A machine learning toolkit for CRISM image analysis

dc.contributor.authorPlebani, Emanuele
dc.contributor.authorEhlmann, Bethany L.
dc.contributor.authorLeask, Ellen K.
dc.contributor.authorFox, Valerie K.
dc.contributor.authorDundar, M. Murat
dc.contributor.departmentComputer and Information Science, School of Scienceen_US
dc.date.accessioned2023-03-09T19:28:22Z
dc.date.available2023-03-09T19:28:22Z
dc.date.issued2022-04
dc.description.abstractHyperspectral images collected by remote sensing have played a significant role in the discovery of aqueous alteration minerals, which in turn have important implications for our understanding of the changing habitability on Mars. Traditional spectral analyzes based on summary parameters have been helpful in converting hyperspectral cubes into readily visualizable three channel maps highlighting high-level mineral composition of the Martian terrain. These maps have been used as a starting point in the search for specific mineral phases in images. Although the amount of labor needed to verify the presence of a mineral phase in an image is quite limited for phases that emerge with high abundance, manual processing becomes laborious when the task involves determining the spatial extent of detected phases or identifying small outcrops of secondary phases that appear in only a few pixels within an image. Thanks to extensive use of remote sensing data and rover expeditions, significant domain knowledge has accumulated over the years about mineral composition of several regions of interest on Mars, which allow us to collect reliable labeled data required to train machine learning algorithms. In this study we demonstrate the utility of machine learning in two essential tasks for hyperspectral data analysis: nonlinear noise removal and mineral classification. We develop a simple yet effective hierarchical Bayesian model for estimating distributions of spectral patterns and extensively validate this model for mineral classification on several test images. Our results demonstrate that machine learning can be highly effective in exposing tiny outcrops of specific phases in orbital data that are not uncovered by traditional spectral analysis. We package implemented scripts, documentation illustrating use cases, and pixel-scale training data collected from dozens of well-characterized images into a new toolkit. We hope that this new toolkit will provide advanced and effective processing tools and improve community’s ability to map compositional units in remote sensing data quickly, accurately, and at scale.en_US
dc.eprint.versionFinal published versionen_US
dc.identifier.citationPlebani, E., Ehlmann, B. L., Leask, E. K., Fox, V. K., & Dundar, M. M. (2022). A machine learning toolkit for CRISM image analysis. Icarus, 376, 114849. https://doi.org/10.1016/j.icarus.2021.114849en_US
dc.identifier.urihttps://hdl.handle.net/1805/31790
dc.language.isoenen_US
dc.publisherElsevieren_US
dc.relation.isversionof10.1016/j.icarus.2021.114849en_US
dc.relation.journalIcarusen_US
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.sourcePublisheren_US
dc.subjectmachine learningen_US
dc.subjecthyperspectral imageen_US
dc.subjectMarsen_US
dc.titleA machine learning toolkit for CRISM image analysisen_US
dc.typeArticleen_US
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