Preprints
https://doi.org/10.5194/egusphere-2023-424
https://doi.org/10.5194/egusphere-2023-424
10 Mar 2023
 | 10 Mar 2023

Intense Anticyclones at the Global Argentine Basin Array of the Ocean Observatory Initiative

Camila Artana and Christine Provost

Abstract. We analyzed physical oceanic parameters gathered by a mooring array at mesoscale spatial sampling deployed in Argentine Basin within the Ocean Observatory Initiative, a National Science Foundation Major Research Facility. The array was maintained at 42° S 42° W, a historically sparsely sampled region with small ocean variability, during 34 months from March 2015 to January 2018. The data documented four anticyclonic extreme structures events in 2016. The four anticyclonic structures had different characteristics (size, vertical extension, origin, lifetime, Rossby Number). They all featured near-inertial waves (NIWs) trapped at depth and low Richardson values well below the mixed layer. Low Richardson values suggest favorable conditions for mixing. The anticyclonic features likely act as mixing structures at the pycnocline bringing heat and salt from the South Atlantic Central Water to the Antarctic Intermediate Waters. The intense structures were unique in the 29-year-long satellite altimetry record at the mooring site. The Argentine Basin is populated with many anticyclones and mixing associated to trapped NIWs probably plays an important role in setting up the upper water masses characteristics in the Basin.

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Journal article(s) based on this preprint

28 Jun 2023
Intense anticyclones at the global Argentine Basin array of the Ocean Observatory Initiative
Camila Artana and Christine Provost
Ocean Sci., 19, 953–971, https://doi.org/10.5194/os-19-953-2023,https://doi.org/10.5194/os-19-953-2023, 2023
Short summary
Camila Artana and Christine Provost

Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2023-424', Anonymous Referee #1, 26 Apr 2023
    • AC1: 'Reply on RC1', Camila Artana, 05 May 2023
    • AC2: 'Reply on RC1', Camila Artana, 22 May 2023
  • RC2: 'Comment on egusphere-2023-424', Anonymous Referee #2, 17 May 2023
    • AC3: 'Reply on RC2', Camila Artana, 22 May 2023
  • EC1: 'Comment on egusphere-2023-424', Karen J. Heywood, 22 May 2023

Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2023-424', Anonymous Referee #1, 26 Apr 2023
    • AC1: 'Reply on RC1', Camila Artana, 05 May 2023
    • AC2: 'Reply on RC1', Camila Artana, 22 May 2023
  • RC2: 'Comment on egusphere-2023-424', Anonymous Referee #2, 17 May 2023
    • AC3: 'Reply on RC2', Camila Artana, 22 May 2023
  • EC1: 'Comment on egusphere-2023-424', Karen J. Heywood, 22 May 2023

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by Camila Artana on behalf of the Authors (23 May 2023)  Author's response   Author's tracked changes   Manuscript 
ED: Publish subject to technical corrections (26 May 2023) by Karen J. Heywood
AR by Camila Artana on behalf of the Authors (27 May 2023)  Author's response   Manuscript 

Journal article(s) based on this preprint

28 Jun 2023
Intense anticyclones at the global Argentine Basin array of the Ocean Observatory Initiative
Camila Artana and Christine Provost
Ocean Sci., 19, 953–971, https://doi.org/10.5194/os-19-953-2023,https://doi.org/10.5194/os-19-953-2023, 2023
Short summary
Camila Artana and Christine Provost
Camila Artana and Christine Provost

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Latest update: 12 Sep 2024
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Short summary
In 2016 exceptional eddies visited a mooring array deployed in the Argentine Basin, a region where in situ data are scarce and ocean currents tend to be calm. The eddies had large rotating velocities and distinct physical characteristics and origins. One eddy with a radius of 100-150 km, was bottom-reaching. Two other were smaller with radius less than 40 km and depth of about 2500 m. The mooring data indicated the presence of waves trapped inside the eddies and favourable conditions for mixing.