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C.E. Rosanova

Publications and source records attributed to C.E. Rosanova.

2 recordsLinked to original sources

Velocities of the Pine Island, Thwaites, and smaller glaciers along the Marie Byrd Land coast, West Antarctica

Average velocities for time intervals ranging from < 1 to 15 years were measured by tracking ice-surface patterns on sequential Landsat and European Remote-sensing Satellite synthetic aperture radar images. Velocities ofThwaites Glacier range from 2.2 km a −1 above the grounding line to 3.4 km a −1 at the limit of measurements onThwaites Glacier ice tongue. The glacier increases in velocity by about 1 km a −1 where it crosses the grounding line. Over the period 1984-93, Thwaites Glacier ice tongue accelerated by about 0.6 kin a .Velocities of the floating part of several minor glaciers and some ice shelves are also determined: Land Glacier, 17—1.9 km a −1 ; DeVicq Glacier, 0.7-1.1 km a −1 ; Dotson Ice Shelf 0.2-0.5 km a −1 ; Gctz Ice Shelf, 0.2-0.8 km a −1 ; and Sulzberger Ice Shelf, 0.01 -0.02 km a −1 . The high velocities along the Marie Byrd Land coast are consistent with the high precipitation rates over West Antarctica and, for some of the glaciers, the lack of buttressing ice shelves.

Annals of Glaciology↗

Velocities of Pine Island and Thwaites Glaciers, West Antarctica, from ERS-1 SAR images

Average velocities of Pine Island and Thwaites Glaciers were measured for the time periods between 1992 and 1994 by tracking ice-surface patterns. Velocities of the central flow of the Pine Island Glacier range from 1.5 km/yr above the grounding line (separating the grounded from the floating parts of a glacier) to 2.8 km/yr near the terminus; velocities of the central Thwaites Glacier range from 2.2 km/yr above the grounding line to 3.4 km/yr at the limit of measurements on the tongue. Both glaciers show an increase in velocity of about 1 km/yr where they cross their grounding lines. The velocities derived from ERS-1 images are higher than those previously derived from Landsat images, perhaps reflecting acceleration of the glaciers. Both glaciers are exceptionally fast. The high velocities may be due to high precipitation rates over West Antarctica and the lack of a major buttressing ice shelf.

European Space Agency, (Special Publication) ESA S↗