As one kind of submesoscale instabilities, symmetric instability (SI) with spatiotemporal scales of O (100) m–O (1) km and O (1) hour exerts significant effects on vertical material transports and forward energy cascade in the ocean. The potential vorticity (PV) is an important conservative parameter controlling quasi-geostrophic flows, whose budget can be modulated by SI. However, due to the small spatial scale of SI which is hardly resolved by most current observations and regional models, how SI affects the PV budget and how big the effect is remain unclear. In this work, the effect of SI on the PV budget in the surface mixed layer (SML) of the Kuroshio Extension region is quantitatively analyzed based on high-resolution simulations by applying an existing SI parameterization scheme. Compared with the case without SI effects, negative PV is found to be eliminated in the SML in the SI-parameterized case. The negative-PV likelihood in the SI-parameterized case is decreased by up to 12% due to SI. Analysis of the PV budget indicates that SI contributes to the PV budget mainly by modulating the friction term. The friction term tends to generate negative PV but its magnitude is decreased by 35% due to SI. Apart from the frictional term, both advection and non-adiabatic terms are also found to be modulated by SI. This work sheds light on the contribution of SI in the PV budget in the ocean mixed layer and suggests a significant role of SI in quasi-geostrophic PV dynamics.
对称不稳定性(SI)是亚中尺度不稳定的一种,其时空尺度为 O (100) m-O (1) km 和 O (1) 小时,对海洋的垂直物质输送和前向能量级联有重要影响。潜在涡度(PV)是控制准地转流的重要保守参数,其预算可由 SI 调节。然而,由于 SI 的空间尺度较小,目前大多数观测资料和区域模式都难以解决这一问题,因此 SI 如何影响 PV 预算以及影响有多大仍不清楚。本研究采用现有的 SI 参数化方案,在高分辨率模拟的基础上定量分析了 SI 对黑潮延伸区表层混合层(SML)的 PV 预算的影响。与没有 SI 效应的情况相比,发现在 SI 参数化的情况下,SML 中的负 PV 消失了。由于 SI 的影响,SI 参数化情况下的负 PV 可能性降低了 12%。对 PV 预算的分析表明,SI 主要通过调节摩擦项来增加 PV 预算。摩擦项倾向于产生负 PV,但由于 SI 的影响,其幅度减少了 35%。除了摩擦项,平流和非绝热项也受到 SI 的调节。这项研究揭示了 SI 对海洋混合层光生伏特预算的贡献,并表明 SI 在准地转营养光生伏特动力学中发挥着重要作用。
{"title":"Effects of Symmetric Instability on Potential Vorticity Budget in the Kuroshio Extension Region via a Parameterization Scheme","authors":"Shuyue Ma, Jihai Dong, Changming Dong, Zhiyou Jing","doi":"10.1029/2023JC020375","DOIUrl":"10.1029/2023JC020375","url":null,"abstract":"<p>As one kind of submesoscale instabilities, symmetric instability (SI) with spatiotemporal scales of <i>O</i> (100) m–<i>O</i> (1) km and <i>O</i> (1) hour exerts significant effects on vertical material transports and forward energy cascade in the ocean. The potential vorticity (PV) is an important conservative parameter controlling quasi-geostrophic flows, whose budget can be modulated by SI. However, due to the small spatial scale of SI which is hardly resolved by most current observations and regional models, how SI affects the PV budget and how big the effect is remain unclear. In this work, the effect of SI on the PV budget in the surface mixed layer (SML) of the Kuroshio Extension region is quantitatively analyzed based on high-resolution simulations by applying an existing SI parameterization scheme. Compared with the case without SI effects, negative PV is found to be eliminated in the SML in the SI-parameterized case. The negative-PV likelihood in the SI-parameterized case is decreased by up to 12% due to SI. Analysis of the PV budget indicates that SI contributes to the PV budget mainly by modulating the friction term. The friction term tends to generate negative PV but its magnitude is decreased by 35% due to SI. Apart from the frictional term, both advection and non-adiabatic terms are also found to be modulated by SI. This work sheds light on the contribution of SI in the PV budget in the ocean mixed layer and suggests a significant role of SI in quasi-geostrophic PV dynamics.</p>","PeriodicalId":54340,"journal":{"name":"Journal of Geophysical Research-Oceans","volume":null,"pages":null},"PeriodicalIF":3.3,"publicationDate":"2024-07-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141797678","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}
Douglas Keller Jr., Yonatan Givon, Romain Pennel, Shira Raveh-Rubin, Philippe Drobinski
