by Mario Parente, Department of Electrical Engineering, Stanford University and SETI Institute
Mario Parente will describe the latest developments in statistical
analysis of hyperspectral images, describing his efforts to enhance the
science return of the CRISM infrared spectrometer using a multi-stage
denoising technique. He will describe how it is possible to model the
CRISM instrument and efforts currently ongoing that involve
investigations of surface minerals at Juventae Chasma and Mawrth Valles
on the surface of Mars.
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