AI-driven surface mapping and explainable AI for climate insights on Mars

We are deriving insights about the climate evolution of Mars by automating surface mapping and monitoring with AI models. We are also analysing these models’ uncertainty and decision-making process with explainable AI and uncertainty estimation techniques. We focus on ice block fall detection at the...

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Main Authors: Fanara, Lida, Su, Shu, Martynchuk, Oleksii, Hauber, Ernst, Gwinner, Klaus
Format: Conference Object
Language:English
Published: 2024
Subjects:
Online Access:https://elib.dlr.de/211452/
https://meetingorganizer.copernicus.org/EPSC2024/EPSC2024-948.html
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author Fanara, Lida
Su, Shu
Martynchuk, Oleksii
Hauber, Ernst
Gwinner, Klaus
author_facet Fanara, Lida
Su, Shu
Martynchuk, Oleksii
Hauber, Ernst
Gwinner, Klaus
author_sort Fanara, Lida
collection Unknown
description We are deriving insights about the climate evolution of Mars by automating surface mapping and monitoring with AI models. We are also analysing these models’ uncertainty and decision-making process with explainable AI and uncertainty estimation techniques. We focus on ice block fall detection at the north polar region and polygon detection globally. The north polar ice cap on Mars is comprised of ice layers relating to the climate cycles of Mars and this way it preserves a ∼ 4 million years climate change record of the planet. These layers are exposed at the marginal steep scarps of the cap, that are currently active with avalanches and block falls. We are monitoring the mass wasting activity at the north polar region by detecting ice blocks [1] and their sources [2]. We estimate the current erosion rates of all scarps resulting in a detailed map of how this extensive ice-layered dome is being shaped today. At the mid-latitude regions, where large volumes of excess ice exist, young patterned ground resembles glacial and periglacial patterns on Earth. Can freeze-thaw cycles have recently thawed the permafrost on Mars to produce these landforms? This would have implications for the recent hydrologic past of the planet. We detect young ice-wedge polygons to determine their distribution and relationship to the topography with the potential of elucidating the formation mechanism and the role of liquid water in the recent past of Mars. We use AI models to automate surface mapping and monitoring, because they outperform all other methods. However, they are treated as black box systems. We want to know why a model produces a specific response and how certain it is about the correctness of each result. To answer these questions, we put together an application-independent framework that deploys uncertainty estimation and explainable AI methods to provide insights into the decision-making process and assess the uncertainty of the results [3], in this project the uncertainty of the surface mapping.
format Conference Object
genre Ice
Ice cap
permafrost
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genre_facet Ice
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institution Open Polar
language English
op_collection_id ftdlr
op_doi https://doi.org/10.5194/epsc2024-948
op_relation https://elib.dlr.de/211452/1/EPSC2024-948-print.pdf
Fanara, Lida und Su, Shu und Martynchuk, Oleksii und Hauber, Ernst und Gwinner, Klaus (2024) AI-driven surface mapping and explainable AI for climate insights on Mars. Europlanet Science Congress 2024, 2024-09-08 - 2024-09-13, Berlin, Germany. doi:10.5194/epsc2024-948 <https://doi.org/10.5194/epsc2024-948>.
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spelling ftdlr:oai:elib.dlr.de:211452 2025-06-15T14:29:17+00:00 AI-driven surface mapping and explainable AI for climate insights on Mars Fanara, Lida Su, Shu Martynchuk, Oleksii Hauber, Ernst Gwinner, Klaus 2024 application/pdf https://elib.dlr.de/211452/ https://meetingorganizer.copernicus.org/EPSC2024/EPSC2024-948.html en eng https://elib.dlr.de/211452/1/EPSC2024-948-print.pdf Fanara, Lida und Su, Shu und Martynchuk, Oleksii und Hauber, Ernst und Gwinner, Klaus (2024) AI-driven surface mapping and explainable AI for climate insights on Mars. Europlanet Science Congress 2024, 2024-09-08 - 2024-09-13, Berlin, Germany. doi:10.5194/epsc2024-948 <https://doi.org/10.5194/epsc2024-948>. cc_by Planetengeodäsie Planetengeologie Konferenzbeitrag NonPeerReviewed 2024 ftdlr https://doi.org/10.5194/epsc2024-948 2025-06-04T04:58:08Z We are deriving insights about the climate evolution of Mars by automating surface mapping and monitoring with AI models. We are also analysing these models’ uncertainty and decision-making process with explainable AI and uncertainty estimation techniques. We focus on ice block fall detection at the north polar region and polygon detection globally. The north polar ice cap on Mars is comprised of ice layers relating to the climate cycles of Mars and this way it preserves a ∼ 4 million years climate change record of the planet. These layers are exposed at the marginal steep scarps of the cap, that are currently active with avalanches and block falls. We are monitoring the mass wasting activity at the north polar region by detecting ice blocks [1] and their sources [2]. We estimate the current erosion rates of all scarps resulting in a detailed map of how this extensive ice-layered dome is being shaped today. At the mid-latitude regions, where large volumes of excess ice exist, young patterned ground resembles glacial and periglacial patterns on Earth. Can freeze-thaw cycles have recently thawed the permafrost on Mars to produce these landforms? This would have implications for the recent hydrologic past of the planet. We detect young ice-wedge polygons to determine their distribution and relationship to the topography with the potential of elucidating the formation mechanism and the role of liquid water in the recent past of Mars. We use AI models to automate surface mapping and monitoring, because they outperform all other methods. However, they are treated as black box systems. We want to know why a model produces a specific response and how certain it is about the correctness of each result. To answer these questions, we put together an application-independent framework that deploys uncertainty estimation and explainable AI methods to provide insights into the decision-making process and assess the uncertainty of the results [3], in this project the uncertainty of the surface mapping. Conference Object Ice Ice cap permafrost wedge* Unknown
spellingShingle Planetengeodäsie
Planetengeologie
Fanara, Lida
Su, Shu
Martynchuk, Oleksii
Hauber, Ernst
Gwinner, Klaus
AI-driven surface mapping and explainable AI for climate insights on Mars
title AI-driven surface mapping and explainable AI for climate insights on Mars
title_full AI-driven surface mapping and explainable AI for climate insights on Mars
title_fullStr AI-driven surface mapping and explainable AI for climate insights on Mars
title_full_unstemmed AI-driven surface mapping and explainable AI for climate insights on Mars
title_short AI-driven surface mapping and explainable AI for climate insights on Mars
title_sort ai-driven surface mapping and explainable ai for climate insights on mars
topic Planetengeodäsie
Planetengeologie
topic_facet Planetengeodäsie
Planetengeologie
url https://elib.dlr.de/211452/
https://meetingorganizer.copernicus.org/EPSC2024/EPSC2024-948.html