (3.0) × 10−23 per meg per joule by crudely assuming a one-box ocean with a temperature of 3.5 (7.5) ∘C, we obtained an increase rate in the global OHC of 17.1 ± 8.6 (20.2 ± 10) ZJ yr−1 for the 8-year period, which is consistent with 12.2 ± 1.2 ZJ yr−1 reported by NOAA/NCEI from the Argo float observations. On the other hand, the increase rate in the global OHC, obtained from the secular trend of δ(Ar∕N2) at TKB under enhanced BDC, was found to be significantly larger than that from the Argo float observations. These results indicate that the surface δ(Ar∕N2) is a unique tracer for spatiotemporally integrated OHC and BDC. Although an increase in global OHC is well known as an essential parameter to evaluate recent global warming, there is no method yet to adequately measure OHC via ocean temperature observations in the full-depth volume of the ocean. Long-term precise observations of δ(Ar∕N2) will meet this demand after correction for gravitational separation of the whole atmosphere.
We performed numerical simulations using a two-dimensional model of the middle atmosphere (SOCRATES) developed by the National Center for Atmospheric Research (NCAR) (Huang et al., 1998; Park et al., 1999; Khosravi et al., 2002). Since details of our model calculation for gravitational separation have already been described in Ishidoya et al. (2013) and Sugawara et al. (2018), only a brief description is given here. The model extends from the surface to 120 km altitude with a 1 km vertical resolution and from 85∘ S to 85∘ N latitude with a 5∘ latitudinal resolution. The time step of this model can be varied to accommodate chemical transport equations of various species. However, in our study, we used a time step of 1 d, because Ar and N2 molecules have no chemical reaction and the time constant of the molecular diffusion process is sufficiently longer than 1 d. The meridional and vertical eddy diffusivity coefficients (Kyy and Kzz) are parameterized by including three types of waves: planetary, gravity and tidal waves. The mass transport processes caused by molecular diffusion were originally taken into account only above the mesosphere in SOCRATES, since the molecular diffusion effect was thought to be negligibly small in the troposphere and stratosphere, compared with the eddy diffusion effect. But since our study needed to include the effect of molecular diffusion in the lower atmosphere, however small compared to eddy diffusion, we simply lowered its vertical domain to the surface for the calculation of molecular diffusion. The molecular diffusion theory included in SOCRATES is based on Banks and Kockarts (1973).
The annual mean meridional distribution of the δ(Ar∕N2)Ω value calculated using the updated SOCRATES model is shown in Fig. B1. The model shows that the vertical δ(Ar∕N2)Ω gradient increases with increasing height, especially at high latitude, which is consistent with the meridional distributions reported by Ishidoya et al. (2013) and Sugawara et al. (2018) calculated using the original SOCRATES model. The basic structure of the vertical–meridional δ(Ar∕N2)Ω distribution can be interpreted as a result of a balance between the mass-dependent molecular diffusions and the mass-independent transport processes. Figure B2 shows the vertical δ(Ar∕N2) profiles observed over Sanriku (39∘ N, 142∘ E), Japan, on 4 June 2007 (Ishidoya et al., 2013) and Biak (1∘ S, 136∘ E), Indonesia, on 22–28 February 2015 (Sugawara et al., 2018). The vertical δ(Ar∕N2)Ω profiles calculated by the updated SOCRATES model for the same seasons are also shown. As seen from the figure, the average vertical gradients of the observed vertical δ(Ar∕N2) profiles are generally reproduced by the calculated δ(Ar∕N2)Ω, although the fluctuations in the observed profiles are not simulated. These fluctuations are also observed over Antarctica and could be attributed to the horizontal mixing of the stratospheric air over the region (Ishidoya et al., 2018); their occurrences at low and middle latitudes are still not well understood. Overall, however, we are satisfied with the performance of the updated SOCRATES model in reproducing the average vertical gradient of the δ(Ar∕N2) profiles from the surface to the stratosphere.
Figure B3 shows the annual mean meridional distribution of the AoA secular trend calculated using the updated SOCRATES model for weakened- and enhanced-BDC simulations. The simulations were made by arbitrarily changing the mass stream function in the model so that AoA changed by +0.02 (weakened BDC) or −0.02 (enhanced BDC) yr yr−1 at 35 km over the northern mid-latitudes. The AoA trends are larger in the middle stratosphere than those in the lower stratosphere for the weakened-BDC simulation. This altitudinal increase in the AoA trend is consistent with that derived from the ERA-Interim (Diallo et al., 2012); however, the updated SOCRATES model cannot reproduce the negative AoA trend in the lower stratosphere found in Fig. 13 of Diallo et al. (2012). Ray et al. (2014) also reported an increase and decrease in AoA in the middle and lower stratosphere, respectively. Therefore, simulations of the BDC secular trend using the updated SOCRATES model do not fully represent the details of the meridional distribution in the real atmosphere. Further studies using 3-D models for validating the δ(Ar∕N2)Ω secular trend discussed in the present study are needed.
The observational data of δ(Ar∕N2) presented in this study can be accessed by contacting the corresponding author.
SI designed the study, carried out δ(Ar∕N2) measurements and drafted the manuscript. SS improved the 2-D model and carried out δ(Ar∕N2)Ω simulations. YT and DG managed the collections of air samples at Hateruma, Ochiishi and Syowa station. KI examined the relationship of Ar and N2 fluxes with air–sea heat flux. NA prepared gravimetric standard mixtures of Ar, O2, N2 and CO2. SS, YT, DG, KI, YN, NA and SM examined the results and provided feedback on the manuscript. All the authors approved the final manuscript.
The authors declare that they have no conflict of interest.
We thank the staff of the Global Environmental Forum (GEF) and the Science Program of the Japan Antarctic Research Expedition (JARE) for their work to collect the air samples at Hateruma and Ochiishi stations (GEF) and Syowa station (JARE).
This study was partly supported by the JSPS KAKENHI (grant nos. 15H02814, 19H01975 and 19K03963) and the Global Environment Research Coordination System from the Ministry of the Environment, Japan (grant nos. METI1454 and METI1953).
This paper was edited by Peter Haynes and reviewed by three anonymous referees.
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