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.
Exploratory data analysis of planetary hyperspectral datasets - use of statistics to enhance mission science return
Details
Date
Wednesday, June 18 2008 - 12:00 pm, PDT
Speaker
Mario Parente
Affiliation
Department of Electrical Engineering, Stanford University and SETI Institute
Description
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