Radio-echo sounding is a powerful geophysical technique for directly characterizing the subsurface conditions of terrestrial and planetary ice masses at the local, regional and global scales. As a result, a wide array of orbital, airborne, towed and in situ instruments, platforms and data analysis approaches for radar sounding have been developed, applied or proposed. Terrestrially, airborne radar-sounding data have been used in physical glaciology to observe ice thickness, basal topography and englacial layers for more than five decades. More recently, radar-sounding data have also been exploited to estimate the extent and configuration of subglacial water, the ice-sheet surface, the geometry of subglacial bedforms, the spatial variation of basal melt, englacial temperature, and the transition between frozen and thawed bed. Planetary radar sounders have been used or are planned to observe the subsurface and near-surface conditions of Mars, Earth’s Moon, comets and the icy moons of Jupiter. These instruments provide critical subsurface context for surface-sensing, particle, and potential-field instruments in planetary exploration payloads. This symposium will discuss advances in radar-sounding systems, mission concepts, signal processing, data analysis, modeling and scientific interpretation.

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