Soumyadeep Dutta, P. Sabu, Aditya Narayanan, Rahul Mohan
Polynyas are within the sea ice cover, typically formed by wind-driven sea ice divergence or upwelling of warm subsurface waters. They play a crucial role in ocean-atmosphere interactions, climate regulation and marine ecosystems by substantially enhancing primary production. Open-ocean polynyas in the Southern Ocean are rare and are typically associated with deep convection, which disrupts conventional circulation pathways and impacts regional heat and carbon budgets. The Cosmonauts Sea (30°E–60°E) is an exception, with open-ocean polynyas forming annually. Using satellite-derived sea ice observations, we examined the spatiotemporal variability of polynyas in this region over the past two decades. The Cosmonauts Sea polynya exhibited large spatial and interannual variability, with the largest event occurring in 2016 (139,000 km2). An Argo float near the polynya recorded deep mixed layers (>400 m) and near-complete erosion of stratification, and the presence of dense water. This event coincided with anomalously intense cyclonic wind stress curl due to synoptic scale storms and a prolonged positive Southern Annular Mode (SAM) phase (2014–2016), both generally associated with reduced sea ice concentrations. While the southward shift of the Antarctic Circumpolar Current (ACC) during 2015 acted as a preconditioning mechanism, bringing warmer water towards the polynya region and inducing upwelling by vortex stretching. Additionally, anomalously high shortwave radiative fluxes (∼+20 Wm−2) were observed in the summer preceding the 2016 event. The deep convective mixing observed during this event, together with the presence of dense water, indicates that the Cosmonauts Sea could be a potential dense water formation site.
{"title":"Characteristics of an Annually Recurring Open-Ocean Polynya in the Southern Ocean","authors":"Soumyadeep Dutta, P. Sabu, Aditya Narayanan, Rahul Mohan","doi":"10.1029/2025JC022821","DOIUrl":"https://doi.org/10.1029/2025JC022821","url":null,"abstract":"<p>Polynyas are within the sea ice cover, typically formed by wind-driven sea ice divergence or upwelling of warm subsurface waters. They play a crucial role in ocean-atmosphere interactions, climate regulation and marine ecosystems by substantially enhancing primary production. Open-ocean polynyas in the Southern Ocean are rare and are typically associated with deep convection, which disrupts conventional circulation pathways and impacts regional heat and carbon budgets. The Cosmonauts Sea (30°E–60°E) is an exception, with open-ocean polynyas forming annually. Using satellite-derived sea ice observations, we examined the spatiotemporal variability of polynyas in this region over the past two decades. The Cosmonauts Sea polynya exhibited large spatial and interannual variability, with the largest event occurring in 2016 (139,000 km<sup>2</sup>). An Argo float near the polynya recorded deep mixed layers (>400 m) and near-complete erosion of stratification, and the presence of dense water. This event coincided with anomalously intense cyclonic wind stress curl due to synoptic scale storms and a prolonged positive Southern Annular Mode (SAM) phase (2014–2016), both generally associated with reduced sea ice concentrations. While the southward shift of the Antarctic Circumpolar Current (ACC) during 2015 acted as a preconditioning mechanism, bringing warmer water towards the polynya region and inducing upwelling by vortex stretching. Additionally, anomalously high shortwave radiative fluxes (∼+20 Wm<sup>−2</sup>) were observed in the summer preceding the 2016 event. The deep convective mixing observed during this event, together with the presence of dense water, indicates that the Cosmonauts Sea could be a potential dense water formation site.</p>","PeriodicalId":54340,"journal":{"name":"Journal of Geophysical Research-Oceans","volume":"131 1","pages":""},"PeriodicalIF":3.4,"publicationDate":"2026-01-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146096503","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Changjie Dong, Quanrui Chen, Shujing Liu, Nianzhi Jiao, Kai Tang
While the importance of organic sulfur for marine bacteria is widely recognized, how it relates to bacterial community composition, particularly in coastal environments, remains poorly understood. In this study, we quantified dissolved organic sulfur (DOS) and particulate organic sulfur (POS) in the Bohai and Yellow Seas. DOS ranged from 1.7 to 6.8 μM in surface waters and 0.9–5.4 μM in bottom waters, while POS ranged from 0.3 to 1.7 μM in surface waters and 0.2–1.6 μM in bottom waters. In the Bohai Sea, particulate and dissolved C:S ratios averaged 57 ± 38 and 41.4 ± 7.5, respectively, with minimum sulfur inventories of 0.039 ± 0.025 (POS) and 0.300 ± 0.058 Tg S (DOS). In contrast, the Yellow Sea had a lower particulate C:S ratio (25 ± 17) but a comparable dissolved ratio (46.5 ± 12.5), alongside minimum inventories of 1.14 ± 0.69 (POS) and 1.91 ± 0.52 Tg S (DOS). In contrast to previously reported data from the open ocean, the Bohai and Yellow Seas are characterized by distinctly higher organic sulfur concentrations and lower molar C:S ratios. Bacterial communities differed significantly between surface and bottom waters in terms of diversity and network complexity. However, path analysis showed no significant association of organic sulfur with bacterial community composition in either layer. These findings suggest that despite high total organic sulfur concentrations in these coastal waters, its low concentration of bioavailable fractions and taxon-specific utilization may explain its limited association with bacterial community.
