Contributors | Affiliation | Role |
---|---|---|
Seltzer, Alan M. | Woods Hole Oceanographic Institution (WHOI) | Principal Investigator |
Barry, Peter | Woods Hole Oceanographic Institution (WHOI) | Co-Principal Investigator |
Jenkins, William J. | Woods Hole Oceanographic Institution (WHOI) | Co-Principal Investigator |
Khatiwala, Samar | University of Oxford (Oxford) | Co-Principal Investigator |
Nicholson, David P. | Woods Hole Oceanographic Institution (WHOI) | Co-Principal Investigator |
Smethie Jr., William M. | Lamont-Doherty Earth Observatory (LDEO) | Co-Principal Investigator |
Stanley, Rachel | Wellesley College | Co-Principal Investigator |
Stute, Martin | Lamont-Doherty Earth Observatory (LDEO) | Co-Principal Investigator |
Rauch, Shannon | Woods Hole Oceanographic Institution (WHOI BCO-DMO) | BCO-DMO Data Manager |
Note: all methods are described in detail in the accompanying publication currently in final review at Proceedings of the National Academy of Sciences.
Samples were collected in the field at the Bermuda Atlantic Time-series (BATS) on cruise 10391 on R/V Atlantic Explorer (AE2208) from 30 April 2022 - 05 May 2022. Samples were collected at the BATS site located at 31°50'N, 64°10'W. Samples were collected in evacuated 6-liter (L) stainless steel canisters by subsampling from 12-L Niskin bottles, filling each to ~3.5 L.
Noble gas isotopes and elemental ratios were measured in the Seltzer Lab at Woods Hole Oceanographic Institution following the methods described in Seltzer and Bekaert (2022). In the lab, samples were equilibrated on a shaking table at constant temperature before being drained, leaving a headspace that was chemically gettered to remove all reactive gases. The purified sample was analyzed on a dual-inlet mass spectrometer in the Seltzer Lab for stable Argon, Krypton, and Xenon (Ar, Kr, and Xe) isotope ratios as well as Kr/Ar and Xe/Ar ratios. All samples (n=27) were analyzed between 13 May and 10 June 2022 and air standards were analyzed weekly throughout this period.
The model simulations are available as a related dataset at BCO-DMO. See: https://www.bco-dmo.org/dataset/890293
Data Processing:
All data were processed using MATLAB. Codes are available upon request.
BCO-DMO Processing:
- renamed fields to comply with BCO-DMO naming conventions;
- converted dates to YYYY-MM-DD format.
File |
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bats_measurements.csv (Comma Separated Values (.csv), 6.16 KB) MD5:82bfe8c2f1e628a2e5e4bc2ab9af3bb4 Primary data file for datset ID 890342. |
Parameter | Description | Units |
Date_Meas | Date of sample collection | unitless |
Cast | Rosette cast number on BATS cruise 10391 | unitless |
Bottle | Rosette bottle number on BATS cruise 10391 | unitless |
Depth | Sample depth | meeters (m) |
T | Sample temperature | degrees C |
S | Sample salinity | Practical Salinity Units (PSU) |
Theta | Potential temperature | degrees C |
Pres | Sample pressure | decibars (dbar) |
Flask_ID | serial number of flask | unitless |
Flask_Weight_Empty | weight of evacuated sample flask | grams (g) |
Flask_Weight_Full | weight of full flask | grams (g) |
Flask_Weight_Drained | Weight of drained flask | grams (g) |
Shaking_EQ_Temp | temperature during headspace equibration | degrees C |
Shaking_EQ_Time | equilibration time on shaker table | days |
Dissolved_gas_dvalue_40_to_36 | Dissolved gas δ values (w.r.t. air, per mil) 40/36 | permil (0/00) |
Dissolved_gas_dvalue_38_to_36 | Dissolved gas δ values (w.r.t. air, per mil) 38/36 | permil (0/00) |
Dissolved_gas_dvalue_86_to_82 | Dissolved gas δ values (w.r.t. air, per mil) 86/82 | permil (0/00) |
Dissolved_gas_dvalue_86_to_84 | Dissolved gas δ values (w.r.t. air, per mil) 86/84 | permil (0/00) |
Dissolved_gas_dvalue_136_to_129 | Dissolved gas δ values (w.r.t. air, per mil) 136/129 | permil (0/00) |
Dissolved_gas_dvalue_134_to_129 | Dissolved gas δ values (w.r.t. air, per mil) 134/129 | permil (0/00) |
