Meteoric, marine and total ice thickness maps of Filchner-Ronne-Schelfeis, Antarctica H. Sandhäger

The Water Ice Subsurface Deposit Observation on Mars (WISDOM) ground-penetrating radar has been designed to provide infor- mation about the nature of the shallow subsurface over

Forsberg and Skourup [25] used an improved Arctic geoid model and ICESat laser altimeter measurements to find sea-ice freeboard height using a coarse “lowest-level” surface

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Figure 5: The observed data of ice thickness and ice drift speed based on upward looking sonar (ULS) and acoustic Doppler current profilers (ADCP) during 2010-2017. The

Using the values of ridging parameters defined in section 3.2 (assuming they are constant for the entire area), and in combination with ice concentration and level ice thickness

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