Deep convection occurs periodically in the Gulf of Lion, in the northwestern Mediterranean Sea, driven by the seasonal atmospheric change and Mistral winds. To determine the variability and drivers of both forcings, multiple 1 year ocean simulations were run, spanning from 1993 to 2013. Two sets of simulations were performed: a control and seasonal set, the first forced by unfiltered atmospheric forcing and the other by filtered forcing. The filtered forcing was bandpass filtered, retaining the seasonal and intraday aspects but removing the high frequency phenomena. Comparing the two sets allows for distinguishing the effects of the high frequency component of the Mistral on the ocean response. During the preconditioning phase, the seasonal forcing was found to be the main destratifying process, removing on average 46% of the stratification needed for deep convection to occur, versus the 28% removed by the Mistral. Despite this, each forcing triggered deep convection in roughly half of the deep-convection events. Sensible and latent heat fluxes were found to be the main drivers of the seasonal forcing during deep-convection years, removing 0.17 and 0.43 m2s−2 of stratification, respectively. They were themselves driven by increased wind speeds, believed to be the low frequency signal of the Mistral, as more Mistral events occur during deep-convection winters (34% vs. 29% of the preconditioning period days). An evolving seasonal forcing in a changing climate may have significant effects on the future deep convection cycle of the western Mediterranean Sea.
{"title":"Untangling the Mistral and Seasonal Atmospheric Forcing Driving Deep Convection in the Gulf of Lion: 1993–2013","authors":"Douglas Keller Jr., Yonatan Givon, Romain Pennel, Shira Raveh-Rubin, Philippe Drobinski","doi":"10.1029/2022JC019245","DOIUrl":"10.1029/2022JC019245","url":null,"abstract":"<p>Deep convection occurs periodically in the Gulf of Lion, in the northwestern Mediterranean Sea, driven by the seasonal atmospheric change and Mistral winds. To determine the variability and drivers of both forcings, multiple 1 year ocean simulations were run, spanning from 1993 to 2013. Two sets of simulations were performed: a control and seasonal set, the first forced by unfiltered atmospheric forcing and the other by filtered forcing. The filtered forcing was bandpass filtered, retaining the seasonal and intraday aspects but removing the high frequency phenomena. Comparing the two sets allows for distinguishing the effects of the high frequency component of the Mistral on the ocean response. During the preconditioning phase, the seasonal forcing was found to be the main destratifying process, removing on average 46% of the stratification needed for deep convection to occur, versus the 28% removed by the Mistral. Despite this, each forcing triggered deep convection in roughly half of the deep-convection events. Sensible and latent heat fluxes were found to be the main drivers of the seasonal forcing during deep-convection years, removing 0.17 and 0.43 m<sup>2</sup>s<sup>−2</sup> of stratification, respectively. They were themselves driven by increased wind speeds, believed to be the low frequency signal of the Mistral, as more Mistral events occur during deep-convection winters (34% vs. 29% of the preconditioning period days). An evolving seasonal forcing in a changing climate may have significant effects on the future deep convection cycle of the western Mediterranean Sea.</p>","PeriodicalId":54340,"journal":{"name":"Journal of Geophysical Research-Oceans","volume":null,"pages":null},"PeriodicalIF":3.3,"publicationDate":"2024-07-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2022JC019245","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141845390","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}
W. C. Clemo, K. M. Dorgan, D. J. Wallace, B. Dzwonkowski
Sediment dynamics are fundamental to understanding coastal resiliency to climate change in the coming decades. Tropical cyclones can radically alter shallow sediment properties; however, the uncertain and destructive nature of tropical cyclones make understanding and predicting their impacts on sediments challenging. Here, grain size sampling in conjunction with continuous hydrodynamic data provided an unprecedented perspective of the impacts of two tropical cyclones, including Hurricane Sally (2020), in which the inner core of the storm passed directly over the field sites, on shallow coastal sediments in Alabama (USA). Sampling directly before and after Sally as well as out to ∼7 months after the second storm event, Hurricane Zeta, showed that the changes in sediments following storm events exhibited notable site-to-site variability. This variability during the first storm event was consistent with low sand supply and flow interactions driven by local bathymetry that led to sand transport and deposition at some previously-muddy sites, near-surface mud loss at some sandy sites, or little change at others. Post-Sally impacts to grain size were well preserved 8 months after the storm, despite passage of Zeta as well as seasonal winds and riverine inputs during winter and spring. Overall, high temporal-resolution sampling over a relatively large area (<500 km2) revealed relatively small-scale spatial variability (on the order of 5–10 km) of hurricane impacts to sediment structure. These observations demonstrate a critical limitation for accurately predicting changes to coastal sediment dynamics in the face of a changing climate and its impact on tropical cyclones.
