International audienceRadar detection of subsurface ice on Mars has been widely debated in part because the dielectric signature of ice, as deduced from the dielectric constant, can be confused with dry-silicate-rich materials. To identify the ice dielectric signature, it is crucial to estimate the imaginary part of the dielectric permittivity inferred from the dielectric attenuation after removing the scattering loss. Unfortunately, the latter remains poorly quantified at both Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) and shallow subsurface radar SHARAD frequencies. To address this ambiguity, we conducted multiple-frequency ground-penetrating radar and resistivity investigations in well-characterized temperate pe...
[1] Signals from the Shallow Radar were intended to penetrate hundreds of meters or more into Mars, ...
Meridiani Planum is one of the most intensely studied regions on Mars, yet little is known about the...
The polar layered deposits are the largest reservoir of water on the surface of Mars. The physical p...
International audienceFor the last decade, the SHARAD radar on board NASA's Mars Reconnaissance Orbi...
Abstract P41B-1372The SHAllow RADar (SHARAD) is a subsurface sounding instrument aboard the NASA's M...
The nature of the materials underlying the superficial deposits of Mars can be inferred, applying an...
Ground penetrating radar measurements performed on the Greenland ice sheet show internal reflectors,...
The dielectric permittivity of glaciers and ice caps can be measured in field or airborne surveys us...
International audienceTo test the volcanic and fluvial hypotheses for the origin of the rafted plate...
Martian Polar Layered Deposits, most likely dusty ice are transparent to radar waves. In the North ...
Polygonal patterned ground and buried ice are features of the permafrost environments of Earth and M...
Several radar experiments are planned to map the martian subsurface down to several kilometers, sear...
Amazonis Planitia has undergone alternating episodes of sedimentary and volcanic infilling, forming ...
International audienceWe have undertaken laboratory electromagnetic characterization of the total se...
A 130 m long ice core has been dielectrically profiled. From an analysis of the measurements, we obt...
[1] Signals from the Shallow Radar were intended to penetrate hundreds of meters or more into Mars, ...
Meridiani Planum is one of the most intensely studied regions on Mars, yet little is known about the...
The polar layered deposits are the largest reservoir of water on the surface of Mars. The physical p...
International audienceFor the last decade, the SHARAD radar on board NASA's Mars Reconnaissance Orbi...
Abstract P41B-1372The SHAllow RADar (SHARAD) is a subsurface sounding instrument aboard the NASA's M...
The nature of the materials underlying the superficial deposits of Mars can be inferred, applying an...
Ground penetrating radar measurements performed on the Greenland ice sheet show internal reflectors,...
The dielectric permittivity of glaciers and ice caps can be measured in field or airborne surveys us...
International audienceTo test the volcanic and fluvial hypotheses for the origin of the rafted plate...
Martian Polar Layered Deposits, most likely dusty ice are transparent to radar waves. In the North ...
Polygonal patterned ground and buried ice are features of the permafrost environments of Earth and M...
Several radar experiments are planned to map the martian subsurface down to several kilometers, sear...
Amazonis Planitia has undergone alternating episodes of sedimentary and volcanic infilling, forming ...
International audienceWe have undertaken laboratory electromagnetic characterization of the total se...
A 130 m long ice core has been dielectrically profiled. From an analysis of the measurements, we obt...
[1] Signals from the Shallow Radar were intended to penetrate hundreds of meters or more into Mars, ...
Meridiani Planum is one of the most intensely studied regions on Mars, yet little is known about the...
The polar layered deposits are the largest reservoir of water on the surface of Mars. The physical p...