{"title":"Spatial Patterns of Organic Sulfur and Its Limited Association With Bacterial Communities in the Bohai and Yellow Seas","authors":"Changjie Dong, Quanrui Chen, Shujing Liu, Nianzhi Jiao, Kai Tang","doi":"10.1029/2025JC023819","DOIUrl":"https://doi.org/10.1029/2025JC023819","url":null,"abstract":"<p>While the importance of organic sulfur for marine bacteria is widely recognized, how it relates to bacterial community composition, particularly in coastal environments, remains poorly understood. In this study, we quantified dissolved organic sulfur (DOS) and particulate organic sulfur (POS) in the Bohai and Yellow Seas. DOS ranged from 1.7 to 6.8 μM in surface waters and 0.9–5.4 μM in bottom waters, while POS ranged from 0.3 to 1.7 μM in surface waters and 0.2–1.6 μM in bottom waters. In the Bohai Sea, particulate and dissolved C:S ratios averaged 57 ± 38 and 41.4 ± 7.5, respectively, with minimum sulfur inventories of 0.039 ± 0.025 (POS) and 0.300 ± 0.058 Tg S (DOS). In contrast, the Yellow Sea had a lower particulate C:S ratio (25 ± 17) but a comparable dissolved ratio (46.5 ± 12.5), alongside minimum inventories of 1.14 ± 0.69 (POS) and 1.91 ± 0.52 Tg S (DOS). In contrast to previously reported data from the open ocean, the Bohai and Yellow Seas are characterized by distinctly higher organic sulfur concentrations and lower molar C:S ratios. Bacterial communities differed significantly between surface and bottom waters in terms of diversity and network complexity. However, path analysis showed no significant association of organic sulfur with bacterial community composition in either layer. These findings suggest that despite high total organic sulfur concentrations in these coastal waters, its low concentration of bioavailable fractions and taxon-specific utilization may explain its limited association with bacterial community.</p>","PeriodicalId":54340,"journal":{"name":"Journal of Geophysical Research-Oceans","volume":"131 1","pages":""},"PeriodicalIF":3.4,"publicationDate":"2026-01-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146091354","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Dong Jian, Xiaoming Zhai, David P. Stevens, Ian A. Renfrew
The poleward warm Atlantic Water and returning cold water in the Nordic Seas play a crucial role in regulating the Northern Hemisphere climate. While previous studies have recognized the importance of mesoscale dynamics, a quantitative assessment of the role of mesoscale eddies in poleward heat transport is lacking. Our study investigates the role of eddies in poleward oceanic heat transport in the Nordic Seas using an ocean model where eddies are well represented. Using a novel configuration of the MITgcm ocean-ice model, we analyze 21 years of simulation. We show that eddy heat flux divergence offsets more than 70% of heat flux convergence induced by the mean flow along the Norwegian Atlantic Slope Current. Eddy heat flux divergence peaks at a depth of about 400 m near the thermocline and reaches a maximum near the steep Lofoten Escarpment. A temporal decomposition reveals that eddy heat flux divergence is stable on interannual timescales, although there is strong seasonality. Our study emphasizes the significant role of eddies in reducing poleward heat transport by diverting heat out of the Norwegian Atlantic Current into the Nordic Seas.
