Hyperspectral instruments (HSIs) measure the electromagnetic energy emitted by materials at high resolution (hundreds to thousands of channels) enabling material identification through spectroscopic analysis. Laser-induced breakdown spectroscopy (LIBS) is used by the ChemCam instrument on the Curiosity rover to measure the emission spectra of surface materials on Mars. From orbit, hyperspectral instruments (HSIs) on the CRISM instrument of the Mars Reconnaissance Orbiter (MRO) measure the electromagnetic energy emitted by materials at high resolution (hundreds to thousands of channels) enabling material identification through spectroscopic analysis. The data received are noisy, high-dimensional, and largely unlabeled. The ability to accurately predict elemental and material compositions of surface samples as well as to simulate spectra from hypothetical compositions, collectively known as hyperspectral unmixing, is invaluable to the exploration process. The nature of the problem allows us to construct deep (semi-supervised) generative models to accomplish both these tasks while making use of a large unlabeled dataset. Our main technical contribution is an invertibility trick where we train our model in reverse.
['Ian Gemp', 'Ishan P. Durugkar', 'Mario Parente', 'M. Darby Dyar', 'Sridhar Mahadevan']
Deep Generative Models for Spectroscopic Analysis on Mars