Abstract

The giant tabular iceberg A68 broke away from the Larsen C Ice Shelf, Antarctic Peninsula, in July 2017. The evolution of A68 would have been affected by both the Larsen C Ice Shelf, the surrounding sea ice, and the nearby shallow seafloor. In this study, we analyze the initial evolution of iceberg A68A—the largest originating from A68—in terms of changes in its area, drift speed, rotation, and freeboard using Sentinel-1 synthetic aperture radar (SAR) images and CryoSat-2 SAR/Interferometric Radar Altimeter observations. The area of iceberg A68A sharply decreased in mid-August 2017 and mid-May 2018 via large calving events. In September 2018, its surface area increased, possibly due to its longitudinal stretching by melting of surrounding sea ice. The decrease in the area of A68A was only 2% over 1.5 years. A68A was relatively stationary until mid-July 2018, while it was surrounded by the Larsen C Ice Shelf front and a high concentration of sea ice, and when its movement was interrupted by the shallow seabed. The iceberg passed through a bay-shaped region in front of the Larsen C Ice Shelf after July 2018, showing a nearly circular motion with higher speed and greater rotation. Drift was mainly inherited from its rotation, because it was still located near the Bawden Ice Rise and could not pass through by the shallow seabed. The freeboard of iceberg A68A decreased at an average rate of −0.80 ± 0.29 m/year during February–November 2018, which could have been due to basal melting by warm seawater in the Antarctic summer and increasing relative velocity of iceberg and ocean currents in the winter of that year. The freeboard of the iceberg measured using CryoSat-2 could represent the returned signal from the snow surface on the iceberg. Based on this, the average rate of thickness change was estimated at −12.89 ± 3.34 m/year during the study period considering an average rate of snow accumulation of 0.82 ± 0.06 m/year predicted by reanalysis data from the Modern-Era Retrospective analysis for Research and Applications, version 2 (MERRA-2). The results of this study reveal the initial evolution mechanism of iceberg A68A, which cannot yet drift freely due to the surrounding terrain and sea ice.

Highlights

  • An iceberg is a freely floating mass of ice calved from a glacier, ice shelf, or larger iceberg

  • In several Sentinel-1 synthetic aperture radar (SAR) images obtained in summer, iceberg A68A appeared as dark as the surrounding sea ice due to snowfall or ice surface melting and would not be delineated correctly by the automatic detection techniques

  • This was likely caused by error in the visual digitization of SAR images or by an actual increase in surface area due to the longitudinal stretching of the iceberg

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Summary

Introduction

An iceberg is a freely floating mass of ice calved from a glacier, ice shelf, or larger iceberg. Satellite microwave scatterometers can observe the whole of Antarctica daily, but the spatial resolution of data generated is several tens of kilometers [12,13], which is not enough to observe changes in icebergs in detail. Using synthetic aperture radar (SAR), which provides higher spatial resolution data, a detailed analysis of even small changes in icebergs is possible. Moctezuma-Flores and Parimiggiani [16] analyzed the drift characteristics of iceberg C33 calved from the Nansen Ice Shelf, East Antarctica, using Sentinel-1 SAR images shortly after the ice shelf collapsed. Li et al [17] observed the evolution of the tabular icebergs C28A and C28B between 2010 and 2012 using ENVISAT Advanced Synthetic Aperture Radar (ASAR) images, which originated from the Mertz Ice Tongue in East Antarctica

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