P016-0012
S-band Observations of the Aristarchus Plateau from the LRO Mini-RF Instrument
Abstract:
The Mini-RF instrument aboard NASA’s Lunar Reconnaissance Orbiter (LRO) is a hybrid-polarized, dual-frequency synthetic aperture radar (SAR) that operates in cooperation with the Arecibo Observatory (AO) to collect S-band (12.6 cm wavelength) bistatic radar measurements of the lunar nearside and poles. For each observation, the surface is illuminated with a circularly polarized, chirped signal that tracks the Mini-RF antenna boresight intercept on the surface of the Moon. The Mini-RF receiver operates continuously, separately receiving the horizontal and vertical polarization components of the signal backscattered from the lunar surface. In this architecture, the incidence angle varies as a function of the observation geometry and the data have a spatial resolution of ~100 m in range and ~2.5 m in azimuth. This can vary from one observation to another as a function of the viewing geometry. The data are coherently processed onto grids with a spacing of 4 m along track and 25 m cross track. For analysis, they are then incoherently reduced to a uniform 100 m grid yielding approximately a 25-look average for each sampled location.
Four Mini-RF S-band bistatic observations of the Aristarchus Plateau, spanning a range of bistatic angles, have been acquired over the course of 2 different observation campaigns. These data are providing unique insights into the local geology, related to cratering and volcanic processes.