{"title":"Oceanic Heat Transport Along the Norwegian Atlantic Slope Current and the Role of Eddies","authors":"Dong Jian, Xiaoming Zhai, David P. Stevens, Ian A. Renfrew","doi":"10.1029/2025JC022960","DOIUrl":"https://doi.org/10.1029/2025JC022960","url":null,"abstract":"<p>The poleward warm Atlantic Water and returning cold water in the Nordic Seas play a crucial role in regulating the Northern Hemisphere climate. While previous studies have recognized the importance of mesoscale dynamics, a quantitative assessment of the role of mesoscale eddies in poleward heat transport is lacking. Our study investigates the role of eddies in poleward oceanic heat transport in the Nordic Seas using an ocean model where eddies are well represented. Using a novel configuration of the MITgcm ocean-ice model, we analyze 21 years of simulation. We show that eddy heat flux divergence offsets more than 70% of heat flux convergence induced by the mean flow along the Norwegian Atlantic Slope Current. Eddy heat flux divergence peaks at a depth of about 400 m near the thermocline and reaches a maximum near the steep Lofoten Escarpment. A temporal decomposition reveals that eddy heat flux divergence is stable on interannual timescales, although there is strong seasonality. Our study emphasizes the significant role of eddies in reducing poleward heat transport by diverting heat out of the Norwegian Atlantic Current into the Nordic Seas.</p>","PeriodicalId":54340,"journal":{"name":"Journal of Geophysical Research-Oceans","volume":"131 1","pages":""},"PeriodicalIF":3.4,"publicationDate":"2026-01-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1029/2025JC022960","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146096502","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
C. W. Fairall, Elizabeth J. Thompson, Ludovic Bariteau, Gary A. Wick, Peter J. Minnett, Malgorzata Szczodrak, Andrew T. Jessup, Carson Witte
This paper presents physics improvements to the cool skin parameterization in the Coupled Ocean-Atmosphere Response Experiment (COARE) bulk flux algorithm. The principal improvement is adopting a specification of the ocean side mixing profile that combines molecular and turbulent diffusivities via a form that allows turbulent dissipation to suppress turbulence near the interface. The turbulence is also scaled with the viscous friction velocity, since the stress input to waves is not realized continuously as turbulence at the interface but only intermittently at localized regions where the waves are breaking. Additional improvements include adopting a newer specification of the solar absorption profile in the ocean and incorporating the impacts of the rain sensible heat flux. The new parameterization is tuned to published observations of cool skin from a series of cruises and a recent publication of the turbo-molecular mixing term deduced for observations of gas fluxes. Data from three recent ship-based field programs, particularly the Propagation of Intraseasonal Oscillations in the Maritime Continent Region (PISTON) experiment, with radiometric sea surface and floating near-surface temperature sensors as well as high-quality air-sea flux measurements were analyzed to evaluate the model. The improvements led to modest decreases in the nonsolar cool skin (∼16%) and in the solar heating contribution, both principally in light winds. The new model better reproduced mean nighttime cool skin amplitudes and was somewhat better than the previous COARE v3.6 model at reproducing the mean diurnal cycle. Overall, cool skin predictions for a large cruise database were reduced by ∼0.01°C.