Dissolved_gas_dvalue_132_to_129 | Dissolved gas δ values (w.r.t. air, per mil) 132/129 | permil (0/00) |
Dissolved_gas_dvalue_131_to_129 | Dissolved gas δ values (w.r.t. air, per mil) 131/129 | permil (0/00) |
Dissolved_gas_dvalue_130_to_129 | Dissolved gas δ values (w.r.t. air, per mil) 130/129 | permil (0/00) |
Dissolved_gas_dvalue_128_to_129 | Dissolved gas δ values (w.r.t. air, per mil) 128/129 | permil (0/00) |
Dissolved_gas_dvalue_Kr_to_Ar | Dissolved gas δ values (w.r.t. air, per mil) Kr/Ar | permil (0/00) |
Dissolved_gas_dvalue_Xe_to_Ar | Dissolved gas δ values (w.r.t. air, per mil) Xe/Ar | permil (0/00) |
Solubility_anomaly_Kr_to_Ar | Solubility Anomalies. Deviations of dissolved gas ratios from solubility equilibrium. Δ (‰) Kr/Ar | permil (0/00) |
Solubility_anomaly_Xe_to_Ar | Solubility Anomalies. Deviations of dissolved gas ratios from solubility equilibrium. Δ (‰) Xe/Ar | permil (0/00) |
Solubility_anomaly_40_to_36Ar | Solubility Anomalies. Deviations of dissolved gas ratios from solubility equilibrium. Δ (‰) 40/36Ar | permil (0/00) |
Solubility_anomaly_86_to_82Kr | Solubility Anomalies. Deviations of dissolved gas ratios from solubility equilibrium. Δ (‰) 86/82Kr | permil (0/00) |
Solubility_anomaly_136_to_129Xe | Solubility Anomalies. Deviations of dissolved gas ratios from solubility equilibrium. Δ (‰) 136/129Xe | permil (0/00) |
Solubility_equilibria_40_to_36Ar | Solubility equilibria. Deviations of solubility equilibrium ratios from air. (‰, vs air) 40/36Ar | permil (0/00) |
Solubility_equilibria_86_to_82Kr | Solubility equilibria. Deviations of solubility equilibrium ratios from air. (‰, vs air) 86/82Kr | permil (0/00) |
Solubility_equilibria_136_to_129Xe | Solubility equilibria. Deviations of solubility equilibrium ratios from air. (‰, vs air) 136/129Xe | permil (0/00) |
Dataset-specific Instrument Name | Thermo MAT 253 Plus |
Generic Instrument Name | Isotope-ratio Mass Spectrometer |
Dataset-specific Description | A Thermo MAT 253 Plus dual-inlet isotope-ratio mass spectrometer with custom 10-cup collector was used for Ar/Kr/Xe analysis. |
Generic Instrument Description | The Isotope-ratio Mass Spectrometer is a particular type of mass spectrometer used to measure the relative abundance of isotopes in a given sample (e.g. VG Prism II Isotope Ratio Mass-Spectrometer). |
Dataset-specific Instrument Name | 12-L Niskin bottles |
Generic Instrument Name | Niskin bottle |
Dataset-specific Description | Samples were collected in evacuated 6-liter (L) stainless steel canisters by subsampling from 12-L Niskin bottles. |
Generic Instrument Description | A Niskin bottle (a next generation water sampler based on the Nansen bottle) is a cylindrical, non-metallic water collection device with stoppers at both ends. The bottles can be attached individually on a hydrowire or deployed in 12, 24, or 36 bottle Rosette systems mounted on a frame and combined with a CTD. Niskin bottles are used to collect discrete water samples for a range of measurements including pigments, nutrients, plankton, etc. |
Dataset-specific Instrument Name | shaking table |
Generic Instrument Name | Shaker |
Dataset-specific Description | Samples were equilibrated on a shaking table at constant temperature. |
Generic Instrument Description | A Shaker is a piece of lab equipment used to mix, blend, or to agitate substances in tube(s) or flask(s) by shaking them, which is mainly used in the fields of chemistry and biology. A shaker contains an oscillating board which is used to place the flasks, beakers, test tubes, etc. |
Website | |
Platform | R/V Atlantic Explorer |
Start Date | 2022-04-30 |
End Date | 2022-05-05 |
Description | See more cruise information from the Rolling Deck to Repository (R2R): https://www.rvdata.us/search/cruise/AE2208 |
NSF Award Abstract:
This award is funded in whole or in part under the American Rescue Plan Act of 2021 (Public Law 117-2).
