TY - JOUR
T1 - Polar Cyclones at the Origin of the Reoccurrence of the Maud Rise Polynya in Austral Winter 2017
AU - Francis, Diana
AU - Eayrs, Clare
AU - Cuesta, Juan
AU - Holland, David
N1 - Funding Information:
The European Centre for Medium‐ Range Weather Forecasts (ECMWF) is acknowledged for making the meteorological analyses available from their data server (https://apps.ecmwf. int/datasets/). The National Snow and Ice Data Center (NSIDC) is acknowledged for making the satellite observations on sea ice available from their data server (https://nsidc.org/ data/icesat/data.html). The CALIPSO data used in this study are available at the website (https://www‐calipso.larc. nasa.gov/tools/data_avail/). We acknowledge the use of imagery provided by services from the Global Imagery Browse Services (GIBS), operated by NASA's Earth Science Data and Information System (ESDIS) Project. The authors wish to thank two anonymous reviewers for their valuable comments and suggestions. This research work was supported by the NYU Abu Dhabi Research Institute in the UAE, grant 1204.
Publisher Copyright:
©2019. American Geophysical Union. All Rights Reserved.
PY - 2019/5/27
Y1 - 2019/5/27
N2 - 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.
AB - 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.
KW - Antarctica
KW - cyclones
KW - cyclonic winds
KW - polynya
KW - sea ice
KW - storms
UR - http://www.scopus.com/inward/record.url?scp=85066888409&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85066888409&partnerID=8YFLogxK
U2 - 10.1029/2019JD030618
DO - 10.1029/2019JD030618
M3 - Article
AN - SCOPUS:85066888409
SN - 2169-897X
VL - 124
SP - 5251
EP - 5267
JO - Journal of Geophysical Research: Atmospheres
JF - Journal of Geophysical Research: Atmospheres
IS - 10
ER -