GC022-0015
Scene Invariants for Imaging Spectrometer Uncertainty Quantification

Tuesday, 8 December 2020
Poster
David R Thompson1, Urs Niklas Bohn2, Amy J Braverman3, Philip G Brodrick3, Nimrod Carmon1, Jay Fahlen1, Robert L Herman4, Jonathan Hobbs5, Robert O Green1, Maggie Johnson1, Jouni Susiluoto1 and Michael Turmon1, (1)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (2)Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences, Potsdam, Germany, (3)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (4)JPL, Pasadena, CA, United States, (5)Jet Propulsion Laboratory, Pasadena, CA, United States
Abstract:
Remote imaging spectroscopy investigations typically use Radiative Transfer Models (RTMs) to predict the measured radiance at the sensor given specific surface and atmosphere properties. Discrepancies between RTM model assumptions and physical reality can lead to subtle and systematic errors in derived measurements. We demonstrate an approach to characterize these model errors based on scene invariants - properties of the environment which are stable over time. Spatially and temporally invariant properties can disentangle different sources of retrieval variance, such as RTM model discrepancies and instrument noise. This allows investigators to estimate the aggregate uncertainty due to model discrepancies without having to explicitly identify them. The resulting distributions can be used to improve retrieval accuracy as well as the fidelity of posterior uncertainty predictions. We present the theoretical motivation for our approach, and initial results from a field dataset acquired by the AVIRIS-NG airborne imaging spectrometer.

Copyright 2020 California Institute of Technology. Government Support Acknowledged.