The transfer of gases between the atmosphere and the interior of ocean is controlled by processes in the high latitudes, where deep waters are “formed” by the sinking of cold and/or salty surface waters. The processes that affect air-sea gas exchange during water mass formation play an important role in the uptake of carbon dioxide and other important gases by the ocean. Dissolved noble gases, which are not affected by chemistry or biology, are excellent tracers of the physics of air-sea gas exchange: their abundances in the ocean interior tell us about how efficient gas exchange was when water was last at the sea surface. Another tracer, the “triple oxygen isotope” (TOI) composition of dissolved oxygen (a measure of the relative abundances of oxygen-16, oxygen-17, and oxygen-18) is sensitive to both biology and physics. However, each of these important tracers of air-sea exchange remains understudied in the modern ocean. This project aims to make new state-of-the-art measurements of noble gases and TOIs in 100 archived gas samples from the North and South Atlantic. The methods developed in this project will also enable future research opportunities that take advantage of these valuable samples. The project will support the training of a PhD student and multiple undergraduates, while contributing to ongoing efforts to develop workshop and lecture materials for a new partnership between Woods Hole Oceanographic Institution (WHOI) and a nearby public high school that has a primarily underrepresented minority student body.
The primary objective of this project is to quantify the magnitude and spatial variability of two sets conservative tracers that are each independently sensitive to air-sea gas exchange at the time of deep-water formation: noble gases and TOIs. A deeper understanding of these tracers will provide insight into the physical mechanisms that regulate the efficiency of deep-ocean ventilation. Over recent decades, multiple studies have consistently found undersaturation of the heavy noble gases (Ar, Kr, and Xe) in the deep ocean, with respect to their solubility equilibrium concentrations in seawater. However, while several theories exist, there is no consensus on why the heavy noble gases are undersaturated throughout the deep ocean nor any reason to suspect that a single process is responsible. The spatial variability in noble gas disequilibrium between the North and South Atlantic may provide key clues to this open question, given the vastly different mechanisms of northern and southern deep-water formation. However, to date, analytical limitations have limited the robust detection and quantification of inter water-mass differences in disequilibrium. TOIs may also provide insight into air-sea disequilibrium during deep-water formation, as the relative excess of oxygen-17 (with respect to the atmospheric oxygen isotope ratios and corrected for isotopic fractionation due to respiration) reflects the balance between air-sea exchange and photosynthesis. Together, noble gases and TOIs provide useful constraints to elucidate fundamental mechanisms. For example, sea-ice cover in regions of deep-water formation will simultaneously lead to undersaturation of noble gases and accumulation of photosynthetic oxygen (and thus excess oxygen-17). However, few high-quality measurements of TOI in the deep ocean exist, due to analytical challenges, despite the great potential of TOI as a conservative tracer of physics and biogeochemistry during deep-water formation. The proposed work will involve 100 measurements of archived dissolved gas samples that were extracted at sea in the 1980s and stored in robust tanks since collection. This project is the first effort to measure noble gases and TOI in the same deep-ocean samples across a wide spatial range, by consistently employing the same methodology and instrumentation to eliminate inter-laboratory biases. It involves measurements in three WHOI labs and makes use of state-of-the-art techniques for each independent tracer measurement. This work builds in redundancy to improve the accuracy of results by measuring all samples on multiple instruments, including pairs of adjacent stations, and carrying out extraction experiments with the original equipment used in the 1980s to collect these samples. For example, heavy noble gas elemental ratios will be measured independently on two separate instruments, and high-precision (order 0.01 permil) measurements of noble gas isotopes will be used to test and correct for sample integrity. Overall, this large set of archived gases offers a unique opportunity to better understand these tracers and explore the quantitative insight they may offer into outstanding questions about the deep-ocean ventilation.