{"title":"Spatially and Temporally Variable Impacts of Hurricanes on Shallow Sediment Structure","authors":"W. C. Clemo, K. M. Dorgan, D. J. Wallace, B. Dzwonkowski","doi":"10.1029/2023JC020820","DOIUrl":"10.1029/2023JC020820","url":null,"abstract":"<p>Sediment dynamics are fundamental to understanding coastal resiliency to climate change in the coming decades. Tropical cyclones can radically alter shallow sediment properties; however, the uncertain and destructive nature of tropical cyclones make understanding and predicting their impacts on sediments challenging. Here, grain size sampling in conjunction with continuous hydrodynamic data provided an unprecedented perspective of the impacts of two tropical cyclones, including Hurricane Sally (2020), in which the inner core of the storm passed directly over the field sites, on shallow coastal sediments in Alabama (USA). Sampling directly before and after Sally as well as out to ∼7 months after the second storm event, Hurricane Zeta, showed that the changes in sediments following storm events exhibited notable site-to-site variability. This variability during the first storm event was consistent with low sand supply and flow interactions driven by local bathymetry that led to sand transport and deposition at some previously-muddy sites, near-surface mud loss at some sandy sites, or little change at others. Post-Sally impacts to grain size were well preserved 8 months after the storm, despite passage of Zeta as well as seasonal winds and riverine inputs during winter and spring. Overall, high temporal-resolution sampling over a relatively large area (<500 km<sup>2</sup>) revealed relatively small-scale spatial variability (on the order of 5–10 km) of hurricane impacts to sediment structure. These observations demonstrate a critical limitation for accurately predicting changes to coastal sediment dynamics in the face of a changing climate and its impact on tropical cyclones.</p>","PeriodicalId":54340,"journal":{"name":"Journal of Geophysical Research-Oceans","volume":null,"pages":null},"PeriodicalIF":3.3,"publicationDate":"2024-07-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141839951","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}
R. K. Thomas, S. E. Fawcett, H. J. Forrer, C. M. Robinson, A. N. Knapp
The Southern Ocean is a high-nutrient, low-chlorophyll (HNLC) region characterized by incomplete nitrate (NO3−) consumption by phytoplankton in surface waters. During this incomplete consumption, phytoplankton preferentially assimilate the 14N- versus the 15N-bearing form of NO3−, quantified as the NO3− assimilation isotope effect (15ε). Previous summertime estimates of the 15ε from HNLC regions range from 4 to 11‰. While culture work has shown that the 15ε varies among phytoplankton species, as well as with light and iron stress, we lack a systematic understanding of how and why the 15ε varies in the field. Here we estimate the 15ε from water-column profile and surface-water samples collected in the Indian sector of the Southern Ocean—the first leg of the Antarctic Circumnavigation Expedition (December 2016–January 2017) and the Crossroads transect (April 2016). Consistent with prior work in the mid-to-late summer Southern Ocean, we estimate a higher 15ε (8.9 ± 0.6‰) for the northern Subantarctic Zone and a lower 15ε (5.4 ± 0.9‰) at and south of the Subantarctic Front. We interpret our data in the context of coincident measurements of phytoplankton community composition and estimates of iron and light stress. Similar to prior work, we find a significant, negative relationship between the 15ε and the average mixed-layer photosynthetically active radiation flux of 30–100 μmol m−2 s−1, while above 100 μmol m−2 s−1, 15ε increases again. In addition, while we observe no robust relationship of the 15ε to iron availability or phytoplankton community, mixed-layer nitrification over the Kerguelen Plateau appears to strongly influence its magnitude.
