Satellite observations of upper-ocean currents in Terra Nova Bay, Antarctica

Ship and iceberg drifts, along with data from modern satellite-tracked drifting buoys, portray generally northward flow in the southwest Ross Sea. Less is known, however, about the ocean variability in this region. Here we use Defense Meteorological Satellite Program (DMSP) Operational Linescan Syst...

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Bibliographic Details
Main Authors: van Woert, Michael, Meier, Walter, Zou, Cheng-Zhi, Archer, Andy, Pellegrini, Andrea, Grigioni, Paola, Bertoia, Cheryl
Format: Text
Language:unknown
Published: DigitalCommons@University of Nebraska - Lincoln 2001
Subjects:
Environmental Sciences
Ross Sea
Terra Nova Bay
Antarc*
Antarctica
Online Access:https://digitalcommons.unl.edu/usdeptcommercepub/74
https://digitalcommons.unl.edu/context/usdeptcommercepub/article/1063/viewcontent/Bertoia_AG_2001_Satellite_observations.pdf
Description
Summary:Ship and iceberg drifts, along with data from modern satellite-tracked drifting buoys, portray generally northward flow in the southwest Ross Sea. Less is known, however, about the ocean variability in this region. Here we use Defense Meteorological Satellite Program (DMSP) Operational Linescan System (OLS) imagery to describe a cyclonically rotating gyre in Terra Nova Bay, Antarctica (75° S, 165° E). The image sequence is taken from an exceptionally clear, calm, period during winter 1998. Surface currents, derived from tracking drifting ice with a maximum cross-correlation algorithm, were found to be ~20 to 30 cm s-1. Based on scaling arguments, the observed currents appear to be best explained as an oceanic response to a rapidly changing, offshore, katabatic wind jet.

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