{"title":"An Updated Treatment of the Oceanic Cool Skin in the COARE Bulk Flux Algorithm","authors":"C. W. Fairall, Elizabeth J. Thompson, Ludovic Bariteau, Gary A. Wick, Peter J. Minnett, Malgorzata Szczodrak, Andrew T. Jessup, Carson Witte","doi":"10.1029/2025JC023539","DOIUrl":"https://doi.org/10.1029/2025JC023539","url":null,"abstract":"<p>This paper presents physics improvements to the cool skin parameterization in the Coupled Ocean-Atmosphere Response Experiment (COARE) bulk flux algorithm. The principal improvement is adopting a specification of the ocean side mixing profile that combines molecular and turbulent diffusivities via a form that allows turbulent dissipation to suppress turbulence near the interface. The turbulence is also scaled with the viscous friction velocity, since the stress input to waves is not realized continuously as turbulence at the interface but only intermittently at localized regions where the waves are breaking. Additional improvements include adopting a newer specification of the solar absorption profile in the ocean and incorporating the impacts of the rain sensible heat flux. The new parameterization is tuned to published observations of cool skin from a series of cruises and a recent publication of the turbo-molecular mixing term deduced for observations of gas fluxes. Data from three recent ship-based field programs, particularly the Propagation of Intraseasonal Oscillations in the Maritime Continent Region (PISTON) experiment, with radiometric sea surface and floating near-surface temperature sensors as well as high-quality air-sea flux measurements were analyzed to evaluate the model. The improvements led to modest decreases in the nonsolar cool skin (∼16%) and in the solar heating contribution, both principally in light winds. The new model better reproduced mean nighttime cool skin amplitudes and was somewhat better than the previous COARE v3.6 model at reproducing the mean diurnal cycle. Overall, cool skin predictions for a large cruise database were reduced by ∼0.01°C.</p>","PeriodicalId":54340,"journal":{"name":"Journal of Geophysical Research-Oceans","volume":"131 1","pages":""},"PeriodicalIF":3.4,"publicationDate":"2026-01-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1029/2025JC023539","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146091471","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
This study provides a comprehensive assessment of the spatial and temporal variability of euphotic zone depth (Zeu) across the Arabian Sea from 1998 to 2023, focusing on three sub-regions: the Northern Arabian Sea (NAS), South Eastern Arabian Sea (SEAS), and South Western Arabian Sea (SWAS), using satellite-derived data sets. The analysis reveals that Zeu variability occurs on interannual, intra-annual, and decadal timescales. Annual mean Zeu values across the basin ranges from 6 to 80 m, reflecting considerable spatial heterogeneity in water clarity. Regionally, NAS recorded Zeu values ranging from ∼10 to 62 m, SEAS from ∼10 to 74 m, and SWAS from ∼12 to 72 m. Empirical Orthogonal Function (EOF) analysis confirmed that interannual variability accounts for 21.57% of the total variance. Interannual variability is primarily modulated by the Indian Ocean Dipole (IOD), followed by the El Niño–Southern Oscillation (ENSO), particularly in the SEAS and SWAS regions. Zeu in the NAS showed a significant lagged response, with Principal Component (PC1) lagging Dipole Mode Index (DMI) and ENSO by approximately 10 and 8 months, respectively. A statistically significant positive trend in Zeu was observed across the basin and within all three sub-regions, with the NAS exhibiting the strongest increase. Seasonal trend analysis showed increasing Zeu trends across all seasons, with the NAS during the ON (October–November) season demonstrating the highest trend (0.47 m/year). Overall, this work offers the first detailed analysis of Zeu variability in the Arabian Sea using multi-sensor satellite data.
{"title":"Variability of Euphotic Zone Depth in the Arabian Sea Over the Period 1998–2023","authors":"Francis Shincy, R. Mani Murali, P. J. Vidya","doi":"10.1029/2025JC023204","DOIUrl":"https://doi.org/10.1029/2025JC023204","url":null,"abstract":"<p>This study provides a comprehensive assessment of the spatial and temporal variability of euphotic zone depth (Zeu) across the Arabian Sea from 1998 to 2023, focusing on three sub-regions: the Northern Arabian Sea (NAS), South Eastern Arabian Sea (SEAS), and South Western Arabian Sea (SWAS), using satellite-derived data sets. The analysis reveals that Zeu variability occurs on interannual, intra-annual, and decadal timescales. Annual mean Zeu values across the basin ranges from 6 to 80 m, reflecting considerable spatial heterogeneity in water clarity. Regionally, NAS recorded Zeu values ranging from ∼10 to 62 m, SEAS from ∼10 to 74 m, and SWAS from ∼12 to 72 m. Empirical Orthogonal Function (EOF) analysis confirmed that interannual variability accounts for 21.57% of the total variance. Interannual variability is primarily modulated by the Indian Ocean Dipole (IOD), followed by the El Niño–Southern Oscillation (ENSO), particularly in the SEAS and SWAS regions. Zeu in the NAS showed a significant lagged response, with Principal Component (PC1) lagging Dipole Mode Index (DMI) and ENSO by approximately 10 and 8 months, respectively. A statistically significant positive trend in Zeu was observed across the basin and within all three sub-regions, with the NAS exhibiting the strongest increase. Seasonal trend analysis showed increasing Zeu trends across all seasons, with the NAS during the ON (October–November) season demonstrating the highest trend (0.47 m/year). Overall, this work offers the first detailed analysis of Zeu variability in the Arabian Sea using multi-sensor satellite data.