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Formation of sea ice ponds from ice-shelf runoff, adjacent to the McMurdo Ice Shelf, Antarctica

Published online by Cambridge University Press:  11 March 2020

Grant J. Macdonald*
Affiliation:
Department of the Geophysical Sciences, University of Chicago, Chicago, IL, USA
Predrag Popović
Affiliation:
Department of the Geophysical Sciences, University of Chicago, Chicago, IL, USA
David P. Mayer
Affiliation:
United States Geological Survey, Astrogeology Science Center, Flagstaff, AZ, USA
*
Author for correspondence: Grant J. Macdonald, E-mail: gjmacdonald@uchicago.edu
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Abstract

Ponds that form on sea ice can cause it to thin or break-up, which can promote calving from an adjacent ice shelf. Studies of sea ice ponds have predominantly focused on Arctic ponds formed by in situ melting/ponding. Our study documents another mechanism for the formation of sea ice ponds. Using Landsat 8 and Sentinel-2 images from the 2015–16 to 2018–19 austral summers, we analyze the evolution of sea ice ponds that form adjacent to the McMurdo Ice Shelf, Antarctica. We find that each summer, meltwater flows from the ice shelf onto the sea ice and forms large (up to 9 km2) ponds. These ponds decrease the sea ice's albedo, thinning it. We suggest the added mass of runoff causes the ice to flex, potentially promoting sea-ice instability by the ice-shelf front. As surface melting on ice shelves increases, we suggest that ice-shelf surface hydrology will have a greater effect on sea-ice stability.

Information

Type
Letter
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited.
Copyright
Copyright © The Author(s) 2020
Figure 0

Fig. 1. Part of the McMIS and McMurdo Sound sea ice (green star in top-left inset shows location in Antarctica). The background image is a true-color composite Sentinel-2B image dated 4 January 2019. The white line marks the boundary between the portion of the McMIS where there is an active surface hydrology during the summer, and the portion where there is typically no surface hydrology. The black line marks the boundary between the ice shelf and sea ice. The yellow box marks the study area and extent of the images in Figure 2. Sea ice ponds are visible close to the ice-shelf front adjacent to the ‘active surface hydrology’ portion of the McMIS.

Figure 1

Fig. 2. The development of sea ice ponds adjacent to the ‘active surface hydrology’ portion of the McMIS in the (a) 2015–16 and (b) 2018–19 austral summers. The extent of each image is shown in Figure 1. The complete time series of all 32 images acquired from 29 November 2015 to 24 January 2019 can be seen in Video S1.

Figure 2

Fig. 3. Total ponded area in the study area during each melt season of the study period (2015–16 to 2018–19).

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