Polar Cyclones at the Origin of the Reoccurrence of the Maud Rise Polynya in Austral Winter 2017

Diana Karam Francis, Clare Eayrs, Juan Cuesta, David Holland

Research output: Contribution to journalArticle

Abstract

This study examines the role of atmospheric forcings in the occurrence of open-ocean polynyas by investigating the case of the austral winter 2017's polynya located in the Lazarev Sea sector to the east of the Weddell Sea, known as the Maud Rise polynya or the Weddell Polynya. The ice-free zone appeared in mid-September 2017 and grew to as large as 80,000 km2 by the end of October 2017 before merging with the open ocean after the sea ice started to retreat at the beginning of the austral summer. Using a combination of satellite observations and reanalysis data at high spatiotemporal resolution, we found that severe cyclones, occurring over the ice pack, have a deterministic role in creating strong divergence in the sea ice field through strong cyclonic surface winds leading to the opening of the polynya. The occurrence of intense and frequent cyclones over the ice pack during austral winter 2017 was unusual, and it occurred under an enhanced strong positive meridional transport of heat flux and moisture toward Antarctica associated with an amplification of the atmospheric zonal wave 3 and a strong positive Southern Annular Mode index. We found that the opening of the polynya was not primarily due to direct ice melt by thermodynamic effects but rather to strong dynamical forcing by the winds on the sea ice, as in the case of coastal polynyas. Indeed, the meridional transport of heat toward Antarctica occurred over the Weddell Sea sector (i.e., to the east of the Lazarev Sea sector where the polynya is located) whereas the Lazarev Sea sector was under the influence of equatorward transport of cold air masses at that time. Our results show that the supply of warm and moist air coming from the west side of the South Atlantic Ocean into the Weddell Sea significantly increased the potential for cyclone formation as measured by the Eady growth rate leading to intense and frequent cyclogenesis over the ice pack, far south from the ice edge. After cyclogenesis in the Weddell Sea, these cyclones intensified as they moved eastward spinning over the Lazarev Sea with intensity comparable to category 11—violent storms—in the Beaufort scale. The cyclonic winds generated sea ice divergence by pushing the ice away from the cyclone center: To the east, north of it and to the west, south of it, which led to the reoccurrence of the Maud Rise polynya in mid-September 2017.

Original languageEnglish (US)
Pages (from-to)5251-5267
Number of pages17
JournalJournal of Geophysical Research: Atmospheres
Volume124
Issue number10
DOIs
StatePublished - May 27 2019

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polynya
cyclones
Ice
sea ice
cyclone
winter
ice
Sea ice
polynyas
sectors
cyclogenesis
Antarctic regions
open ocean
divergence
oceans
occurrences
Antarctica
ice field
Atlantic Ocean
pushing

Keywords

  • Antarctica
  • cyclones
  • cyclonic winds
  • polynya
  • sea ice
  • storms

ASJC Scopus subject areas

  • Geophysics
  • Forestry
  • Oceanography
  • Aquatic Science
  • Ecology
  • Water Science and Technology
  • Soil Science
  • Geochemistry and Petrology
  • Earth-Surface Processes
  • Atmospheric Science
  • Earth and Planetary Sciences (miscellaneous)
  • Space and Planetary Science
  • Palaeontology

Cite this

Polar Cyclones at the Origin of the Reoccurrence of the Maud Rise Polynya in Austral Winter 2017. / Francis, Diana Karam; Eayrs, Clare; Cuesta, Juan; Holland, David.

In: Journal of Geophysical Research: Atmospheres, Vol. 124, No. 10, 27.05.2019, p. 5251-5267.

Research output: Contribution to journalArticle

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