</p>","PeriodicalId":54340,"journal":{"name":"Journal of Geophysical Research-Oceans","volume":"131 1","pages":""},"PeriodicalIF":3.4,"publicationDate":"2026-01-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146099346","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
L. Ibáñez-Tejero, R. Somavilla, L. Valdés, E. Marcos, A. Viloria, A. Lavín
Zooplanktonic organisms are considered a key link between different trophic levels. The ecosystem structure and dynamics are affected by changes in their population and phenology. In this work, the causes and timing of changes within the seasonal cycle of zooplankton biomass vertical distribution in oceanic waters of the Bay of Biscay were investigated. For this purpose, long-term oceanographic time-series from zooplankton nets and high-frequency Acoustic Doppler Current Profiler backscattering data, employed as a proxy for zooplankton biomass, were used. This combination enables the observation of the concurrence of a strong seasonality in zooplankton biomass and its daily oscillation tightly linked to phytoplankton stock and its vertical distribution in relation to water column stability and air–sea forcing. During the spring bloom, when food availability is guaranteed, an increase in zooplankton biomass is observed and it is concentrated at the ocean surface, with a reduction in its diel vertical migration. Later in the year, zooplankton biomass is concentrated above the deep chlorophyll maximum (DCM), and the depth range that it occupied is increased or reduced as the DCM deepens or shoals.
{"title":"Acoustic Observations Unveil Seasonal Fluctuations and Regulation of Zooplankton Biomass and Its Vertical Distribution at a Mid-Latitude Long-Term Ocean Observatory","authors":"L. Ibáñez-Tejero, R. Somavilla, L. Valdés, E. Marcos, A. Viloria, A. Lavín","doi":"10.1029/2024JC021987","DOIUrl":"https://doi.org/10.1029/2024JC021987","url":null,"abstract":"<p>Zooplanktonic organisms are considered a key link between different trophic levels. The ecosystem structure and dynamics are affected by changes in their population and phenology. In this work, the causes and timing of changes within the seasonal cycle of zooplankton biomass vertical distribution in oceanic waters of the Bay of Biscay were investigated. For this purpose, long-term oceanographic time-series from zooplankton nets and high-frequency Acoustic Doppler Current Profiler backscattering data, employed as a proxy for zooplankton biomass, were used. This combination enables the observation of the concurrence of a strong seasonality in zooplankton biomass and its daily oscillation tightly linked to phytoplankton stock and its vertical distribution in relation to water column stability and air–sea forcing. During the spring bloom, when food availability is guaranteed, an increase in zooplankton biomass is observed and it is concentrated at the ocean surface, with a reduction in its diel vertical migration. Later in the year, zooplankton biomass is concentrated above the deep chlorophyll maximum (DCM), and the depth range that it occupied is increased or reduced as the DCM deepens or shoals.</p>","PeriodicalId":54340,"journal":{"name":"Journal of Geophysical Research-Oceans","volume":"131 1","pages":""},"PeriodicalIF":3.4,"publicationDate":"2026-01-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1029/2024JC021987","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146057969","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
E. J. Rainville, Jim Thomson, Melissa Moulton, Morteza Derakhti
Free-drifting buoyant objects, including plastics, marine debris, and organisms, move with the wind, waves, and surface currents. These objects also surf on breaking waves; this process adds to the total transport of the objects and can control beaching. Observations of surfing transport are made using small free-drifting buoys called microSWIFTs. The drifters are deployed nearshore at the US Army Corps of Engineers Field Research Facility in Duck, NC, USA, as part of the During Nearshore Events Experiment in October 2021. Surfing events are observed in the drift trajectories of the buoys as “jumps” in the time series of cross-shore position. There are 3,172 surfing events observed, with a median jump amplitude of 8.3 m and a median duration of 2.5 s. These median values are 13