This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.
NSF Award Abstract:
The proposed work brings together the fields of chemical oceanography, ocean modeling, and solid Earth geochemistry to develop the stable isotope composition of heavy noble gases dissolved in seawater as novel physical tracers of air-sea gas exchange. Noble gases represent ideal tools for quantifying physical processes due to the fact that they are chemically inert. Because argon (Ar), krypton (Kr), and xenon (Xe) isotope ratios have distinct solubility and diffusivity ratios, as recently quantified in laboratory experiments, they complement existing bulk noble gas measurements in seawater by adding new constraints with unique sensitivities. Precise constraints on air-sea exchange of inert gases are paramount to properly quantifying production, consumption, and physical transport of biogeochemically important gases (such as carbon dioxide and oxygen) as well as ventilation age tracers (such as sulfur hexafluoride and CFCs). Additionally, global circulation models (GCMs) routinely underestimate deep-ocean ventilation compared to noble gas observations. Introducing these new isotopic constraints into model simulations will help identify physical processes related to deep-water formation that require improvement in future GCM development. Because the overturning circulation is closely tied to projections of future climate, by both the transports of radiative gases and heat into the deep ocean, there is broad international interest in improving future model projections. Therefore, adding high-precision noble gas isotope measurements to the existing body of research on inert gases in seawater will provide valuable new constraints for both the marine biogeochemistry and physical oceanography communities. Education and training of a graduate student and postdoctoral scholar will contribute to the human resource base of the United States.
The proposed work will develop high-precision Ar, Kr, and Xe stable isotope ratios in seawater as new oceanographic tracers. Along with a 2018 pilot study, the proposed measurements represent the first high- precision Kr and Xe isotope ratio analyses in seawater. A key goal of this project is to test two specific hypotheses for the observed undersaturation of Ar, Kr, and Xe throughout the deep ocean: (1) rapid cooling-induced gas uptake by the surface ocean during deep-water formation with insufficient time for equilibration before sinking, or (2) subsurface cooling caused by melting of glacial ice, leading to the dissolution of air bubbles trapped in ice. Whereas both of these non-mutually exclusive processes produce similar patterns of heavy noble gas undersaturation, the isotope ratios of these gases are well suited to distinguish the relative importance of each process. Specifically, theoretical predictions suggest a decrease in heavy-to-light isotope ratios from the kinetic fractionation associated with rapid surface ocean gas uptake, but an increase in these ratios from the input of gravitationally enriched glacial meltwater. Other goals include: (a) comparing observations to model simulations to identify successes and shortcomings of GCM representations of deep-water formation processes, and (b) a year-long time series of surface-ocean observations from the SIO pier to test models of isotopic fractionation associated with bubble injection and upwelling, with implications for the saturation of biogeochemically important gases. This work will improve upon a recent method for dissolved noble gas isotopic analysis by increasing sample sizes and refining purification techniques to achieve a >60% improvement in precision.
This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.
Funding Source | Award |
---|---|
NSF Division of Ocean Sciences (NSF OCE) | |
NSF Division of Ocean Sciences (NSF OCE) |