4.6 Review

Malvinas current at 44.7°S: First assessment of velocity temporal variability from in situ data

Journal

PROGRESS IN OCEANOGRAPHY
Volume 195, Issue -, Pages -

Publisher

PERGAMON-ELSEVIER SCIENCE LTD
DOI: 10.1016/j.pocean.2021.102592

Keywords

Malvinas current variability; In situ time series; Satellite altimetry data; Patagonian slope

Categories

Funding

  1. Prefetcura Naval Argentina
  2. Servicio de Hidrografia Naval
  3. SHN
  4. Mincyt
  5. INIDEP
  6. CONICET
  7. UBA
  8. Prefectura Naval Argentina
  9. Puerto Deseado crew
  10. CNRS
  11. Sorbonne Universite LOCEAN
  12. LOPS
  13. DTINSU
  14. ONR Global [12275382]
  15. InterAmerican Institute for Global Change Research through NSF grant [CRN3070, GEO1128040]
  16. CONICET, Argentina

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The study reports current meter measurements obtained by four moorings deployed across the Malvinas Current (MC) at 44.7 degrees S over 18 months. The results suggest that the MC flow variability is affected by sea level anomalies (SLA) and the interaction between mesoscale features and complex bathymetry may enhance the generation and propagation of SLAs.
We report current meter measurements obtained by four moorings deployed across the Malvinas Current (MC) at 44.7 degrees S during 18 months between December 2015-June 2017. Previous measurements of the MC strength have been reported only close to the Brazil-Malvinas Confluence, hindering the interpretation of the flow variability. The record-length time averaged velocities and variance ellipses indicate a strong northward along-isobath. The MC flow is dominated by its barotropic component. The meridional velocities at the western and eastern moorings are not correlated and show large amplitude oscillations which are coherent with the passage of mesoscale features over the moorings. Satellite altimetry data, that are highly correlated with 20-day low-pass filtered in situ velocities (r similar to 0.80), show that the MC variability is affected by the propagation of sea level anomalies (SLA) along the Patagonian slope with phase speeds that range between 0.21 +/- 0.04 m s(-1) and 0.14 +/- 0.01 m s(-1). SLAs propagate northward along the slope following contours of constant planetary potential vorticity and its phase speeds decrease towards the east along the slope. SLA arriving at 44.7 degrees S originate near the North Scotia Ridge and along the Malvinas Escarpment, along the northern edge of the Malvinas Plateau. We suggest that the interaction between mesoscale features and the complex bathymetry at those locations generate instabilities that enhance the generation of SLAs that propagate in the flow direction along the western boundary of the Argentine Basin and affect the variability of the MC velocities observed at 44.7 degrees S.

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