{"title":"Estimates of the Isotope Effect for Nitrate Assimilation in the Indian Sector of the Southern Ocean","authors":"R. K. Thomas, S. E. Fawcett, H. J. Forrer, C. M. Robinson, A. N. Knapp","doi":"10.1029/2023JC020830","DOIUrl":"10.1029/2023JC020830","url":null,"abstract":"<p>The Southern Ocean is a high-nutrient, low-chlorophyll (HNLC) region characterized by incomplete nitrate (NO<sub>3</sub><sup>−</sup>) consumption by phytoplankton in surface waters. During this incomplete consumption, phytoplankton preferentially assimilate the <sup>14</sup>N- versus the <sup>15</sup>N-bearing form of NO<sub>3</sub><sup>−</sup>, quantified as the NO<sub>3</sub><sup>−</sup> assimilation isotope effect (<sup>15</sup>ε). Previous summertime estimates of the <sup>15</sup>ε from HNLC regions range from 4 to 11‰. While culture work has shown that the <sup>15</sup>ε varies among phytoplankton species, as well as with light and iron stress, we lack a systematic understanding of how and why the <sup>15</sup>ε varies in the field. Here we estimate the <sup>15</sup>ε from water-column profile and surface-water samples collected in the Indian sector of the Southern Ocean—the first leg of the Antarctic Circumnavigation Expedition (December 2016–January 2017) and the Crossroads transect (April 2016). Consistent with prior work in the mid-to-late summer Southern Ocean, we estimate a higher <sup>15</sup>ε (8.9 ± 0.6‰) for the northern Subantarctic Zone and a lower <sup>15</sup>ε (5.4 ± 0.9‰) at and south of the Subantarctic Front. We interpret our data in the context of coincident measurements of phytoplankton community composition and estimates of iron and light stress. Similar to prior work, we find a significant, negative relationship between the <sup>15</sup>ε and the average mixed-layer photosynthetically active radiation flux of 30–100 μmol m<sup>−2</sup> s<sup>−1</sup>, while above 100 μmol m<sup>−2</sup> s<sup>−1</sup>, <sup>15</sup>ε increases again. In addition, while we observe no robust relationship of the <sup>15</sup>ε to iron availability or phytoplankton community, mixed-layer nitrification over the Kerguelen Plateau appears to strongly influence its magnitude.</p>","PeriodicalId":54340,"journal":{"name":"Journal of Geophysical Research-Oceans","volume":null,"pages":null},"PeriodicalIF":3.3,"publicationDate":"2024-07-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2023JC020830","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141846453","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}
The bottom boundary layer (BBL) dynamics play an important role in regulating the energy, momentum balance, and circulation in the shallow shelf areas. Unlike previous studies that disconnected BBL with background variable shelf circulation, we investigate the dynamic connection between the wind-driven shelf circulation and BBL dynamics, and show the spatial characteristics of BBL dynamics in response to three-dimensional (3D) heterogeneous transport over the highly variable shelf topography in the Northern South China Sea. Our process-oriented modeling study demonstrates that the mixing dynamics and upslope buoyancy transport over varying shelf topography alter the spatial variability of BBL dynamics. Driven by southwesterly upwelling-favorable winds, the along-shelf current generated a frictional upslope Ekman transport. The along-isobath pressure gradient force (